#: locale=en

## Action

### Text to Speech
TextToSpeechBehaviour_DDD8D7A8_DA85_C174_41E0_F925DA55388D.text =  Sirius  \
brightest star in the night sky
TextToSpeechBehaviour_DC45C5CF_D98F_C0CD_41D4_9094ACF3012B.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
TextToSpeechBehaviour_3F222A6C_4136_2D25_41CA_28C6EF87E8C2.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
TextToSpeechBehaviour_DB796D98_DF84_C153_41D0_C0CF37B99956.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
TextToSpeechBehaviour_DD6EA468_DB9C_47F3_41EA_3C7C90545883.text = Active Surface \
The UArizona 12-meter Telescope has an active surface. Actuators maintain the parabolic shape of the dish to keep the telescope focused accurately. 
TextToSpeechBehaviour_DDDE2E62_DABC_43F4_41C4_53DB9C5A78C6.text = Aldebaran
TextToSpeechBehaviour_DDDA8EC2_DA84_4334_41DD_336E8FAA8DC9.text = Betelgeuse
TextToSpeechBehaviour_0E60CCF1_2939_2052_41B8_548324F4077C.text = Burrell Schmidt Telescope
TextToSpeechBehaviour_A8DD46A7_D68C_437D_41E7_7522ADB02BCB.text = Calibration Screen \
The calibration screen is illuminated with light sources with known properties to help astronomers to properly calibrate their images and spectra. 
TextToSpeechBehaviour_DC119C22_D984_4774_41E1_41DA0CBF2679.text = Calibration screen \
The calibration screen is used for astro imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects. 
TextToSpeechBehaviour_DE50D871_D985_CFD4_41D3_CD3D1723B2D0.text = Calibration screen \
The calibration screen is used for astro-imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects. 
TextToSpeechBehaviour_DDDDEBF4_DABF_C0DC_41D3_12D37D837442.text = California Nebula
TextToSpeechBehaviour_C125E139_D244_381E_41E8_BE8709CD76D9.text = Calypso 1.2-meter Telescope
TextToSpeechBehaviour_DDD73AB9_DA8C_4354_41DA_8A43706BEDA4.text = Canopus
TextToSpeechBehaviour_DDDEE91E_DABD_C14C_41B9_3F965ACD0AAD.text = Capella
TextToSpeechBehaviour_A57D7C16_D1C4_C813_41D2_A6936B404347.text = Dorm 1 \
 \
Several dorms on Kitt Peak allow astronomers to spend the night during their observing runs.
TextToSpeechBehaviour_F3D27885_D1C4_48F1_41D9_5F4A7DBF40C3.text = Eclipsed Moon \
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 The totally eclipsed Moon shows up next to the Mayall Telescope.
TextToSpeechBehaviour_FBF2799B_D1FC_C812_41E5_4C5247767A1F.text = Eclipsed Moon \
 \
The totally eclipsed Moon shows up below the McMath-Pierce Solar Telescope. 
TextToSpeechBehaviour_DDDE6EC6_DABC_C33F_41D5_5DD9A9656FCF.text = Flaming star nebula
TextToSpeechBehaviour_DD43D63B_DB8B_C354_41CB_C5F500DDE419.text = Gegenschein \
Click here to learn more
TextToSpeechBehaviour_1E76404B_41F2_3D63_41A5_646561FFE4BF.text = Go to Admin Building
TextToSpeechBehaviour_DD69C33E_DB87_C14C_41AA_D4EC60A560BC.text = Go to Hiltner 2.4 meter Telescope
TextToSpeechBehaviour_DE3E6279_D9FC_C3D4_41E2_BCE7F9CD2B64.text = Go to Hiltner 2.4-meter Telescope
TextToSpeechBehaviour_6103E6D8_2B19_6052_41BF_E8AD519A5F1E.text = Go to Hiltner 2.4-meter Telescope
TextToSpeechBehaviour_2808B210_4152_5CFD_41CB_AE134FA8EDA4.text = Go to Interior of the Mayall
TextToSpeechBehaviour_2BA4C011_DA8C_7F57_41C8_5BBA77246454.text = Go to Interior of the Mayall
TextToSpeechBehaviour_75F00478_D98C_47D4_41B6_DF3F11E3BA8F.text = Go to Interior of the Mayall
TextToSpeechBehaviour_CE9DDFBE_D79C_414F_41D5_97A23BCA50CD.text = Go to KPNO Admin Building
TextToSpeechBehaviour_DC12A7EF_D984_40CD_41DC_594EEAEE4565.text = Go to KPNO Admin Building
TextToSpeechBehaviour_454EDD4D_43CE_6767_41AF_8F819633390C.text = Go to KPNO Drone View
TextToSpeechBehaviour_452B391B_4376_2CE2_41C1_C79CD783B188.text = Go to KPNO Drone View
TextToSpeechBehaviour_4535EB16_4352_2CE4_41C6_BF0514D1D946.text = Go to KPNO Drone View
TextToSpeechBehaviour_45381821_4351_ECDF_41AA_4E8D0332F6DD.text = Go to KPNO Drone View
TextToSpeechBehaviour_4544C271_4332_5D3F_41D0_7C6BFAD6E24F.text = Go to KPNO Drone View
TextToSpeechBehaviour_451FE67B_434E_2523_41C6_7E9B3E25DAA3.text = Go to KPNO Drone View
TextToSpeechBehaviour_4542412A_4336_5F2D_41D0_65A426DBCCE9.text = Go to KPNO Drone View
TextToSpeechBehaviour_4531FB15_4352_2CE7_41C0_1EAD60F57F9A.text = Go to KPNO Drone View
TextToSpeechBehaviour_452622A8_4371_DD2D_41C5_4F3787E02DD2.text = Go to KPNO Drone View
TextToSpeechBehaviour_1DBB4A55_41DE_6D64_41B7_159206974E30.text = Go to Kitt Peak 2.1-m Telescope Interior
TextToSpeechBehaviour_B7E1E510_38FB_4F9F_41C4_1BBF83D7188D.text = Go to Kitt Peak 2.1-m Telescope Interior
TextToSpeechBehaviour_DB9CA4D2_DEBC_40D4_41BA_05043AECCF1C.text = Go to Kitt Peak 2.1-meter Telescope Interior
TextToSpeechBehaviour_DC4456A0_D98C_C373_41D1_1AC563EF000C.text = Go to Kitt Peak 2.1-meter Telescope Interior
TextToSpeechBehaviour_FD912219_D7FC_4355_41D6_7088D724F6B6.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_7B653385_2B09_20B2_41C1_ADCB9C8AC87B.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_D8F5215F_DA8C_41CC_41C8_E12BA96F9612.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_DC43CF12_D98B_C157_41E0_5428EF21B8F8.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_DDE92073_DA84_7FD5_41E4_C22837B3DC09.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_79C04D46_DA84_C13F_41E2_AE3440702DA3.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_B7E38516_38FB_4F83_41C4_D3D615EF695F.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_0AB1AE4C_4171_E565_41C3_570A803EA01D.text = Go to Kitt Peak Visitor Center
TextToSpeechBehaviour_5157D820_D68B_CF74_41D2_EEDE0BE4C805.text = Go to Mayall  Exterior
TextToSpeechBehaviour_2A714E31_386B_D667_41CB_9AB1BE5BCB98.text = Go to Mayall At Night
TextToSpeechBehaviour_780BA7AF_2B09_60CE_41AD_A6A9F88168E0.text = Go to Mayall Exterior
TextToSpeechBehaviour_6D2C16F3_D99D_C0D5_41E2_5C6253632202.text = Go to Mayall Exterior
TextToSpeechBehaviour_38C35261_2906_E072_41AC_C71990256696.text = Go to Mayall Exterior
TextToSpeechBehaviour_3438B52C_4132_2724_4182_256304AA53F7.text = Go to Mayall Exterior
TextToSpeechBehaviour_DDC9A0A5_DA84_7F7C_41EA_4D9DA3CC5854.text = Go to Mayall Exterior
TextToSpeechBehaviour_6D5B143C_2B09_27D2_41B1_5F955FD79089.text = Go to Mayall Exterior
TextToSpeechBehaviour_582D27C5_2909_20B2_41BB_DEECBB05B3CD.text = Go to Mayall Exterior
TextToSpeechBehaviour_59CBD1F5_2919_E052_41BB_657C469ED830.text = Go to Mayall With Zodiacal Light
TextToSpeechBehaviour_28D7EAA0_4152_EDDD_41D0_C5DE20BC65D7.text = Go to Mayall at Night
TextToSpeechBehaviour_91D6CA90_2919_60D2_41B8_CA426B891CDD.text = Go to Mayall at Night
TextToSpeechBehaviour_DE2FDB66_D99B_C1FC_41D1_EAF909367CAF.text = Go to McGraw-Hill 1.3-meter Telescope
TextToSpeechBehaviour_4667B9C2_2B19_20B7_419B_542373601396.text = Go to McGraw-Hill 1.3-meter Telescope
TextToSpeechBehaviour_134182DB_4132_5D63_41BD_A9076641C4D5.text = Go to McMath-Pierce Exterior
TextToSpeechBehaviour_9231F7B3_290A_E0D6_41C0_B56B95675770.text = Go to McMath-Pierce Exterior
TextToSpeechBehaviour_06D5F79D_2919_60D2_41B7_66F3585C3259.text = Go to McMath-Pierce Exterior
TextToSpeechBehaviour_129BB7B3_4132_6323_41CB_DC72EBE9FB68.text = Go to McMath-Pierce Roof
TextToSpeechBehaviour_D8CCEDA5_DA9D_C17C_41E5_FBF2F9093AC7.text = Go to McMath-Pierce Roof 
TextToSpeechBehaviour_DC453F0C_D98C_4133_41D2_3658454F80BF.text = Go to McMath-Pierce Roof 
TextToSpeechBehaviour_DDE1DE54_DA87_C3D3_41D7_0DF49CF33E0F.text = Go to McMath-Pierce Solar Telescope Exterior
TextToSpeechBehaviour_DC11F71B_D987_C155_41EB_2E6AF550B073.text = Go to McMath-Pierce Solar Telescope Exterior
TextToSpeechBehaviour_CE6E8BED_D784_C0CD_41E8_D634C419CABD.text = Go to McMath-Pierce Solar Telescope Exterior
TextToSpeechBehaviour_6488D156_38EB_4783_41C0_0535DC17044B.text = Go to McMath-Pierce at Night
TextToSpeechBehaviour_DC4335D4_D984_40DC_41DD_91B5B8B2C65E.text = Go to McMath-Pierce at night
TextToSpeechBehaviour_DD230D0C_DB84_414C_41CE_241CFC181703.text = Go to Milkyway Over Kitt Peak
TextToSpeechBehaviour_AA8C3F86_2939_20BE_41C3_1C8EBF39FCA5.text = Go to Milkyway Over Kitt Peak
TextToSpeechBehaviour_DD770479_DB8C_47D5_41C9_BC3E967C196E.text = Go to Milkyway Over Kitt Peak
TextToSpeechBehaviour_E63595AA_290A_E0F6_41B2_05460CEABC8A.text = Go to Roll Off Roof Observatory
TextToSpeechBehaviour_251319E5_41D2_2F27_41CD_7F1BD5BFE053.text = Go to Roll Off Roof Observatory
TextToSpeechBehaviour_E9086D3E_2906_E1CE_41A6_AFCCDCFF1F2E.text = Go to Roll Off Roof Observatory
TextToSpeechBehaviour_DD19E692_DB87_C357_41CC_D5CF3C858053.text = Go to SARA Kitt Peak Telescope
TextToSpeechBehaviour_2095B930_387B_DA65_41A3_107AB7411918.text = Go to SARA Kitt Peak Telescope
TextToSpeechBehaviour_1E11CC22_41F2_E4DC_41CF_7F006291285F.text = Go to SARA Kitt Peak Telescope
TextToSpeechBehaviour_D8EA5BEC_DA84_C0CC_41E3_4A37F9E33405.text = Go to Total Lunar Eclipse
TextToSpeechBehaviour_2A712E37_386B_D66B_41C0_70E8DA791FD5.text = Go to Total Lunar Eclipse
TextToSpeechBehaviour_DDD02EE4_DA84_40F3_41EA_30C8C7E33A75.text = Go to Total Lunar Eclipse
TextToSpeechBehaviour_6B85793B_2B09_E1D6_41AD_FAF425CB442A.text = Go to UArizona 0.9-meter Telescope
TextToSpeechBehaviour_D908B97E_DB84_41CF_41D1_539BECE1EF60.text = Go to UArizona 0.9-meter Telescope
TextToSpeechBehaviour_217836EA_4172_652D_41B8_D3B7ED43E142.text = Go to UArizona 0.9m Telescope
TextToSpeechBehaviour_22170420_4172_24DD_41CD_647B82643325.text = Go to UArizona 12-m Telescope
TextToSpeechBehaviour_76AB5B13_2B7A_E1D6_41B1_7A3DC7767E61.text = Go to UArizona 12-meter Telescope
TextToSpeechBehaviour_DE032D9A_D984_4154_41E2_ED5BD0223320.text = Go to UArizona 12-meter Telescope
TextToSpeechBehaviour_2E5F1765_4152_6327_419A_C86D61EC80F2.text = Go to UArizona Bok 2.3-m Telescope
TextToSpeechBehaviour_13C010C1_2B1F_20B2_4199_137FA6A2ABA0.text = Go to UArizona Bok 2.3-meter Telescope
TextToSpeechBehaviour_D8D5CBF5_DA8F_C0DC_41DD_6E3E3FAC72A3.text = Go to UArizona Bok 2.3-meter Telescope
TextToSpeechBehaviour_23A1C4AA_4172_652D_41BE_4B111531ABA4.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_CFBF9D82_D784_C137_4194_48D9EC1BE003.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_DD5A8486_DB84_473C_41DE_9A07ADAF59AA.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_DE3496AB_D98C_4374_41B3_B9563F193AC0.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_D8EE90E3_DA9C_40F5_41EA_37A85D97A556.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_DE4D01E7_D99C_40FD_41CD_B72215519682.text = Go to Very Long Baseline Array Dish
TextToSpeechBehaviour_4208C737_DA84_C15C_41D5_6B36F2767729.text = Go to Visitor Center 0.5-meter Telescope
TextToSpeechBehaviour_DDF31A26_DA84_437A_41E7_2726F3048A29.text = Go to Visitor Center 0.5-meter Telescope
TextToSpeechBehaviour_CE8F0E50_D79C_43D3_41D9_009644B13FE1.text = Go to Visitor Center 0.5-meter Telescope
TextToSpeechBehaviour_CE3C741D_D784_C74D_41B5_A10EB47B4FDC.text = Go to Visitor Center Interior
TextToSpeechBehaviour_FB68CAC8_D7FC_C333_41DD_1E0112826314.text = Go to Visitor Center Interior
TextToSpeechBehaviour_0F71180F_2909_EFCE_41C2_447B961A6311.text = Go to WIYN 3.5-meter Telescope Interior
TextToSpeechBehaviour_D8F43B8C_DA8C_4133_41E1_19344B6FC6E8.text = Go to WIYN 3.5-meter Telescope Interior
TextToSpeechBehaviour_255B999A_4172_2FED_41B5_9F57E5605775.text = Go to WIYN Telescopes Exterior
TextToSpeechBehaviour_5F9FD0F4_D68C_C0D3_41D7_9DF94ABCF9BB.text = Go to desi Control Room
TextToSpeechBehaviour_09DF9B6F_DAFC_C1CD_41E8_F68468E7137D.text = Go to desi Control Room
TextToSpeechBehaviour_CF0E823B_D784_C355_41DD_E5408745A286.text = Go to solario
TextToSpeechBehaviour_E5BACD02_D784_4137_41CC_68B07980A61D.text = Go to solario
TextToSpeechBehaviour_DB78AD7F_DF84_41CD_416C_01CDF1DE0F7C.text = Go to wiyn 3.5-meter Telescope Interior
TextToSpeechBehaviour_DC133668_D984_43F3_41E3_33536F4FBC95.text = Go to wyin Telescopes Exterior
TextToSpeechBehaviour_DDD789F4_DA8C_40DC_41DC_099BA735534F.text = Gum Nebula
TextToSpeechBehaviour_03F97B47_297B_61BE_4179_B6DE3B47386E.text = Heliostats \
The three heliostats reflect light to the primary mirrors. 
TextToSpeechBehaviour_DDDAD1AC_DA85_C173_41D4_88567B58E6C2.text = Horsehead Nebula 
TextToSpeechBehaviour_DDE09B74_DA84_41DC_41E4_02BAFEA4878A.text = Interior of the Mayall
TextToSpeechBehaviour_85988AB2_D1C4_4813_41BD_29140B03B429.text = KPNO 2.1-meter Telescope
TextToSpeechBehaviour_E6CF553D_D1C4_3811_41DC_1216DB061C07.text = Light Pollution from Phoenix, Arizona
TextToSpeechBehaviour_DDDBE84B_DABB_CF35_41D8_CF559CEAE0FC.text = Light pollution from Tucson. \
Click here for more info
TextToSpeechBehaviour_E6E83CF3_C7E6_4E08_41DD_6EDFFD0752FD.text = McMath-Pierce Solar Telescope \
For many years the largest solar telescope in the world, the iconic McMath-Pierce Solar Telescope, is a triple telescope. In addition to the primary 1.61-meter mirror fed by the 2.03-meter heliostat, there are a pair of telescopes fed by 0.81-meter heliostats mounted beside the main heliostat. These two instruments have 1.07-meter and 0.91-meter primary mirrors. The telescope used the heliostat at the top of its main tower to direct the Sun’s light down a long shaft to the primary mirrors. The distinctive diagonal shaft continues far underground, where the telescope’s primary mirror is located.  \
 \
The facility is named to honor astronomers Keith Pierce and Robert McMath. \
 \
Scientific research stopped at the McMath-Pierce Solar Telescope in 2017 and it now houses the noirlab Windows on the Universe Center for Astronomy Outreach.
TextToSpeechBehaviour_D98234E6_C7E2_5E08_41DB_ACB41371571A.text = McMath-Pierce Solar Telescope \
For many years the largest solar telescope in the world, the iconic McMath-Pierce Solar Telescope, is a triple telescope. In addition to the primary 1.61-meter mirror fed by the 2.03-meter heliostat, there are a pair of telescopes fed by 0.81-meter heliostats mounted beside the main heliostat. These two instruments have 1.07-meter and 0.91-meter primary mirrors. The telescope used the heliostat at the top of its main tower to direct the Sun’s light down a long shaft to the primary mirrors. The distinctive diagonal shaft continues far underground, where the telescope’s primary mirror is located.  \
 \
The facility is named to honor astronomers Keith Pierce and Robert McMath. \
 \
Scientific research stopped at the McMath-Pierce Solar Telescope in 2017 and it now houses the noirlab Windows on the Universe Center for Astronomy Outreach.
TextToSpeechBehaviour_E69804EB_C7E6_3E18_41C7_B847A659B427.text = McMath-Pierce Solar Telescope \
For many years the largest solar telescope in the world, the iconic McMath-Pierce Solar Telescope, is a triple telescope. In addition to the primary 1.61-meter mirror fed by the 2.03-meter heliostat, there are a pair of telescopes fed by 0.81-meter heliostats mounted beside the main heliostat. These two instruments have 1.07-meter and 0.91-meter primary mirrors. The telescope used the heliostat at the top of its main tower to direct the Sun’s light down a long shaft to the primary mirrors. The distinctive diagonal shaft continues far underground, where the telescope’s primary mirror is located.  \
 \
The facility is named to honor astronomers Keith Pierce and Robert McMath. \
 \
Scientific research stopped at the McMath-Pierce Solar Telescope in 2017 and it now houses the noirlab Windows on the Universe Center for Astronomy Outreach.
TextToSpeechBehaviour_DDF733B3_DA8C_4154_41DF_2106B6BAF153.text = Model of McMath-Pierce Solar Telescope \
This cutaway model of the McMath-Pierce Solar Telescope shows the optical path that light takes through the facility and shows the underground portion of the telescope. 
TextToSpeechBehaviour_C2235FE1_D25B_C831_41E8_69EC0861E1F2.text = Nicholas U. Mayall 4-meter Telescope
TextToSpeechBehaviour_DD20E74C_DB85_C1CC_41CA_0356A57AC4DC.text = Nicholas U. Mayall 4-meter Telescope \
It is the largest optical telescope on Kitt Peak. The Mayall telescope currently hosts the Department of Energy’s Dark Energy Spectroscopic Instrument (desi), the most powerful multi-object survey spectrograph in the world. 
TextToSpeechBehaviour_DC429591_D984_4155_41DB_D6836F6888BF.text = Optical Tunnel \
The heliostat (mirror) at the top of the telescope reflects light down the optical tunnel. Less than half of the optical tunnel is visible as it extends approximately another 90 meters (300 feet) underground!
TextToSpeechBehaviour_55D0EAA8_D68C_C373_41E3_3F0461165E52.text = Original Control Room \
This control room was used until the installation of the DESI instrument and the construction of the DESI control room. This control room is still used for testing and engineering. 
TextToSpeechBehaviour_DDDB1749_DA84_4134_41A8_350517500297.text = Orion Nebula
TextToSpeechBehaviour_DDDD2445_DABC_473D_41E9_EA5BBF0D5CA5.text = Pleiades 
TextToSpeechBehaviour_DDDC3E1A_DABC_4357_41D5_5EECB56A53B2.text = Polaris
TextToSpeechBehaviour_DDD96B54_DA84_C1DC_41E6_3EF83420E4CC.text = Procyon
TextToSpeechBehaviour_DDDB7B77_DA84_C1DD_41C4_A8F1D20EC87B.text = Regulus
TextToSpeechBehaviour_0070BE17_2909_23DE_41AD_A235159E6B9A.text = Robotically Controlled Telescope
TextToSpeechBehaviour_DDD9E06F_DA87_FFCC_4174_2834CD6E01C5.text = Rosette Nebula
TextToSpeechBehaviour_DDDA71DA_DA84_C0D4_41E9_626B34B13DBD.text = Rosette Nebula
TextToSpeechBehaviour_0DD102B1_291A_E0D2_418D_B6F727B7DDAB.text = SARA Kitt Peak Telescope
TextToSpeechBehaviour_DDD84504_DA84_C13C_41E7_E9E40962FCAE.text = Seagull Nebula
TextToSpeechBehaviour_DD2188DB_DB84_40D5_41EA_72576518FBBC.text = Sells, Arizona \
 Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land.
TextToSpeechBehaviour_92526521_D1DC_7831_41E5_C1CF0EB35CB9.text = Sells, Arizona \
capital of Tohono O’odham Nation
TextToSpeechBehaviour_75918462_DA8B_C7F7_41C6_75AAB2A43D04.text = Solar viewing area \
Three solar telescopes are located around the corner which allow visitors to view the Sun through several filters, including white-light, hydrogen-alpha, and calcium-K. 
TextToSpeechBehaviour_A457A663_B9EC_00E0_41D0_CA7A864CCE9E.text = Spacewatch is the name of a group,founded by Tom Gehrels and Robert S. McMillan in 1980, at the University of Arizona’s Lunar and Planetary Laboratory. Today, Spacewatch is led by Dr. Melissa Brucker. The original goal of Spacewatch was to explore the various populations of small objects in the Solar System, and study the statistics of asteroids and comets in order to investigate the dynamical evolution of the Solar System. Since 1998, Spacewatch has focused primarily on follow-up astrometry of such targets, and especially monitors the positions and motions of objects that might present a hazard to Earth.
TextToSpeechBehaviour_A57920DC_B9A4_05A9_41DE_217813C80170.text = Spacewatch is the name of a group,founded by Tom Gehrels and Robert S. McMillan in 1980, at the University of Arizona’s Lunar and Planetary Laboratory. Today, Spacewatch is led by Dr. Melissa Brucker. The original goal of Spacewatch was to explore the various populations of small objects in the Solar System, and study the statistics of asteroids and comets in order to investigate the dynamical evolution of the Solar System. Since 1998, Spacewatch has focused primarily on follow-up astrometry of such targets, and especially monitors the positions and motions of objects that might present a hazard to Earth.
TextToSpeechBehaviour_A57940DD_B9A4_05AB_41C9_30DC5E3021E3.text = Spacewatch is the name of a group,founded by Tom Gehrels and Robert S. McMillan in 1980, at the University of Arizona’s Lunar and Planetary Laboratory. Today, Spacewatch is led by Dr. Melissa Brucker. The original goal of Spacewatch was to explore the various populations of small objects in the Solar System, and study the statistics of asteroids and comets in order to investigate the dynamical evolution of the Solar System. Since 1998, Spacewatch has focused primarily on follow-up astrometry of such targets, and especially monitors the positions and motions of objects that might present a hazard to Earth.
TextToSpeechBehaviour_CDB1DCBA_D1BC_4812_41EA_2C8816D8417D.text = Support Building
TextToSpeechBehaviour_D6F4211C_C862_5638_41E6_4F73CCA45131.text = The DESI Control Room was constructed in conjunction with the installation of the Department of Energy’s Dark Energy Spectroscopic Instrument (DESI). The DESI Control Room is currently used to control the telescope and acquire data with DESI (the original control room can be used for testing and engineering purposes). \

TextToSpeechBehaviour_D5E47E77_C866_CA08_41D9_0E5A7A2252F9.text = The DESI Control Room was constructed in conjunction with the installation of the Department of Energy’s Dark Energy Spectroscopic Instrument (DESI). The DESI Control Room is currently used to control the telescope and acquire data with DESI (the original control room can be used for testing and engineering purposes). \

TextToSpeechBehaviour_D600551D_C862_5E38_41D4_1E724D40C854.text = The DESI Control Room was constructed in conjunction with the installation of the Department of Energy’s Dark Energy Spectroscopic Instrument (DESI). The DESI Control Room is currently used to control the telescope and acquire data with DESI (the original control room can be used for testing and engineering purposes). \

TextToSpeechBehaviour_A99F3F80_B964_1B9A_41E7_17BE0CFC9C96.text = The Hiltner 2.4-meter Telescope is operated by a consortium of universities including Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. This telescope performs galactic surveys. 
TextToSpeechBehaviour_A92857C2_B964_0B99_41D6_D91BBA1232DB.text = The Hiltner 2.4-meter Telescope is operated by a consortium of universities including Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. This telescope performs galactic surveys. 
TextToSpeechBehaviour_A8C32083_B964_059F_41E0_36FF295CB5E7.text = The Hiltner 2.4-meter Telescope is operated by a consortium of universities including Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. This telescope performs galactic surveys. 
TextToSpeechBehaviour_D3FC4E29_C8AF_CA18_41DA_49891E71561C.text = The KPNO 2.1-meter Telescope was one of the earliest Kitt Peak telescopes and is used for both imaging and spectroscopy. It is paired with the Coudé Tower (now retired), which enabled spectroscopic work to be performed independently of the main telescope, effectively making the 2.1-meter telescope a dual observing facility. 
TextToSpeechBehaviour_D057AFD4_C8A3_CA08_41D4_79AA79FFC868.text = The KPNO 2.1-meter Telescope was one of the earliest Kitt Peak telescopes and is used for both imaging and spectroscopy. It is paired with the Coudé Tower (now retired), which enabled spectroscopic work to be performed independently of the main telescope, effectively making the 2.1-meter telescope a dual observing facility. 
TextToSpeechBehaviour_D3CE02B7_C8AF_DA08_41DA_E2EBC756E3C2.text = The KPNO 2.1-meter Telescope was one of the earliest Kitt Peak telescopes and is used for both imaging and spectroscopy. It is paired with the Coudé Tower (now retired), which enabled spectroscopic work to be performed independently of the main telescope, effectively making the 2.1-meter telescope a dual observing facility. 
TextToSpeechBehaviour_9D8563D7_B964_002F_41CD_4D3F96A8F468.text = The Kitt Peak Administration Building houses offices for Kitt Peak administrative staff and the Kitt Peak Associate Director. The Robotically Controlled Telescope (RCT) is attached to the east side of the Administration Building (here obscured by trees) and operated by a consortium led by Western Kentucky University. Dorm 1 can be seen on the far right side of the image. 
TextToSpeechBehaviour_9D8503D9_B964_0023_41E0_7711733B1E0E.text = The Kitt Peak Administration Building houses offices for Kitt Peak administrative staff and the Kitt Peak Associate Director. The Robotically Controlled Telescope (RCT) is attached to the east side of the Administration Building (here obscured by trees) and operated by a consortium led by Western Kentucky University. Dorm 1 can be seen on the far right side of the image. 
TextToSpeechBehaviour_9D8653D6_B964_0021_41D6_17271A76FD3C.text = The Kitt Peak Administration Building houses offices for Kitt Peak administrative staff and the Kitt Peak Associate Director. The Robotically Controlled Telescope (RCT) is attached to the east side of the Administration Building (here obscured by trees) and operated by a consortium led by Western Kentucky University. Dorm 1 can be seen on the far right side of the image. 
TextToSpeechBehaviour_A8061B00_B96C_049A_41C9_2F5AAB32C613.text = The Kitt Peak Visitor Center (KPVC) is the first place visitors go upon arrival at the summit. The KPVC contains exhibits on astronomy, Kitt Peak, and the Tohono O’odham Nation. The gift shop contains a variety of Kitt Peak merchandise and Tohono O’odham art. 
TextToSpeechBehaviour_A9A68AC9_B964_05AB_41E4_49E1A33BBAC0.text = The Kitt Peak Visitor Center (KPVC) is the first place visitors go upon arrival at the summit. The KPVC contains exhibits on astronomy, Kitt Peak, and the Tohono O’odham Nation. The gift shop contains a variety of Kitt Peak merchandise and Tohono O’odham art. 
TextToSpeechBehaviour_A8891DB3_B96C_7FFF_41E1_AC75BA312B07.text = The Kitt Peak Visitor Center (KPVC) is the first place visitors go upon arrival at the summit. The KPVC contains exhibits on astronomy, Kitt Peak, and the Tohono O’odham Nation. The gift shop contains a variety of Kitt Peak merchandise and Tohono O’odham art. 
TextToSpeechBehaviour_DCF4A5DF_42F6_2763_4197_EB73DE81CBB2.text = The Kitt Peak Visitor Center is the first stop for visitors to Kitt Peak. The Visitor Center has displays outlining the history of Kitt Peak and astronomy, and a gift shop that features an outstanding selection of Tohono O'odham baskets and art. Tours and nightly programs begin at the Visitor Center. 
TextToSpeechBehaviour_EB54F925_C861_D608_41AA_97FB129B45F7.text = The Kitt Peak Visitor Center is the first stop for visitors to Kitt Peak. The Visitor Center has displays outlining the history of Kitt Peak and astronomy, and a gift shop that features an outstanding selection of Tohono O'odham baskets and art. Tours and nightly programs begin at the Visitor Center. 
TextToSpeechBehaviour_EA54C95F_C863_D639_41A6_D7D41980DE7B.text = The Kitt Peak Visitor Center is the first stop for visitors to Kitt Peak. The Visitor Center has displays outlining the history of Kitt Peak and astronomy, and a gift shop that features an outstanding selection of Tohono O'odham baskets and art. Tours and nightly programs begin at the Visitor Center. 
TextToSpeechBehaviour_A9119E97_B828_EBD7_41DB_ABAA4A538D12.text = The McGraw-Hill 1.3-meter Telescope is part of the MDM Observatory, which is owned and operated by a consortium of five educational institutions — Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. The telescope was moved to Kitt Peak in 1975. The asteroid 4432 McGraw-Hill is named after this telescope.
TextToSpeechBehaviour_AA3D231D_B827_5ADB_41AF_8CC84CAADAA5.text = The McGraw-Hill 1.3-meter Telescope is part of the MDM Observatory, which is owned and operated by a consortium of five educational institutions — Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. The telescope was moved to Kitt Peak in 1975. The asteroid 4432 McGraw-Hill is named after this telescope.
TextToSpeechBehaviour_A8EC73E1_B839_596B_4186_7A1D7FD0C1A1.text = The McGraw-Hill 1.3-meter Telescope is part of the MDM Observatory, which is owned and operated by a consortium of five educational institutions — Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. The telescope was moved to Kitt Peak in 1975. The asteroid 4432 McGraw-Hill is named after this telescope.
TextToSpeechBehaviour_D70D193C_C866_D678_41C0_C7ADEC534D41.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
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noirlab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
TextToSpeechBehaviour_E94DF558_C87E_5E38_41D1_B5FF48BBC49B.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
 \
noirlab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
TextToSpeechBehaviour_AD20EF0E_D68B_C14F_41D1_34D1B99D3E58.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
 \
noirlab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
TextToSpeechBehaviour_AE36E43D_D68B_C74D_41A1_A633EB4C1232.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
 \
noirlab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
TextToSpeechBehaviour_E95E8181_C87E_5608_41E0_728B72496F6B.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
 \
noirlab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
TextToSpeechBehaviour_CE79F872_D78C_CFD7_41D0_DE37AE63D759.text = The Robotically Controlled Telescope \
The telescope has been operated by the RCT Consortium, led by Western Kentucky University since 2006. 
TextToSpeechBehaviour_C6487345_D25D_F871_41CA_68CF4EABBF56.text = The Spacewatch 0.9-meter Telescope is the oldest telescope on Kitt Peak. It was installed in 1923 on the University of Arizona campus and houses the first large telescope mirror successfully cast in the United States. The telescope was then moved to Kitt Peak in 1962.
TextToSpeechBehaviour_D458167F_C7FE_3AF8_41AD_D17E4A405071.text = The UArizona 12-meter Telescope was previously a European prototype antenna for the Atacama Large Millimeter/submillimeter Array (alma). Originally from the European Southern Observatory, it was transported to the Kitt Peak National Observatory in Arizona in 2013. This telescope is the only millimeter-wavelength telescope in the US operated full-time as a national facility and is now part of the Event Horizon Telescope (EHT).
TextToSpeechBehaviour_D392CC0A_C7E6_CE18_41D0_82027C0AAC52.text = The UArizona 12-meter Telescope was previously a European prototype antenna for the Atacama Large Millimeter/submillimeter Array (alma). Originally from the European Southern Observatory, it was transported to the Kitt Peak National Observatory in Arizona in 2013. This telescope is the only millimeter-wavelength telescope in the US operated full-time as a national facility and is now part of the Event Horizon Telescope (EHT).
TextToSpeechBehaviour_D388C00F_C7E6_F618_41E0_48518DA8AA3F.text = The UArizona 12-meter Telescope was previously a European prototype antenna for the Atacama Large Millimeter/submillimeter Array (alma). Originally from the European Southern Observatory, it was transported to the Kitt Peak National Observatory in Arizona in 2013. This telescope is the only millimeter-wavelength telescope in the US operated full-time as a national facility and is now part of the Event Horizon Telescope (EHT).
TextToSpeechBehaviour_A7719659_B9AC_0020_41D8_F881857272D6.text = The UArizona Bok 2.3-meter Telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona.
TextToSpeechBehaviour_A71738AE_B9DC_0061_41D0_B940D9A4AA32.text = The UArizona Bok 2.3-meter Telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona.
TextToSpeechBehaviour_A71718AD_B9DC_0063_41DF_402BD153A603.text = The UArizona Bok 2.3-meter Telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona.
TextToSpeechBehaviour_CD875084_D1C4_78F6_41E9_80AC8E7F3F31.text = The VLBA Dish is controlled remotely from the Science Operations Center in Socorro, New Mexico. Each VLBA station consists of a 25-meter antenna and an adjacent control building. 
TextToSpeechBehaviour_A785B32E_B9AC_0060_41C6_7C1A51F6F8D5.text = The Very Long Baseline Array Dish at Kitt Peak is part of the National Radio Astronomy Observatory’s VLBA interferometer. The array consists of 10 identical antennas, separated by distances from 200 kilometers to a transcontinental 8600 kilometers (with the longest baseline between Maunakea, Hawai‘i and St. Croix, Virgin Islands). 
TextToSpeechBehaviour_A785F332_B9AC_0060_41C8_D18182A03056.text = The Very Long Baseline Array Dish at Kitt Peak is part of the National Radio Astronomy Observatory’s VLBA interferometer. The array consists of 10 identical antennas, separated by distances from 200 kilometers to a transcontinental 8600 kilometers (with the longest baseline between Maunakea, Hawai‘i and St. Croix, Virgin Islands). 
TextToSpeechBehaviour_A6611654_B9A4_0020_41CB_2A8F7559AAE9.text = The Very Long Baseline Array Dish at Kitt Peak is part of the National Radio Astronomy Observatory’s VLBA interferometer. The array consists of 10 identical antennas, separated by distances from 200 kilometers to a transcontinental 8600 kilometers (with the longest baseline between Maunakea, Hawai‘i and St. Croix, Virgin Islands). The VLBA Dish is controlled remotely from the Science Operations Center in Socorro, New Mexico. Each VLBA station consists of a 25-meter antenna and an adjacent control building. 
TextToSpeechBehaviour_ED061053_C866_7608_41B3_64E94C090DF1.text = The Visitor Center 0.5-meter Telescope is used for a variety of nighttime observing programs for the public. The telescope is a Ritchey-Chretien design that delivers an outstanding image for both visual and photographic purposes. 
TextToSpeechBehaviour_ED13CEA3_C866_4A08_41CA_41C839B0C47F.text = The Visitor Center 0.5-meter Telescope is used for a variety of nighttime observing programs for the public. The telescope is a Ritchey-Chretien design that delivers an outstanding image for both visual and photographic purposes. 
TextToSpeechBehaviour_E99D85C3_C862_DE08_4174_74960EE83E0E.text = The Visitor Center 0.5-meter Telescope is used for a variety of nighttime observing programs for the public. The telescope is a Ritchey-Chretien design that delivers an outstanding image for both visual and photographic purposes. 
TextToSpeechBehaviour_9AA8E74E_B96C_0021_41C2_D2C14EDE958A.text = The Winter Milky Way arches high over three telescopes on Kitt Peak. These telescopes are (from left to right) The Burrell Schmidt Telescope, the 0.9-meter SARA Kitt Peak Telescope and Kitt Peak National Observatory's Visitor Center Roll Off Roof Observatory. The pillar of the Zodiacal Light can be seen in this image as well. Visitors to Kitt Peak’s evening program watch the sunset from this area. 
TextToSpeechBehaviour_9AA9C752_B96C_0021_41D4_5B342EFC159E.text = The Winter Milky Way arches high over three telescopes on Kitt Peak. These telescopes are (from left to right) The Burrell Schmidt Telescope, the 0.9-meter SARA Kitt Peak Telescope and Kitt Peak National Observatory's Visitor Center Roll Off Roof Observatory. The pillar of the Zodiacal Light can be seen in this image as well. Visitors to Kitt Peak’s evening program watch the sunset from this area. 
TextToSpeechBehaviour_9AB45756_B96C_0021_41E6_DA9A6B4F2566.text = The Winter Milky Way arches high over three telescopes on Kitt Peak. These telescopes are (from left to right) The Burrell Schmidt Telescope, the 0.9-meter SARA Kitt Peak Telescope and Kitt Peak National Observatory's Visitor Center Roll Off Roof Observatory. The pillar of the Zodiacal Light can be seen in this image as well. Visitors to Kitt Peak’s evening program watch the sunset from this area. 
TextToSpeechBehaviour_9AD378C0_B964_0021_41E0_16AF8FF1AB53.text = The arch of the winter Milky Way can be seen to the left of the Nicholas U. Mayall 4-meter Telescope. 
TextToSpeechBehaviour_9ACDC8BB_B964_0067_41AB_3B09779C39C2.text = The arch of the winter Milky Way can be seen to the left of the Nicholas U. Mayall 4-meter Telescope. 
TextToSpeechBehaviour_9AD318BE_B964_0061_41D7_F86324904930.text = The arch of the winter Milky Way can be seen to the left of the Nicholas U. Mayall 4-meter Telescope. 
TextToSpeechBehaviour_C8BC3C25_D784_477D_41E6_94409E9C2E40.text = The calibration screen is used for astro-imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects. 
TextToSpeechBehaviour_D5296540_C8A2_DE08_41D9_93BF0EEFC7C4.text = The distinctive dome of the Nicholas U. Mayall 4-meter Telescope can be seen over 80 kilometers (50 miles) away. This telescope was the second largest in the world upon its completion and has been producing ground-breaking science for almost 50 years. It is currently equipped with Department of Energy’s Dark Energy Spectroscopic Instrument (desi). 
TextToSpeechBehaviour_D2B689CA_C8A6_D618_41DE_84304F30CC4E.text = The distinctive dome of the Nicholas U. Mayall 4-meter Telescope can be seen over 80 kilometers (50 miles) away. This telescope was the second largest in the world upon its completion and has been producing ground-breaking science for almost 50 years. It is currently equipped with Department of Energy’s Dark Energy Spectroscopic Instrument (desi). 
TextToSpeechBehaviour_D51CF6FE_C8A2_DBF8_41E4_82B803439117.text = The distinctive dome of the Nicholas U. Mayall 4-meter Telescope can be seen over 80 kilometers (50 miles) away. This telescope was the second largest in the world upon its completion and has been producing ground-breaking science for almost 50 years. It is currently equipped with Department of Energy’s Dark Energy Spectroscopic Instrument (desi). 
TextToSpeechBehaviour_B78E9423_8E8E_27F1_41CC_6B8EDF23A5E5.text = The heliostats at the top of the McMath-Pierce reflect sunlight down to the primary mirrors. The largest heliostat is 2.03 meters in diameter and reflects light to a 1.61-meter mirror. The two smaller heliostats measure 1.07 meters in diameter and feed light to 0.91-meter primary mirrors. All three heliostats can observe the Sun simultaneously.
TextToSpeechBehaviour_B9F3D31C_8E82_61D7_41D6_5A2958C1510C.text = The heliostats at the top of the McMath-Pierce reflect sunlight down to the primary mirrors. The largest heliostat is 2.03 meters in diameter and reflects light to a 1.61-meter mirror. The two smaller heliostats measure 1.07 meters in diameter and feed light to 0.91-meter primary mirrors. All three heliostats can observe the Sun simultaneously. 
TextToSpeechBehaviour_BB6F792D_8E83_E1F1_41DA_412CCCA279CF.text = The heliostats at the top of the McMath-Pierce reflect sunlight down to the primary mirrors. The largest heliostat is 2.03 meters in diameter and reflects light to a 1.61-meter mirror. The two smaller heliostats measure 1.07 meters in diameter and feed light to 0.91-meter primary mirrors. All three heliostats can observe the Sun simultaneously. 
TextToSpeechBehaviour_DEA252F5_C7EE_5A08_41CE_F94D80898BD5.text = The subtle band of the winter Milky Way can be seen along the horizon below the telescopes of Kitt Peak National Observatory. The Nicholas U. Mayall 4-meter Telescope and the UArizona Bok 2.3-meter Telescope are in the foreground, with distant telescopes in the background. The lights of Sells, Arizona can be seen in this image. Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land. Also seen is the faint glow of the Zodiacal light and Gegenschein arching across the sky — faint reflections of sunlight from dust particles in the Solar System.
TextToSpeechBehaviour_DE1AA663_C7EE_5A08_41DE_E1AF0251B801.text = The subtle band of the winter Milky Way can be seen along the horizon below the telescopes of Kitt Peak National Observatory. The Nicholas U. Mayall 4-meter Telescope and the UArizona Bok 2.3-meter Telescope are in the foreground, with distant telescopes in the background. The lights of Sells, Arizona can be seen in this image. Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land. Also seen is the faint glow of the Zodiacal light and Gegenschein arching across the sky — faint reflections of sunlight from dust particles in the Solar System.
TextToSpeechBehaviour_D2936FC0_C7E6_4A08_41CC_836AFF4A0E12.text = The subtle band of the winter Milky Way can be seen along the horizon below the telescopes of Kitt Peak National Observatory. The Nicholas U. Mayall 4-meter Telescope and the UArizona Bok 2.3-meter Telescope are in the foreground, with distant telescopes in the background. The lights of Sells, Arizona can be seen in this image. Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land. Also seen is the faint glow of the Zodiacal light and Gegenschein arching across the sky — faint reflections of sunlight from dust particles in the Solar System.
TextToSpeechBehaviour_CFA457A6_D78C_417F_41DB_0F6FE8A8FEC6.text = The sundial teaches visitors to tell the time using the Sun.
TextToSpeechBehaviour_A663D657_B9A4_0020_41E2_F29E41D62098.text = The totally eclipsed Moon can be seen here just to the right of the Nicholas U. Mayall 4-meter Telescope. This image was created with a camera modified to bring out the red glow of hydrogen gas which can be seen in abundance in the winter Milky Way arching over the Mayall Telescope. 
TextToSpeechBehaviour_A662A659_B9A4_0020_41D5_D95C787D58C1.text = The totally eclipsed Moon can be seen here just to the right of the Nicholas U. Mayall 4-meter Telescope. This image was created with a camera modified to bring out the red glow of hydrogen gas which can be seen in abundance in the winter Milky Way arching over the Mayall Telescope. 
TextToSpeechBehaviour_985F2017_B95C_002F_41E5_E81E314AF193.text = The winter Milky Way arches above the SARA (Southeastern Association For Research In Astronomy) 0.9-meter Telescope. The Zodiacal light can be seen as a bright pillar in the western sky. The Zodiacal light is caused by sunlight reflecting off interplanetary dust. 
TextToSpeechBehaviour_985EC018_B95C_0021_41DD_B4AAA121FDF6.text = The winter Milky Way arches above the SARA (Southeastern Association For Research In Astronomy) 0.9-meter Telescope. The Zodiacal light can be seen as a bright pillar in the western sky. The Zodiacal light is caused by sunlight reflecting off interplanetary dust. 
TextToSpeechBehaviour_985FC015_B95C_0023_41D3_8CCDF4E73F2D.text = The winter Milky Way arches above the SARA (Southeastern Association For Research In Astronomy) 0.9-meter Telescope. The Zodiacal light can be seen as a bright pillar in the western sky. The Zodiacal light is caused by sunlight reflecting off interplanetary dust. 
TextToSpeechBehaviour_D6223D48_C7A2_CE18_41B6_73E274167EA1.text = The winter Milky Way arches high over the dome of the Mayall 4-meter Telescope. The Zodiacal light can be seen to the right of the Mayall reaching up toward the Milky Way. The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_D72063D2_C7A6_DA08_41DF_309EEBD19EA2.text = The winter Milky Way arches high over the dome of the Mayall 4-meter Telescope. The Zodiacal light can be seen to the right of the Mayall reaching up toward the Milky Way. The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_D607759C_C7A2_DE38_41B3_FEB00B463697.text = The winter Milky Way arches high over the dome of the Mayall 4-meter Telescope. The Zodiacal light can be seen to the right of the Mayall reaching up toward the Milky Way. The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_99FB5624_B9A4_0060_41E5_74F655B1A013.text = The winter Milky Way arches over the McMath-Pierce Solar Telescope. The specially modified camera reveals the red nebulosity. The McMath-Pierce Solar Telescope is currently being transformed into the Windows On the Universe Center For Astronomy Outreach. 
TextToSpeechBehaviour_99FB861F_B9A4_0020_41BC_B419A3E8E6AE.text = The winter Milky Way arches over the McMath-Pierce Solar Telescope. The specially modified camera reveals the red nebulosity. The McMath-Pierce Solar Telescope is currently being transformed into the Windows On the Universe Center For Astronomy Outreach. 
TextToSpeechBehaviour_99FD8621_B9A4_0060_4191_DA0C2B03170C.text = The winter Milky Way arches over the McMath-Pierce Solar Telescope. The specially modified camera reveals the red nebulosity. The McMath-Pierce Solar Telescope is currently being transformed into the Windows On the Universe Center For Astronomy Outreach. 
TextToSpeechBehaviour_9EB0D3AC_39ED_4A80_417F_D42B227FF465.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak.  \
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noirlab operates the 3.5-meter wiyn Telescope on behalf of the  partnership between Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa).  \
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Its neid instrument is designed to measure the motion of nearby stars with extreme precision, with the potential to uncover Earth-mass exoplanets.  \

TextToSpeechBehaviour_D09BACAF_C8A2_4E18_41DA_B918D8886485.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak.  \
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noirlab operates the 3.5-meter wiyn Telescope on behalf of the  partnership between Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa).  \
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Its neid instrument is designed to measure the motion of nearby stars with extreme precision, with the potential to uncover Earth-mass exoplanets.  \

TextToSpeechBehaviour_9EB0E3AC_39ED_4A80_41C7_281FD6D2B322.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak.  \
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noirlab operates the 3.5-meter wiyn Telescope on behalf of the  partnership between Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa).  \
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Its neid instrument is designed to measure the motion of nearby stars with extreme precision, with the potential to uncover Earth-mass exoplanets.  \

TextToSpeechBehaviour_D1D05880_C8A2_3607_41B1_B5CA0B619A67.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak. The wiyn telescope is operated by noirlab on behalf of Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa. wiyn currently hosts neid, a radial velocity instrument designed to measure the motion of nearby stars with extreme precision. The Visitor Center Levine 0.4-meter Telescope is used for public viewing by the Kitt Peak Visitor Center. The wiyn 0.9-meter Telescope is a short walk up the hill.
TextToSpeechBehaviour_D1A62A72_C8A2_CA08_41E6_DB32EAC603EC.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak. The wiyn telescope is operated by noirlab on behalf of Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa. wiyn currently hosts neid, a radial velocity instrument designed to measure the motion of nearby stars with extreme precision. The Visitor Center Levine 0.4-meter Telescope is used for public viewing by the Kitt Peak Visitor Center. The wiyn 0.9-meter Telescope is a short walk up the hill.
TextToSpeechBehaviour_D1697C5D_C8A3_CE38_4160_B2CAA07A88B2.text = The wiyn 3.5-meter Telescope is the second-largest telescope on Kitt Peak. The wiyn telescope is operated by noirlab on behalf of Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s noirlab, and nasa. wiyn currently hosts neid, a radial velocity instrument designed to measure the motion of nearby stars with extreme precision. The Visitor Center Levine 0.4-meter Telescope is used for public viewing by the Kitt Peak Visitor Center. The wiyn 0.9-meter Telescope is a short walk up the hill.
TextToSpeechBehaviour_C8438721_D785_C175_41D8_858FCD19A399.text = This computer allows the telescope operator to control the telescope and the imaging camera(s) attached to the telescope.
TextToSpeechBehaviour_322ABB9D_4131_E3E7_41B6_850F941797B4.text = Total Lunar Eclipse
TextToSpeechBehaviour_05AECEC0_2979_60B2_41C0_3D7C6FF12FB3.text = UArizona 0.9-meter Spacewatch Telescope
TextToSpeechBehaviour_C83067F4_D24C_5816_41E5_DA1E2E774061.text = UArizona 0.9-meter Spacewatch Telescope
TextToSpeechBehaviour_0C6710D2_2919_E056_41BD_1C63D31F4803.text = UArizona 1.8-meter Spacewatch Telescope
TextToSpeechBehaviour_C054553A_D244_D812_41E1_9F8B080A59E4.text = UArizona ARO 12-meter Telescope
TextToSpeechBehaviour_058C2946_2907_E1BE_41B5_4E097DFCC7BF.text = UArizona Bok 2.3-meter Telescope
TextToSpeechBehaviour_C609C01A_D24C_5812_41E5_9715A7B7BDDC.text = UArizona Bok 2.3-meter Telescope
TextToSpeechBehaviour_C24D1846_D24C_4872_41E3_C9F1E88EAD99.text = UArizona Bok 2.3-meter Telescope
TextToSpeechBehaviour_DD200440_DB84_4734_41D2_1157FAE15B38.text = UArizona Bok 2.3-meter Telescope \
It was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona. It is the largest optical telescope operated solely by Steward Observatory.
TextToSpeechBehaviour_3A7DAB23_DA84_C174_41E5_55F8104EAE80.text = UArizona Bok 2.3-meter Telescope \
This telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona. It is the largest optical telescope operated solely by Steward Observatory.
TextToSpeechBehaviour_C263FD8A_D24C_48F2_41C0_41063D4FAE14.text = UArizona Spacewatch 0.9-meter Telescope
TextToSpeechBehaviour_C119622C_D27D_D836_41D0_3C7394DA7CB0.text = Very Long Baseline Array Dish
TextToSpeechBehaviour_0A723A52_2919_2056_41B7_22C50C697E8E.text = Visitor Center 0.5-meter Telescope
TextToSpeechBehaviour_CE109DEF_D78C_40CD_4165_D579C4F8C6B2.text = Visitors to Kitt Peak can relax and enjoy lunch outside the Visitor Center.
TextToSpeechBehaviour_C0BD5610_D24C_3BEE_41E7_09BF77FC8BE5.text = WIYN 0.9-meter Telescope
TextToSpeechBehaviour_0E5450C2_2907_60B6_41C1_E0896FDE2B82.text = WIYN 2.1-meter Telescope
TextToSpeechBehaviour_C0958377_D244_5812_4179_D7629ECD08D8.text = WIYN 3.5-meter Telescope
TextToSpeechBehaviour_2A346774_3F56_58C8_41BD_EDBA0AF032D1.text = Welcome to Kitt Peak National Observatory. \
A birds eye view of Kitt Peak taken before the June 2022 Contreras Fire.  \
Click here for more info
TextToSpeechBehaviour_2A1267AF_3F56_5858_41A4_1A2CCFBC17FA.text = Welcome to Kitt Peak National Observatory. \
A birds eye view of Kitt Peak taken before the June 2022 Contreras Fire.  \
Click here for more info
TextToSpeechBehaviour_2A1FF7A8_3F56_5858_418E_8E39B43FA0BB.text = Welcome to Kitt Peak National Observatory. \
A birds eye view of Kitt Peak taken before the June 2022 Contreras Fire.  \
Click here for more info
TextToSpeechBehaviour_CFE492C1_D78F_C335_41CB_B27FADE1B219.text = Welcome to Kitt Peak National Observatory. \
Click here for more info
TextToSpeechBehaviour_C0F9689D_D78C_CF4D_41E2_DCEFC2DFFAF5.text = Welcome to Kitt Peak National Observatory. \
Click here for more info
TextToSpeechBehaviour_F95114C9_D1CC_587E_41A4_8E57AB016E8F.text = Zodiacal light \
 \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_41279110_38F4_C79F_41BB_D0B3A036BC83.text = Zodiacal light \
 \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_DDDC8814_DABC_4F53_41C0_826167A6DA9E.text = Zodiacal light \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
TextToSpeechBehaviour_D5405D0D_C862_4E18_41E5_F305F08397E6.text = solario (the Solar And Remote Imaging Observatory) is operated by the Kitt Peak Visitor Center and contains several telescopes. The SOLARIO 0.38-meter telescope is equipped with a ZWO ASI071MC Pro camera and is used primarily for nighttime imaging. Members of the public can rent the telescope and control it remotely.
TextToSpeechBehaviour_D53BEB58_C862_4A38_41DA_390750E1E3B3.text = solario (the Solar And Remote Imaging Observatory) is operated by the Kitt Peak Visitor Center and contains several telescopes. The SOLARIO 0.38-meter telescope is equipped with a ZWO ASI071MC Pro camera and is used primarily for nighttime imaging. Members of the public can rent the telescope and control it remotely.
TextToSpeechBehaviour_D4FC3D77_C85F_CE08_419D_1137AEC8861D.text = solario (the Solar And Remote Imaging Observatory) is operated by the Kitt Peak Visitor Center and contains several telescopes. The solario 0.38-meter telescope is equipped with a ZWO ASI071MC Pro camera and is used primarily for nighttime imaging. Members of the public can rent the telescope and control it remotely.
TextToSpeechBehaviour_7BD1C3F8_DA87_C0D3_41E8_968376D3DCCE.text = solario contains three solar telescopes: a Coronado 90-millimeter SolarMax Hydrogen Alpha Telescope, a Coronado 90-millimeter SolarMax Calcium K Telescope, and a refractor with a white-light solar filter. They are open for daytime viewing when weather and staffing permit.
TextToSpeechBehaviour_D9094A8C_DB84_C333_41AD_3E0B69EB5EEF.text = wiyn Telescopes Exterior

### URL
LinkBehaviour_AE50C9DB_9E93_51FC_41B8_FC49BCAF270A.source = https://noirlab.edu/public/images/archive/category/kpno/
LinkBehaviour_2DE3D804_7D24_235C_41D0_AE9A9612907C.source = https://noirlab.edu/public/images/archive/category/kpno/
PopupWebFrameBehaviour_DD49BF13_DB84_4155_41DA_697D1847685F.url = https://noirlab.edu/public/images/iotw2225a/
PopupWebFrameBehaviour_D5FF7171_42D2_FF3F_41C0_EAFB85F35B8E.url = https://noirlab.edu/public/images/iotw2340a/
PopupWebFrameBehaviour_ECED2E43_D9D7_6E2A_41C1_397ABE808304.url = https://noirlab.edu/public/images/noao-dark_sky/
PopupWebFrameBehaviour_0D287B56_87EC_25FC_41D1_393C1B290640.url = https://noirlab.edu/public/images/noao-dark_sky/
PopupWebFrameBehaviour_69D1310D_D984_414D_41E3_8670E6FBE418.url = https://noirlab.edu/public/images/noirlab2117b/
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WebFrame_1DEF4086_7D2C_635C_41DB_DCE460CBDD3B.url = https://noirlab.edu/public/media/archives/images/publicationjpg/iotw2237a.jpg
PopupWebFrameBehaviour_6E2F151D_D9BC_C14D_41CF_1E0D8115ED64.url = https://noirlab.edu/public/news/noirlab2304/
LinkBehaviour_582726D4_57D6_03D8_41CD_48EA5C9FF0A4.source = https://noirlab.edu/public/products/virtual-tours/
LinkBehaviour_6D0E010A_584E_1E49_418E_524F61D493AE.source = https://noirlab.edu/public/products/virtual-tours/
PopupWebFrameBehaviour_E5CBBBE2_C863_CA08_41D5_EEC6CA899621.url = https://noirlab.edu/public/programs/csdc/
PopupWebFrameBehaviour_E24D4448_C866_3E18_41E1_2E1344111174.url = https://noirlab.edu/public/programs/csdc/
LinkBehaviour_B2E09DA2_95D0_28A3_41DE_1089BA875DE3.source = https://noirlab.edu/public/programs/kitt-peak-national-observatory/
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WebFrame_062271C7_8724_24DC_41D7_A31678DC2F29.url = https://noirlab.edu/public/programs/kitt-peak-national-observatory/visitor-center-levine-04-m/
WebFrame_FAAC28A6_86E4_235C_41BE_2B2856E3CDFC.url = https://noirlab.edu/public/programs/kitt-peak-national-observatory/wiyn-09m-telescope/
PopupWebFrameBehaviour_175F0AF8_8724_24B4_41B2_DF3190A9B998.url = https://noirlab.edu/public/projects/desi/
PopupWebFrameBehaviour_E19BC19B_C863_D638_41C2_A675055632F9.url = https://noirlab.edu/public/projects/desi/
PopupWebFrameBehaviour_14706E95_8724_1F7C_41AB_8C4B039BF2B5.url = https://noirlab.edu/public/projects/desi/
PopupWebFrameBehaviour_E3B9DDF0_C862_CE08_41AE_9B209AF72E5E.url = https://noirlab.edu/public/projects/desi/
PopupWebFrameBehaviour_167CB71C_8724_ED73_41DA_4ED96334D02F.url = https://noirlab.edu/public/projects/neid/
PopupWebFrameBehaviour_19B01F15_8724_1D7D_41CB_9253322E2724.url = https://noirlab.edu/public/projects/neid/
LinkBehaviour_AB56D6B3_9E91_53B3_41D8_3C7478CAE902.source = https://noirlab.edu/public/videos/archive/category/kpno/
LinkBehaviour_2F20AEC7_7D24_1CDC_41B3_65668704EAAE.source = https://noirlab.edu/public/videos/archive/category/kpno/
LinkBehaviour_A2B877DF_F5EA_620D_41D5_57B2DC0ACE1E.source = https://www.noirlab.edu/public/
LinkBehaviour_B319BFDA_95D0_28E0_41D9_3BE3F2219CB4.source = https://www.noirlab.edu/public/
LinkBehaviour_71304AC8_584A_03C8_41C2_DF25665D8B45.source = https://www.noirlab.edu/public/about/
LinkBehaviour_71304AC8_584A_03C8_41C2_DF25665D8B45.source = https://www.noirlab.edu/public/about/

## E-Learning

### Question Screen
quizQuestion_2349C385_3EA9_0F84_41CA_5B4B4AECA91E.ok = OK

### Report Screen
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.title = - SCORE -
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.completion = Completed
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.questionsCorrect = Correct
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.downloadCSV = Download .csv
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.questionsIncorrect = Incorrect
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.items = Items Found
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.questions = Questions
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.repeat = Repeat
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.submitToLMS = Submit
quizScore_20B63386_3EA9_0F84_41C0_AD8FCC1CD7CD.elapsedTime = Time

### Score Name
score1.label = Score 1

### Timeout Screen
quizTimeout_234AE384_3EA9_0F84_41C0_6B96A7557C47.title = - TIMEOUT -
quizTimeout_234AE384_3EA9_0F84_41C0_6B96A7557C47.repeat = Repeat
quizTimeout_234AE384_3EA9_0F84_41C0_6B96A7557C47.score = View Score

## Hotspot

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HotspotPanoramaOverlayTextImage_6339A766_DA84_41FF_41C5_9F4186FE3BC2.text =  \
DESI Control Room \

HotspotPanoramaOverlayTextImage_612B66D0_2B19_6052_41AE_1810D722311A.text =  \
Hiltner 2.4-meter Telescope
HotspotPanoramaOverlayTextImage_E82492FD_D9CD_D986_41DA_E19A8570B2AB.text =  \
Kitt Peak  \
Visitor Center
HotspotPanoramaOverlayTextImage_6B75624E_234C_968B_41B5_BE4A5DCB9228.text =  \
Kitt Peak  \
Visitor Center \

HotspotPanoramaOverlayTextImage_B18CF9D4_A19E_ED1D_41E4_169BF7DDEDA0.text =  \
Kitt Peak 2.1-meter Telescope Interior \

HotspotPanoramaOverlayTextImage_B91DF969_9FF1_FEDC_4194_B011D6A8B21C.text =  \
Kitt Peak Visitor Center
HotspotPanoramaOverlayTextImage_B6E91084_9F91_EE54_41DE_7E9C7E645076.text =  \
Library
HotspotPanoramaOverlayTextImage_B6B5D46A_9F90_D6DC_41B1_713F183D198C.text =  \
Main Lobby
HotspotPanoramaOverlayTextImage_7818B7A8_2B09_60F2_41C3_A257AF150FA9.text =  \
Mayall Exterior
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Mayall Exterior
HotspotPanoramaOverlayTextImage_467869BD_2B19_20CD_41C0_62F6440FE734.text =  \
McGraw-Hill 1.3-meter Telescope
HotspotPanoramaOverlayTextImage_920367B3_9D91_724C_41C5_48E8CF675355.text =  \
McMath-Pierce Solar Telescope Exterior
HotspotPanoramaOverlayTextImage_B0A1888F_A183_EB0B_41CC_D478224A7900.text =  \
McMath-Pierce Solar Telescope Exterior \

HotspotPanoramaOverlayTextImage_322D6B9A_4131_E3ED_41B6_FAD036380606.text =  \
Total Lunar Eclipse
HotspotPanoramaOverlayTextImage_B5CBB361_9F93_D2CF_41D6_1C6714768B1C.text =  \
Total Lunar Eclipse \

HotspotPanoramaOverlayTextImage_D903D331_DB8B_C155_41CB_B949433FEABB.text =  \
UArizona 0.9-meter Telescope \

HotspotPanoramaOverlayTextImage_85D3353F_9DAF_001B_41D5_65BA93AC9D64.text =  \
Visitor Center 0.5-meter Telescope
HotspotPanoramaOverlayTextImage_4230A727_DA84_C17C_41E0_EB09780BA080.text =  \
Visitor Center 0.5-meter Telescope
HotspotPanoramaOverlayTextImage_B122E55F_A187_E50B_41D0_7D98B40ACBF6.text =  \
WIYN 3.5-meter  \
Telescope Interior
HotspotPanoramaOverlayTextImage_04A84A34_7BE4_27BC_41C7_837F991E1D56.text =  \
WIYN 3.5-meter  \
Telescope Interior \

HotspotPanoramaOverlayTextImage_B2AD0987_9E90_FE54_41DE_56CC885D0707.text =  \
WIYN Telescopes Exterior \

HotspotPanoramaOverlayTextImage_C24DF844_D24C_4876_41E3_E299FBA28A9B.text =                        UArizona Bok  \
                                    2.3-meter Telescope \
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HotspotPanoramaOverlayTextImage_5924E7F5_D3D9_6AC0_41D4_0235F398B2B9.text =                  Horsehead Nebula ―
HotspotPanoramaOverlayTextImage_5E27DBEC_D3E8_DAC1_41DD_6F8F616A0C77.text =         California Nebula ―
HotspotPanoramaOverlayTextImage_0072AE18_2909_23D2_41C3_A01805B4C642.text =         ―Robotically Controlled Telescope
HotspotPanoramaOverlayTextImage_0A724A53_2919_2056_41B3_E6DA738A37D6.text =        \ \
        Visitor Center 0.5-meter Telescope
HotspotPanoramaOverlayTextImage_0E60FCF2_2939_2056_41AD_17323041C59E.text =        ―Burrell Schmidt Telescope
HotspotPanoramaOverlayTextImage_05AF2EC1_2979_60B2_41B7_75D3E931CA4F.text =        ―UArizona 0.9-meter Spacewatch Telescope
HotspotPanoramaOverlayTextImage_0C67D0D2_2919_E056_41C2_6469F27B44AE.text =        ―UArizona 1.8-meter Spacewatch Telescope
HotspotPanoramaOverlayTextImage_0DD112B2_291A_E0D6_41AA_E18146CAC9E9.text =       ―SARA Kitt Peak Telescope
HotspotPanoramaOverlayTextImage_560A1242_D3A8_E5C1_41E3_8873C4AB20A9.text =   Capella \
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HotspotPanoramaOverlayTextImage_9C1E98CC_89B1_AEB7_41B2_5B5B204B9DD3.text = .
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HotspotPanoramaOverlayTextImage_FA96B330_872C_25B4_41CA_918F84ABCC46.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
HotspotPanoramaOverlayTextImage_03A606EC_8725_ECAC_41C2_893C092DC563.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
HotspotPanoramaOverlayTextImage_3F136A62_4136_2D5D_41B9_62ECB8FE5066.text = 22-degree halo formed by ice crystals in the atmosphere. \
Click here for more info:
HotspotPanoramaOverlayTextImage_1E74C047_41F2_3D62_41A6_998BE48DC159.text = Admin Building
HotspotPanoramaOverlayTextImage_538DBB1F_D3D8_BB7F_41D3_8546F9D27CCC.text = Aldebaran ―
HotspotPanoramaOverlayTextImage_5FC0F6BC_D3E9_6D41_41E9_14593754D0A5.text = Betelgeuse ―
HotspotPanoramaOverlayTextImage_50F3AC9A_D3B9_5D40_41D2_7BC042A76DED.text = Canopus \
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HotspotPanoramaOverlayTextImage_B9F76623_D6BC_4375_41A8_0FC940AD319A.text = DESI Control Room \
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HotspotPanoramaOverlayTextImage_DD69C33B_DB87_C155_41D1_6891ADE9D43F.text = Hiltner 2.4-meter Telescope \
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HotspotPanoramaOverlayTextImage_DE3E6276_D9FC_C3DF_41BC_7BA378604FAB.text = Hiltner 2.4-meter Telescope \
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HotspotPanoramaOverlayTextImage_EB8CB792_D9F5_7E2A_41E9_FEF71CA91CFC.text = Interior of the Mayall
HotspotPanoramaOverlayTextImage_280E320C_4152_5CE5_41C7_93057150ED65.text = Interior of the Mayall
HotspotPanoramaOverlayTextImage_75E97471_D98C_47D4_41D4_B51E7C9FD2CD.text = Interior of the Mayall
HotspotPanoramaOverlayTextImage_B48505F5_9E71_D1B7_41E0_A00D8A887B63.text = Interior of the Mayall \

HotspotPanoramaOverlayTextImage_85991AAE_D1C4_4833_41E6_8E0BD4DB6BC2.text = KPNO 2.1-meter Telescope \
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HotspotPanoramaOverlayTextImage_63D1A8A0_3EAF_19BC_41B2_41C1EF413C77.text = KPNO Admin  \
Building
HotspotPanoramaOverlayTextImage_DBFEE545_DE7D_C13D_41C3_3ACC496A1370.text = KPNO Admin Building
HotspotPanoramaOverlayTextImage_452622A4_4371_DD25_41C4_47765AC481F6.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_45424126_4336_5F25_41D0_472A50238263.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_45243935_4372_2F27_41B5_7CE988174613.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_4531FB11_4352_2CFF_41C7_3A9F4A369498.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_454EDD48_43CE_676D_41C9_15FAD26660E4.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_4544C26D_4332_5D27_4199_ECD0D1F00B0F.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_4535EB12_4352_2CFC_4167_CA545B53DC5C.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_4538181E_4351_ECE5_41BE_5A5BBAC0B258.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_452B391E_4376_2CE5_41C5_17571C3DE6D4.text = KPNO Drone View
HotspotPanoramaOverlayTextImage_B5E72711_A18D_E517_41DB_4AF13AB56526.text = Kitt Peak  \
Visitor Center
HotspotPanoramaOverlayTextImage_86370FF9_9D90_D1BF_41DF_7D7F06CC3591.text = Kitt Peak  \
Visitor Center \

HotspotPanoramaOverlayTextImage_DDE9206E_DA84_7FCF_41D5_2AAF6CFAAAB3.text = Kitt Peak  \
Visitor Center \
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HotspotPanoramaOverlayTextImage_B7DB1508_38FB_4F8F_41CA_BD720E2DBA81.text = Kitt Peak 2.1-m Telescope Interior
HotspotPanoramaOverlayTextImage_1DBDDA51_41DE_6D7C_41CD_FE7A5B31982E.text = Kitt Peak 2.1-m Telescope Interior
HotspotPanoramaOverlayTextImage_BA31E6FB_A38E_A70B_41C0_B17E37FDA662.text = Kitt Peak 2.1-meter \
Telescope Interior
HotspotPanoramaOverlayTextImage_7B72D37C_2B09_2052_419A_8529742DF965.text = Kitt Peak Visitor Center
HotspotPanoramaOverlayTextImage_B7E01512_38FB_4F83_41C5_3A31AD06D6BC.text = Kitt Peak Visitor Center
HotspotPanoramaOverlayTextImage_0AB01E44_4171_E565_41B3_A353FD2C8DAC.text = Kitt Peak Visitor Center \
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HotspotPanoramaOverlayTextImage_E6CAB53A_D1C4_3813_41E8_889D74CA249C.text = Light Pollution from Phoenix, Arizona \
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HotspotPanoramaOverlayTextImage_EBA2CC97_D9DC_F22A_41D4_097CE1EFC843.text = Light pollution from Tucson. \
Click here for more info
HotspotPanoramaOverlayTextImage_BA52E5E0_9FAF_51CC_41CA_B3E530377E7F.text = Mayall  Exterior \
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HotspotPanoramaOverlayTextImage_581E47BE_2909_20CE_41A3_154D5127CA40.text = Mayall Exterior
HotspotPanoramaOverlayTextImage_6CB73434_2B09_27D2_41B8_64704804E1C7.text = Mayall Exterior
HotspotPanoramaOverlayTextImage_34363529_4132_272C_41B7_C47CB0FA354F.text = Mayall Exterior
HotspotPanoramaOverlayTextImage_0C4F1CF1_8724_3CB4_41D5_92D439DF3EE9.text = Mayall Exterior
HotspotPanoramaOverlayTextImage_38C5325C_2906_E052_41B8_6A9DBE47D974.text = Mayall Exterior \
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HotspotPanoramaOverlayTextImage_5124E9CC_291B_20B2_41C1_C3491AE38BFF.text = Mayall With Zodiacal Light \
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HotspotPanoramaOverlayTextImage_2A59BE12_386B_D625_41B4_D5F0ED36B444.text = Mayall at Night
HotspotPanoramaOverlayTextImage_91D18A8D_2919_60B2_41A2_99B40CF5AC01.text = Mayall at Night
HotspotPanoramaOverlayTextImage_28D57A9C_4152_EDE6_41C2_B7A3EB33CB27.text = Mayall at Night
HotspotPanoramaOverlayTextImage_DE2FDB63_D99B_C1F4_41DD_E500A73DBB71.text = McGraw-Hill 1.3-meter Telescope \
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HotspotPanoramaOverlayTextImage_12BF52D6_4132_5D65_4197_79C21BA9A6D8.text = McMath-Pierce  \
Exterior
HotspotPanoramaOverlayTextImage_129827B0_4132_633D_4190_684308149B40.text = McMath-Pierce  \
Roof
HotspotPanoramaOverlayTextImage_9237B7B1_290A_E0D2_41BA_C139A9576368.text = McMath-Pierce Exterior \

HotspotPanoramaOverlayTextImage_06D4A79A_2919_60D6_41BB_C61618AD1F57.text = McMath-Pierce Exterior \
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HotspotPanoramaOverlayTextImage_DC262512_D98C_4154_41E4_A34B63A78113.text = McMath-Pierce Roof 
HotspotPanoramaOverlayTextImage_E9BBA2A4_D9CB_F986_41EA_EAF5B7BF7603.text = McMath-Pierce Roof  \

HotspotPanoramaOverlayTextImage_872CBC96_9DA3_00ED_41D0_C9EC6565B270.text = McMath-Pierce Solar Telescope Exterior \
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HotspotPanoramaOverlayTextImage_64871153_38EB_4781_41C6_10F4C386397B.text = McMath-Pierce at Night
HotspotPanoramaOverlayTextImage_DC3BCA3C_D9FB_C34C_41E7_1EEB1C42342E.text = McMath-Pierce at night \
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HotspotPanoramaOverlayTextImage_DD230D08_DB84_4134_41C4_5D28DE9AD63A.text = Milkyway Over Kitt Peak \

HotspotPanoramaOverlayTextImage_DD770475_DB8C_47DD_41D4_FAD951CD6761.text = Milkyway Over Kitt Peak \
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HotspotPanoramaOverlayTextImage_AA8EFF83_2939_20B6_41A1_7F4FA9CC6A43.text = Milkyway Over Kitt Peak \
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HotspotPanoramaOverlayTextImage_C22D9FDE_D25B_C813_41C2_D2222144328C.text = Nicholas U. Mayall  \
4-meter Telescope \
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HotspotPanoramaOverlayTextImage_55A6B302_D3DF_AB41_41DC_9D9185FDA7F7.text = Orion Nebula―
HotspotPanoramaOverlayTextImage_ABDD73F8_D3E8_EAC1_41DC_C43159E9C9A9.text = Pleiades ―
HotspotPanoramaOverlayTextImage_5AA2148E_D3B7_ED40_41AA_5B61CB1DE7D3.text = Procyon―
HotspotPanoramaOverlayTextImage_2512E9E1_41D2_2F5F_41B5_2F7C81A220B4.text = Roll Off Roof Observatory
HotspotPanoramaOverlayTextImage_E90ADD3B_2906_E1D6_41B4_550059B3AFA6.text = Roll Off Roof Observatory
HotspotPanoramaOverlayTextImage_E634D5A8_290A_E0F2_41B5_9B2F23E4A420.text = Roll Off Roof Observatory \

HotspotPanoramaOverlayTextImage_DDDA71D8_DA84_C0D4_4184_69C5FB9B070E.text = Rosette Nebula ―
HotspotPanoramaOverlayTextImage_58387B75_D3FF_5BC3_41E0_4295D7FB52F4.text = Rosette Nebula ―
HotspotPanoramaOverlayTextImage_209A892C_387B_DA7D_41C3_F18C0BFD1CC8.text = SARA Kitt Peak Telescope
HotspotPanoramaOverlayTextImage_1E1E4C1D_41F2_E4E7_41B8_BB86291AAE55.text = SARA Kitt Peak Telescope \
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HotspotPanoramaOverlayTextImage_DD19E689_DB87_C335_41E8_1C176896502B.text = SARA Kitt Peak Telescope \
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HotspotPanoramaOverlayTextImage_FAFD8A02_F8A3_FBD3_41D2_3652A3B15208.text = SARA Kitt Peak Telescope \
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HotspotPanoramaOverlayTextImage_E5B1CCFD_D784_40CD_41DA_FC2694C3D411.text = SOLARIO
HotspotPanoramaOverlayTextImage_0881DF27_7B24_3D5C_41A0_95EB68D8E4DA.text = SOLARIO \
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HotspotPanoramaOverlayTextImage_12676E7F_21C5_8E89_41BF_DFABC6F6DBB9.text = SOLARIO (the Solar And Remote Imaging Observatory) is operated by the Kitt Peak Visitor Center and contains several telescopes. The SOLARIO 0.38-meter telescope is equipped with a ZWO ASI071MC Pro camera and is used primarily for nighttime imaging. Members of the public can rent the telescope and control it remotely.
HotspotPanoramaOverlayTextImage_10B3873B_21CB_BE89_41B4_82FE9028EC93.text = SOLARIO contains three solar telescopes: a Coronado 90-millimeter SolarMax Hydrogen Alpha Telescope, a Coronado 90-millimeter SolarMax Calcium K Telescope, and a refractor with a white-light solar filter. They are open for daytime viewing when weather and staffing permit.
HotspotPanoramaOverlayTextImage_50A2402A_D3A8_A540_41E8_E7004F383941.text = Seagull Nebula ―
HotspotPanoramaOverlayTextImage_9257D51D_D1DC_7811_418D_3FE48143FDA1.text = Sells, Arizona \
capital of Tohono O’odham Nation \
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HotspotPanoramaOverlayTextImage_A57950DD_B9A4_05AB_41C9_3E623F33E79C.text = Spacewatch is the name of a group,founded by Tom Gehrels and Robert S. McMillan in 1980, at the University of Arizona’s Lunar and Planetary Laboratory. Today, Spacewatch is led by Dr. Melissa Brucker. The original goal of Spacewatch was to explore the various populations of small objects in the Solar System, and study the statistics of asteroids and comets in order to investigate the dynamical evolution of the Solar System. Since 1998, Spacewatch has focused primarily on follow-up astrometry of such targets, and especially monitors the positions and motions of objects that might present a hazard to Earth.
HotspotPanoramaOverlayTextImage_CDB39CB7_D1BC_4812_41C0_B5DC4AC865BE.text = Support Building \
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HotspotPanoramaOverlayTextImage_9988DA57_8E82_2051_41CF_ED836F9482B7.text = The DESI Control Room was constructed in conjunction with the installation of the Department of Energy’s Dark Energy Spectroscopic Instrument (DESI). The DESI Control Room is currently used to control the telescope and acquire data with DESI (the original control room can be used for testing and engineering purposes). \

HotspotPanoramaOverlayTextImage_A50CA56E_8E86_6073_41E0_51F60EF40F24.text = The Hiltner 2.4-meter Telescope is operated by a consortium of universities including Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. This telescope performs galactic surveys. 
HotspotPanoramaOverlayTextImage_B53C274D_A18E_E50E_41E2_9EA8CA506B40.text = The KPNO 2.1-meter Telescope was one of the earliest Kitt Peak telescopes and is used for both imaging and spectroscopy. It is paired with the Coudé Tower (now retired), which enabled spectroscopic work to be performed independently of the main telescope, effectively making the 2.1-meter telescope a dual observing facility. 
HotspotPanoramaOverlayTextImage_9D8573D7_B964_002F_41E6_4CFCB6AF7E12.text = The Kitt Peak Administration Building houses offices for Kitt Peak administrative staff and the Kitt Peak Associate Director. The Robotically Controlled Telescope (RCT) is attached to the east side of the Administration Building (here obscured by trees) and operated by a consortium led by Western Kentucky University. Dorm 1 can be seen on the far right side of the image. 
HotspotPanoramaOverlayTextImage_91C6B51B_8E9E_61D1_41DE_5060319C2B3F.text = The Kitt Peak Visitor Center (KPVC) is the first place visitors go upon arrival at the summit. The KPVC contains exhibits on astronomy, Kitt Peak, and the Tohono O’odham Nation. The gift shop contains a variety of Kitt Peak merchandise and Tohono O’odham art. 
HotspotPanoramaOverlayTextImage_1D893156_7D1C_65FC_41D8_038E2BC9160F.text = The Kitt Peak Visitor Center is the first stop for visitors to Kitt Peak. The Visitor Center has displays outlining the history of Kitt Peak and astronomy, and a gift shop that features an outstanding selection of Tohono O'odham baskets and art. Tours and nightly programs begin at the Visitor Center.  \
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HotspotPanoramaOverlayTextImage_A0051E19_8E86_E3D1_41CB_CAC4F756BD51.text = The McGraw-Hill 1.3-meter Telescope is part of the MDM Observatory, which is owned and operated by a consortium of five educational institutions — Dartmouth College, The Ohio State University, Columbia University, The University of Michigan and Ohio University. The telescope was moved to Kitt Peak in 1975. The asteroid 4432 McGraw-Hill is named after this telescope.
HotspotPanoramaOverlayTextImage_BB110595_9F91_5674_41A6_73390E15795A.text = The Nicholas U. Mayall 4-meter Telescope is the largest optical telescope on Kitt Peak. It was the second-largest optical telescope in the world when it achieved first light in 1973.  \
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NOIRLab operates the Mayall on behalf of the Dark Energy Spectroscopic Instrument (DESI) survey, a project led by the US Department of Energy’s Office of Science. DESI will measure the effect of dark energy on the expansion of the Universe by repeatedly mapping the distances to 35 million galaxies and 2.4 million quasars across one third of the area of the sky over its five-year run. DESI is the most powerful multi-object survey spectrograph in the world, and will continue to be for several years.
HotspotPanoramaOverlayTextImage_C64FD341_D25D_F871_41D7_3168E2103950.text = The Spacewatch 0.9-meter Telescope is the oldest telescope on Kitt Peak. It was installed in 1923 on the University of Arizona campus and houses the first large telescope mirror successfully cast in the United States. The telescope was then moved to Kitt Peak in 1962.
HotspotPanoramaOverlayTextImage_94BD8514_8E82_21D6_41D2_FFCD6982E4E0.text = The UArizona 12-meter Telescope was previously a European prototype antenna for the Atacama Large Millimeter/submillimeter Array (ALMA). Originally from the European Southern Observatory, it was transported to the Kitt Peak National Observatory in Arizona in 2013. This telescope is the only millimeter-wavelength telescope in the US operated full-time as a national facility and is now part of the Event Horizon Telescope (EHT). \

HotspotPanoramaOverlayTextImage_A71708AD_B9DC_0063_41D1_BCC8823F68C3.text = The UArizona Bok 2.3-meter Telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona.
HotspotPanoramaOverlayTextImage_CD867082_D1C4_78F2_41D5_E0C4015EFAA0.text = The VLBA Dish is controlled remotely from the Science Operations Center in Socorro, New Mexico. Each VLBA station consists of a 25-meter antenna and an adjacent control building. 
HotspotPanoramaOverlayTextImage_A7867330_B9AC_0060_41A9_02A6C50D53EB.text = The Very Long Baseline Array Dish at Kitt Peak is part of the National Radio Astronomy Observatory’s VLBA interferometer. The array consists of 10 identical antennas, separated by distances from 200 kilometers to a transcontinental 8600 kilometers (with the longest baseline between Maunakea, Hawai‘i and St. Croix, Virgin Islands). 
HotspotPanoramaOverlayTextImage_E30EB3FC_C2B7_38D2_417F_FF666D79CD25.text = The Visitor Center 0.5-meter Telescope is used for a variety of nighttime observing programs for the public. The telescope is a Ritchey-Chretien design that delivers an outstanding image for both visual and photographic purposes.  \

HotspotPanoramaOverlayTextImage_9F7BDB15_3EA9_1884_41BF_94069770AE6C.text = The WIYN 3.5-meter Telescope is the second-largest telescope on Kitt Peak.  \
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NOIRLab operates the 3.5-meter WIYN Telescope on behalf of the  partnership between Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s NOIRLab, and NASA).  \
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Its NEID instrument is designed to measure the motion of nearby stars with extreme precision, with the potential to uncover Earth-mass exoplanets.  \
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HotspotPanoramaOverlayTextImage_63F743AB_234C_B589_41B5_7A8B7378DB37.text = The WIYN 3.5-meter Telescope is the second-largest telescope on Kitt Peak. The WIYN telescope is operated by NOIRLab on behalf of Indiana University, the University of Wisconsin, Pennsylvania State University, the University of California Irvine, Purdue University, NSF’s NOIRLab, and NASA. WIYN currently hosts NEID, a radial velocity instrument designed to measure the motion of nearby stars with extreme precision. The Visitor Center Levine 0.4-meter Telescope is used for public viewing by the Kitt Peak Visitor Center. The WIYN 0.9-meter Telescope is a short walk up the hill.
HotspotPanoramaOverlayTextImage_9AAA1750_B96C_0021_41E4_F56763144815.text = The Winter Milky Way arches high over three telescopes on Kitt Peak. These telescopes are (from left to right) The Burrell Schmidt Telescope, the 0.9-meter SARA Kitt Peak Telescope and Kitt Peak National Observatory's Visitor Center Roll Off Roof Observatory. The pillar of the Zodiacal Light can be seen in this image as well. Visitors to Kitt Peak’s evening program watch the sunset from this area. 
HotspotPanoramaOverlayTextImage_9ACDF8BB_B964_0067_41E5_71A6883F01BB.text = The arch of the winter Milky Way can be seen to the right of the Nicholas U. Mayall 4-meter Telescope. 
HotspotPanoramaOverlayTextImage_150B92BE_3EEF_0984_41C7_4AD0D333404C.text = The calibration screen is used for astro-imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects.  \

HotspotPanoramaOverlayTextImage_7649028D_23C4_B789_41BF_9CA2FAF8B47C.text = The distinctive dome of the Nicholas U. Mayall 4-meter Telescope can be seen over 80 kilometers (50 miles) away. This telescope was the second largest in the world upon its completion and has been producing ground-breaking science for almost 50 years. It is currently equipped with Department of Energy’s Dark Energy Spectroscopic Instrument (DESI). 
HotspotPanoramaOverlayTextImage_BC9C13FC_8E82_2057_41D3_030F7D7C4029.text = The heliostats at the top of the McMath-Pierce reflect sunlight down to the primary mirrors. The largest heliostat is 2.03 meters in diameter and reflects light to a 1.61-meter mirror. The two smaller heliostats measure 1.07 meters in diameter and feed light to 0.91-meter primary mirrors. All three heliostats can observe the Sun simultaneously. 
HotspotPanoramaOverlayTextImage_973F30D5_8E86_2056_41D8_F969B4D09A8D.text = The subtle band of the winter Milky Way can be seen along the horizon below the telescopes of Kitt Peak National Observatory. The Nicholas U. Mayall 4-meter Telescope and the UArizona Bok 2.3-meter Telescope are in the foreground, with distant telescopes in the background. The lights of Sells, Arizona can be seen in this image. Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land. Also seen is the faint glow of the Zodiacal light and Gegenschein arching across the sky — faint reflections of sunlight from dust particles in the Solar System. \

HotspotPanoramaOverlayTextImage_1E2CB374_7D24_25BC_41CE_495571B9732D.text = The sundial teaches visitors to tell the time using the Sun.
HotspotPanoramaOverlayTextImage_A6610655_B9A4_0020_41C2_E5A9701CCBFB.text = The totally eclipsed Moon can be seen here just to the right of the Nicholas U. Mayall 4-meter Telescope. This image was created with a camera modified to bring out the red glow of hydrogen gas which can be seen in abundance in the winter Milky Way arching over the Mayall Telescope. 
HotspotPanoramaOverlayTextImage_985F5016_B95C_0021_41D7_68E9017A1662.text = The winter Milky Way arches above the SARA (Southeastern Association For Research In Astronomy) 0.9-meter Telescope. The Zodiacal light can be seen as a bright pillar in the western sky. The Zodiacal light is caused by sunlight reflecting off interplanetary dust. 
HotspotPanoramaOverlayTextImage_16313530_2145_9296_41C0_DF4008B99AAC.text = The winter Milky Way arches high over the dome of the Mayall 4-meter Telescope. The Zodiacal light can be seen to the right of the Mayall reaching up toward the Milky Way. The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
HotspotPanoramaOverlayTextImage_99FCA620_B9A4_0060_41D4_3EC6C43F41BE.text = The winter Milky Way arches over the McMath-Pierce Solar Telescope. The specially modified camera reveals the red nebulosity. The McMath-Pierce Solar Telescope is currently being transformed into the Windows On the Universe Center For Astronomy Outreach. 
HotspotPanoramaOverlayTextImage_156E3E37_7D64_1FBC_41B0_82A6FD590E6B.text = This computer allows the telescope operator to control the telescope and the imaging camera(s) attached to the telescope. \

HotspotPanoramaOverlayTextImage_2A6F4E34_386B_D66D_41A1_3CEC3913EB6E.text = Total Lunar Eclipse
HotspotPanoramaOverlayTextImage_DDD02EE0_DA84_40F3_41EB_00DB74912E3B.text = Total Lunar Eclipse \
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HotspotPanoramaOverlayTextImage_C831C7F1_D24C_582E_41E1_0947A38CCAE1.text = UArizona 0.9-meter  \
Spacewatch Telescope \
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HotspotPanoramaOverlayTextImage_6B873938_2B09_E1D2_41A3_DF089295FE16.text = UArizona 0.9-meter Telescope
HotspotPanoramaOverlayTextImage_217FA6E6_4172_6525_41BB_83D895930FFF.text = UArizona 0.9m Telescope
HotspotPanoramaOverlayTextImage_2215B419_4172_24EF_41C6_A4708D22DDBC.text = UArizona 12-m  \
Telescope
HotspotPanoramaOverlayTextImage_76968B0B_2B7A_E1B6_41C3_871A21B242F5.text = UArizona 12-meter Telescope
HotspotPanoramaOverlayTextImage_DE032D97_D984_415C_41EA_126EBB5BDF86.text = UArizona 12-meter Telescope \
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HotspotPanoramaOverlayTextImage_C0519537_D244_D812_41E2_EE75F3CF115C.text = UArizona ARO 12-meter Telescope \
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HotspotPanoramaOverlayTextImage_C60F7017_D24C_5812_41D5_637606FD176A.text = UArizona Bok  \
2.3-meter Telescope \
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HotspotPanoramaOverlayTextImage_2E5E8762_4152_635D_41A4_BD3726C8F21D.text = UArizona Bok 2.3-m Telescope
HotspotPanoramaOverlayTextImage_103110C7_2B1F_20BE_41BC_0C922680CD4F.text = UArizona Bok 2.3-meter Telescope
HotspotPanoramaOverlayTextImage_D8D5CBF3_DA8F_C0D4_41D1_E67504930192.text = UArizona Bok 2.3-meter Telescope \

HotspotPanoramaOverlayTextImage_C2673D84_D24C_48F6_41D0_818C5F3E99B6.text = UArizona Spacewatch 0.9-meter Telescope \
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HotspotPanoramaOverlayTextImage_23AF549C_4172_65E5_41CD_FB31B6E4F485.text = Very Long  \
Baseline Array Dish
HotspotPanoramaOverlayTextImage_C436CF2A_D684_4177_41E2_7E71CD3F355D.text = Very Long  \
Baseline Array Dish \
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HotspotPanoramaOverlayTextImage_DE3496A7_D98C_437C_41E2_AFCF67EE3181.text = Very Long Baseline Array Dish \

HotspotPanoramaOverlayTextImage_D8EE90E1_DA9C_40F5_41E5_AF6D92EAA16B.text = Very Long Baseline Array Dish \

HotspotPanoramaOverlayTextImage_DE4D01E3_D99C_40F5_41E2_25EE55CB7278.text = Very Long Baseline Array Dish \
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HotspotPanoramaOverlayTextImage_DD5A8482_DB84_4734_41D3_E20DCDD93E15.text = Very Long Baseline Array Dish \
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HotspotPanoramaOverlayTextImage_C3B09C31_D784_4755_41E7_6502FC04CC71.text = Visitor Center  \
Interior
HotspotPanoramaOverlayTextImage_DDF31A14_DA84_435E_41E5_D1D9C7B1FE8E.text = Visitor Center 0.5-meter Telescope \
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HotspotPanoramaOverlayTextImage_F01751DB_D784_40D5_41AB_6322C5ABD8B3.text = Visitor Center Interior
HotspotPanoramaOverlayTextImage_1F323C9E_7D24_236C_41C1_EEB81E8A552F.text = Visitors to Kitt Peak can relax and enjoy lunch outside the Visitor Center. \

HotspotPanoramaOverlayTextImage_C0BCF60D_D24C_3BF6_41E6_7B70C2212F9F.text = WIYN 0.9-meter \
Telescope \
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HotspotPanoramaOverlayTextImage_0E5380C2_2907_60B6_41B5_F134BB9D7F80.text = WIYN 2.1-meter \
Telescope \
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HotspotPanoramaOverlayTextImage_0F76F80B_2909_EFB6_41AB_FE5C49AC7897.text = WIYN 3.5-meter Telescope Interior
HotspotPanoramaOverlayTextImage_00286486_291B_E0BE_41BD_785400E44C5F.text = WIYN 3.5-meter Telescope Interior
HotspotPanoramaOverlayTextImage_255AE997_4172_2FE3_41B3_3CACA0DD223A.text = WIYN Telescopes Exterior
HotspotPanoramaOverlayTextImage_DC02CC79_D985_C7D5_41C7_B1BD4D7A6A32.text = WIYN Telescopes Exterior
HotspotPanoramaOverlayTextImage_2A31E771_3F56_58C8_41CC_2700E1A81B1D.text = Welcome to Kitt Peak National Observatory. \
A birds eye view of Kitt Peak taken before the June 2022 Contreras Fire.  \
Click here for more info
HotspotPanoramaOverlayTextImage_2234EAE7_7D2C_24DC_41B6_E2E162B1C4A2.text = Welcome to Kitt Peak National Observatory. \
Click here for more info
HotspotPanoramaOverlayTextImage_F8E3932F_C8E2_3A18_41E3_AE6AD538E20F.text = —Active Surface— \
The UArizona 12-meter Telescope has an active surface. Actuators maintain the parabolic shape of the dish to keep the telescope focused accurately. 
HotspotPanoramaOverlayTextImage_BD8D31FF_9E90_D1B4_41D6_E3C0BB6FCFBA.text = —Calibration Screen—  \
The calibration screen is illuminated with light sources with known properties to help astronomers to properly calibrate their images and spectra.  \

HotspotPanoramaOverlayTextImage_FC2D2101_C8DE_560B_41E6_F7DFBFCAF076.text = —Calibration screen— \
The calibration screen is used for astro-imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects. 
HotspotPanoramaOverlayTextImage_B31948AD_A186_AB0F_41D3_7DC31E01F0A3.text = —Calibration screen—  \
The calibration screen is used for astro imaging. To properly calibrate images, the screen is evenly illuminated by a calibration lamp. The illuminated surface is imaged with the telescope and allows the image to be corrected for a variety of defects. 
HotspotPanoramaOverlayTextImage_A57AAC13_D1C4_C811_41E9_8AA6B7CF84D1.text = —Dorm 1— \
Several dorms on Kitt Peak allow astronomers to spend the night during their observing runs.
HotspotPanoramaOverlayTextImage_F3D09882_D1C4_48F2_41D9_5E22375A2B7D.text = —Eclipsed Moon— \
 The totally eclipsed Moon shows up next to the Mayall Telescope.
HotspotPanoramaOverlayTextImage_FBF5B997_D1FC_C811_41CE_BB8D8DDFFB46.text = —Eclipsed Moon— \
The totally eclipsed Moon shows up below the McMath-Pierce Solar Telescope. 
HotspotPanoramaOverlayTextImage_DD43D638_DB8B_C354_41E1_385F738046F8.text = —Gegenschein— \
Click here to learn more
HotspotPanoramaOverlayTextImage_FED44CC2_C8AE_4E08_4193_9D1C5AA70620.text = —Heliostats—  \
The three heliostats reflect light to the primary mirrors. 
HotspotPanoramaOverlayTextImage_914039A1_3F67_1BBC_41CD_BFA3F96B59DB.text = —McMath-Pierce Solar Telescope— \
For many years the largest solar telescope in the world, the iconic McMath-Pierce Solar Telescope, is a triple telescope. In addition to the primary 1.61-meter mirror fed by the 2.03-meter heliostat, there are a pair of telescopes fed by 0.81-meter heliostats mounted beside the main heliostat. These two instruments have 1.07-meter and 0.91-meter primary mirrors. The telescope used the heliostat at the top of its main tower to direct the Sun’s light down a long shaft to the primary mirrors. The distinctive diagonal shaft continues far underground, where the telescope’s primary mirror is located.  \
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The facility is named to honor astronomers Keith Pierce and Robert McMath. \
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Scientific research stopped at the McMath-Pierce Solar Telescope in 2017 and it now houses the NOIRLab Windows on the Universe Center for Astronomy Outreach.
HotspotPanoramaOverlayTextImage_FB945288_C8FE_FA19_41E1_821994E99EF8.text = —Model of McMath-Pierce Solar Telescope— \
 This cutaway model of the McMath-Pierce Solar Telescope shows the optical path that light takes through the facility and shows the underground portion of the telescope. 
HotspotPanoramaOverlayTextImage_E585B49E_C8AE_DE38_41E0_524ADF1096E1.text = —Nicholas U. Mayall 4-meter Telescope— \
It is the largest optical telescope on Kitt Peak. The Mayall telescope currently hosts the Department of Energy’s Dark Energy Spectroscopic Instrument (DESI), the most powerful multi-object survey spectrograph in the world. 
HotspotPanoramaOverlayTextImage_190DCCB5_8764_3CBC_41D8_80C26AB5A5C0.text = —Optical Tunnel— \
The heliostat (mirror) at the top of the telescope reflects light down the optical tunnel. Less than half of the optical tunnel is visible as it extends approximately another 90 meters (300 feet) underground! \

HotspotPanoramaOverlayTextImage_B8A7E736_9E77_32B4_41C0_A2C3303D119E.text = —Original Control Room—  \
This control room was used until the installation of the DESI instrument and the construction of the DESI control room. This control room is still used for testing and engineering. 
HotspotPanoramaOverlayTextImage_F8A3C4B9_C8E2_DE78_41C6_D1E3FD1AA185.text = —Sells, Arizona— \
 Sells is the capital of the Tohono O’odham Nation. Kitt Peak National Observatory is located on Tohono O’odham Nation land.
HotspotPanoramaOverlayTextImage_1EE36A8D_3EF8_F984_41C6_9192197B8A2C.text = —Solar viewing area—  \
Three solar telescopes are located around the corner which allow visitors to view the Sun through several filters, including white-light, hydrogen-alpha, and calcium-K.  \
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HotspotPanoramaOverlayTextImage_83B95A40_9CA3_0065_41DC_833505FEF0ED.text = —The Robotically Controlled Telescope—  \
The telescope has been operated by the RCT Consortium, led by Western Kentucky University since 2006. 
HotspotPanoramaOverlayTextImage_F8CC0B13_C8DE_4A08_41E8_4958E91DD500.text = —UArizona Bok 2.3-meter Telescope— \
It was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona. It is the largest optical telescope operated solely by Steward Observatory.
HotspotPanoramaOverlayTextImage_B2242E1D_9E71_3274_41D4_55F395984963.text = —UArizona Bok 2.3-meter Telescope—  \
This telescope was named after astronomer Bart Bok, a previous director of Steward Observatory, part of the University of Arizona. It is the largest optical telescope operated solely by Steward Observatory.
HotspotPanoramaOverlayTextImage_8DF9A8A5_9781_16BF_41BE_58601BCFFE3A.text = —Zodiacal light— \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
HotspotPanoramaOverlayTextImage_4126F111_38F4_C781_41C7_856074D4712D.text = —Zodiacal light— \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
HotspotPanoramaOverlayTextImage_F4FE3FEA_D1CC_4832_41E5_165AFD9B9555.text = —Zodiacal light— \
The Zodiacal light is caused by sunlight reflecting off dust grains orbiting the Sun in the plane of the Solar System.
HotspotPanoramaOverlayTextImage_4E4E5E1D_06F4_F86E_417C_76DEC0E6B624.text = ― Gum Nebula 
HotspotPanoramaOverlayTextImage_5AA9F862_D3BB_E5C0_41E9_8777A215EEC0.text = ― Polaris
HotspotPanoramaOverlayTextImage_5F313959_D3D9_A7C3_41E7_1C45E768717F.text = ― Regulus
HotspotPanoramaOverlayTextImage_553E4384_D3E8_EB40_41B9_B2BF4A2591BD.text = ― Sirius  \
(brightest star in the night sky)
HotspotPanoramaOverlayTextImage_C1272135_D244_3816_41E5_2E5581CAC40B.text = ―Calypso 1.2-meter Telescope
HotspotPanoramaOverlayTextImage_C11BB221_D27D_D82E_41E3_C6F942E0DE77.text = ―Very Long Baseline Array Dish
HotspotPanoramaOverlayTextImage_C0903375_D244_5816_41A9_909803BC2562.text = ―WIYN 3.5-meter Telescope
HotspotPanoramaOverlayTextImage_5C480929_D3D8_A743_41DD_D8018FAC2DEA.text = ∣ \
Flaming star nebula \
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HotspotPanoramaOverlayTextImage_058C0947_2907_E1BE_41AF_D716C72AABBA.text = │ \
UArizona Bok 2.3-meter Telescope

### Tooltip
HotspotPanoramaOverlayArea_13385697_8724_6F7C_41DE_A57EF472F4D5.toolTip = Click here to go to DESI webpage
HotspotPanoramaOverlayArea_09299AB3_7B6C_24B4_41D4_607BEB8123C7.toolTip = Click on the logo to go to the NEID webpage
HotspotPanoramaOverlayArea_123FC1CD_7B24_24EC_41D3_62FCE1C4E629.toolTip = Info about SOLARIO
HotspotPanoramaOverlayArea_02051E16_8724_1F66_41D8_A9DD272C6F75.toolTip = Info about Visitor Center Levine 0.4-meter Telescope
HotspotPanoramaOverlayArea_0372C471_86E4_23B4_41D7_8CF58514A2E4.toolTip = Info about WIYN 0.9-meter Telescope
HotspotPanoramaOverlayArea_E0D8B8B7_C867_D608_41BE_C8008D6ED3EF.toolTip = Open Webpage of The Dark Energy Spectroscopic Instrument
HotspotPanoramaOverlayArea_0637F4F6_26C4_939B_41BD_1930D532878F.toolTip = Open webpage about Tucson light pollution
HotspotPanoramaOverlayArea_E09DBBFA_C866_49F8_41C5_929E1E171027.toolTip = Open webpage of Community Science and Data Center Program
HotspotPanoramaOverlayArea_E25A6445_C866_3E08_41E1_82715A31F1F9.toolTip = Open webpage of Community Science and Data Center Program
HotspotPanoramaOverlayArea_6CBED59A_D9BC_4157_41AF_AFF40D907123.toolTip = Open webpage of Galactic Immigration in the Andromeda Galaxy
HotspotPanoramaOverlayArea_6929710B_D984_4135_41D7_D7F0F3814887.toolTip = Open webpage of the image
HotspotPanoramaOverlayArea_6F3DEFAD_D9BC_C14D_41AC_96DB38926514.toolTip = Open webpage of the image
HotspotPanoramaOverlayArea_AA94B013_D3E8_A540_41E3_A407A7C7452F.toolTip = See Milky Way over McMath
HotspotPanoramaOverlayArea_D0CED6FF_42D6_2523_41C9_B8A69B27421D.toolTip = See a photo of 2022 Contreras Fire at KPNO
HotspotPanoramaOverlayArea_C2FE2C29_42D2_652F_41D1_125BA34FA0BF.toolTip = See a photo of 2022 Contreras Fire at KPNO
HotspotPanoramaOverlayArea_61E81177_D99C_41DD_41E6_708673F092CB.toolTip = See a photo of Dr. Roger Lynds lying on the floor of the Cassegrain cage, taken in 1975.
HotspotPanoramaOverlayArea_D5FE516F_42D2_FF23_41B7_D223798E53F0.toolTip = See a photo of Kitt Peak in Recovery
HotspotPanoramaOverlayArea_61721D86_D684_C13F_41E8_53861040782F.toolTip = See a photo of Nicholas U. Mayall Mirror
HotspotPanoramaOverlayArea_6BFE66C4_D984_4333_41E8_6D5D63AC15BA.toolTip = See a photo of telescope operator preparing the telescope for a night of observing by cooling the instrumentation with liquid nitrogen.
HotspotPanoramaOverlayArea_7D592936_D68C_C15F_41C7_40061B4EDAF0.toolTip = See a photo of the Original Control Room
HotspotPanoramaOverlayArea_D910A146_DB84_413C_41E0_83CE4EE95516.toolTip = See a photo of the back of the telescope's primary mirror, showing the complex control systems for the active optics and mirror cooling.
HotspotPanoramaOverlayArea_141CD6D6_873C_2CFC_41D1_10822120E209.toolTip = See a photo of this view at night
HotspotPanoramaOverlayArea_1A3E9F5D_8724_1DEC_41E0_1BD0BB3D6010.toolTip = See a photo taken from here at night
HotspotPanoramaOverlayArea_D913B86D_DB84_4FCD_41D0_B62D0ADE4431.toolTip = See close-up photos of different sides of the telescope

## Media

### Floorplan

### Image
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### Popup Image

### Subtitle
panorama_77C64199_7AFD_EA61_41DD_73BF3081C877.subtitle = The Gemini North Base Facility control room is where all of the nightly observations take place. From here typically two staff members would operate the telescope and execute the scientific plan for the night or que. 

### Title
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panorama_610E2D3D_7772_DF9B_41DA_7DB5CC69FC2F.label = Milkyway Over Kitt Peak
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panorama_7828B6F9_74F3_5605_41DA_81D88A7F10EE.label = UArizona 12-m Telescope
panorama_7AFC677A_74CD_D607_41DC_50B7970F4CE7.label = UArizona Bok 2.3-m Telescope
panorama_7ADC5006_74D3_2A0F_41D2_1DB1329DD5D0.label = Very Long Baseline Array Dish
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video_698ACD61_58DE_06F8_41CE_908F0CA8B62D.label = gemini_demo_real_goebel
photo_F726F517_D9BB_D882_41C0_D7D4A9AC0528.label = iotw2237a
photo_9295A429_3F79_088C_41C4_05B0C51AE061.label = noao-sundog11

### Video
videolevel_CD7CEE63_EF2E_300A_41BD_AFCB54380C53.url = media/video_698ACD61_58DE_06F8_41CE_908F0CA8B62D_en.m3u8
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### Video Subtitles

## Popup

### Body
htmlText_11A483A7_7B1C_655C_419F_8DC8F72A4AED.html = <div style="text-align:left; color:#000; "><HTML><BODY><DIV STYLE="text-align:left;font-size:0.8333333333333334vw;"><SPAN STYLE="display:inline-block; letter-spacing:0vw; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:0.83vw;font-family:'Quatro';">This 0.38-meter telescope is used strictly for imaging. It can be controlled either onsite where it is housed or via the Internet. The public can rent time on the telescope no matter where they live and engage in remote imaging.</SPAN></SPAN></DIV></BODY></HTML></div>
htmlText_3F297A67_4136_2D23_41AD_931DC4476C91.html = <div style="text-align:left; color:#000; "><HTML><BODY><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Have you ever looked up at the sky and noticed a beautiful halo encircling the sun? This is called a solar halo, or 22 degree halo, for the reason that its apparent radius is approximately 22 degrees. It will always appear with the same radius no matter its position in the sky, and is roughly the length of an outstretched hand held at arm’s length.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">A solar halo forms from the refracted sunlight of hexagonally shaped ice crystals high in the atmosphere. Often, these ice crystals can be found suspended in cirrus or cirrostratus clouds within the upper troposphere. Because these clouds usually form right before a storm, solar halos have been used as an indication of oncoming rain in the past — however, cirrus and cirrostratus clouds can occur at any given time without a direct change in weather, thus disproving its reliability.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">This particular halo appeared in the sky near the offices of the National Solar Observatory in Tucson, Arizona, on June 27, 2006. Luckily, a palm tree was around to help obscure the sun for safe viewing!</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Credit:</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Peter Marenfeld and NSO/AURA/NSF</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/images/noao-sundog11/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;">Download &amp; More Info</A></SPAN></SPAN></DIV></BODY></HTML></div>
htmlText_03B876EF_8725_ECAC_41D5_2690320B3B41.html = <div style="text-align:left; color:#000; "><HTML><BODY><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Have you ever looked up at the sky and noticed a beautiful halo encircling the sun? This is called a solar halo, or 22 degree halo, for the reason that its apparent radius is approximately 22 degrees. It will always appear with the same radius no matter its position in the sky, and is roughly the length of an outstretched hand held at arm’s length.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">A solar halo forms from the refracted sunlight of hexagonally shaped ice crystals high in the atmosphere. Often, these ice crystals can be found suspended in cirrus or cirrostratus clouds within the upper troposphere. Because these clouds usually form right before a storm, solar halos have been used as an indication of oncoming rain in the past — however, cirrus and cirrostratus clouds can occur at any given time without a direct change in weather, thus disproving its reliability.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">This particular halo appeared in the sky near the offices of the National Solar Observatory in Tucson, Arizona, on June 27, 2006. Luckily, a palm tree was around to help obscure the sun for safe viewing!</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Credit:</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Peter Marenfeld and NSO/AURA/NSF</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/images/noao-sundog11/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;">Download &amp; More Info</A></SPAN></SPAN></DIV></BODY></HTML></div>
htmlText_FAA33334_872C_25BC_41DC_0CC8F6E89D24.html = <div style="text-align:left; color:#000; "><HTML><BODY><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Have you ever looked up at the sky and noticed a beautiful halo encircling the sun? This is called a solar halo, or 22-degree halo, for the reason that its apparent radius is approximately 22 degrees.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">A solar halo forms from the refracted sunlight of hexagonally shaped ice crystals high in the atmosphere. Often, these ice crystals can be found suspended in cirrus or cirrostratus clouds within the upper troposphere. Because these clouds usually form right before a storm, solar halos have been used as an indication of oncoming rain in the past — however, cirrus and cirrostratus clouds can occur at any given time without a direct change in weather, thus disproving its reliability.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;"> </SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">This particular halo appeared in the sky near the offices of the NOIRLab HQ in Tucson, Arizona, on 27 June 2006. Luckily, a palm tree was around to help obscure the Sun for safe viewing!</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">Credit:</SPAN></SPAN></DIV><DIV STYLE="text-align:left;font-size:1.4814814814814814vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;font-size:1.48vmin;">NOIRLab/NSF/AURA/P. Marenfeld</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#999999;"/></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/images/noao-sundog11/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;">Download &amp; More Info</A></SPAN></SPAN></DIV></BODY></HTML></div>
htmlText_2A19C79D_3F56_5878_419D_50034BA57FDA.html = <div style="text-align:left; color:#000; "><HTML><BODY><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">Founded in 1958, Kitt Peak National Observatory (KPNO) is home to one of the largest collections of optical and radio telescopes in the world. KPNO hosts the facilities of consortia that, between them, operate more than a dozen optical telescopes and two radio telescopes.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-family:'Quatro';"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">KPNO is located 90 kilometers (56 miles) southwest of Tucson, Arizona, at an altitude of 2096 meters (6877 feet) in the Schuk Toak District on the Tohono O'odham Nation. It has a visitor center that is open daily and nightly to the public, offering daytime guided tours and a variety of evening stargazing programs.</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-family:'Quatro';"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">We are privileged to conduct research on I’oligam Du’ag (Kitt Peak) in Arizona and acknowledge the Tohono O'odham Nation as the caretakers of the jewed (land).</SPAN></SPAN></DIV><DIV STYLE="text-align:left;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-family:'Quatro';"/></SPAN></DIV><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">The images for this Virtual Tour were taken before the 2022 Contreras Fire, which affected KPNO. Read more</SPAN><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/news/noirlab2213/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;"><SPAN STYLE="font-family:'Quatro';"> here</SPAN></A></SPAN><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">.</SPAN></SPAN></DIV></BODY></HTML></div>
htmlText_FAB2E8A4_86E4_235D_41D8_49E989310BEC.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:left;font-size:0.8333333333333334vw;"><SPAN STYLE="display:inline-block; letter-spacing:0vw; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:0.83vw;font-family:'Quatro';">In 2001 the WIYN Consortium assumed operational responsibility for the historic 0.9-meter (36-inch) telescope at Kitt Peak National Observatory. </SPAN></SPAN></DIV></div>
htmlText_062431C6_8724_24DC_41CE_3C251AB88E27.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:left;font-size:0.8333333333333334vw;"><SPAN STYLE="display:inline-block; letter-spacing:0vw; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:0.83vw;font-family:'Quatro';">This telescope is used by the Kitt Peak Visitor Center for a variety of public observing programs. </SPAN></SPAN></DIV></div>
htmlText_1DEF9085_7D2C_635C_41B5_BE35118F77AB.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">Founded in 1958, Kitt Peak National Observatory (KPNO) is home to one of the largest collections of optical and radio telescopes in the world. KPNO hosts the facilities of consortia that, between them, operate more than a dozen optical telescopes and two radio telescopes.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">KPNO is located 90 kilometers (56 miles) southwest of Tucson, Arizona, at an altitude of 2096 meters (6877 feet) in the Schuk Toak District on the Tohono O'odham Nation. It has a visitor center that is open daily and nightly to the public, offering daytime guided tours and a variety of evening stargazing programs.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">We are privileged to conduct research on I’oligam Du’ag (Kitt Peak) in Arizona and acknowledge the Tohono O'odham Nation as the caretakers of the jewed (land).</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">The images for this Virtual Tour were taken before the 2022 Contreras Fire, which affected KPNO. Read more</SPAN><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/news/noirlab2213/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;"><SPAN STYLE="font-family:'Quatro';"> here</SPAN></A></SPAN><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">.</SPAN></SPAN></DIV></div>
htmlText_22404AF4_7D2C_24BC_41D8_036169F34524.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">Founded in 1958, Kitt Peak National Observatory (KPNO) is home to one of the largest collections of optical and radio telescopes in the world. KPNO hosts the facilities of consortia that, between them, operate more than a dozen optical telescopes and two radio telescopes.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">KPNO is located 90 kilometers (56 miles) southwest of Tucson, Arizona, at an altitude of 2096 meters (6877 feet) in the Schuk Toak District on the Tohono O'odham Nation. It has a visitor center that is open daily and nightly to the public, offering daytime guided tours and a variety of evening stargazing programs.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">We are privileged to conduct research on I’oligam Du’ag (Kitt Peak) in Arizona and acknowledge the Tohono O'odham Nation as the caretakers of the jewed (land).</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">The images for this Virtual Tour were taken before the 2022 Contreras Fire, which affected KPNO. Read more</SPAN><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/news/noirlab2213/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;"><SPAN STYLE="font-family:'Quatro';"> here</SPAN></A></SPAN><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">.</SPAN></SPAN></DIV></div>
htmlText_1FA471EC_7DE5_E4D3_41CD_87EAF40375E3.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">Founded in 1958, Kitt Peak National Observatory (KPNO) is home to one of the largest collections of optical and radio telescopes in the world. KPNO hosts the facilities of consortia that, between them, operate more than a dozen optical telescopes and two radio telescopes.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">KPNO is located 90 kilometers (56 miles) southwest of Tucson, Arizona, at an altitude of 2096 meters (6877 feet) in the Schuk Toak District on the Tohono O'odham Nation. It has a visitor center that is open daily and nightly to the public, offering daytime guided tours and a variety of evening stargazing programs.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">We are privileged to conduct research on I’oligam Du’ag (Kitt Peak) in Arizona and acknowledge the Tohono O'odham Nation as the caretakers of the jewed (land).</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:16px;"><BR STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-size:16px;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:left;font-size:16px;"><SPAN STYLE="display:inline-block; letter-spacing:0px; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">The images for this Virtual Tour were taken before the 2022 Contreras Fire, which affected KPNO. Read more</SPAN><SPAN STYLE="color:#f3a22e;"><A HREF="https://noirlab.edu/public/news/noirlab2213/" TARGET="_blank" STYLE="text-decoration:none; color:inherit;"><SPAN STYLE="font-family:'Quatro';"> here</SPAN></A></SPAN><SPAN STYLE="color:#cccccc;font-size:16px;font-family:'Quatro';">.</SPAN></SPAN></DIV></div>

### Title
window_6F359FB4_D9BC_C153_41DE_93C7F43760E9.title = A slice through the 3D map of galaxies from DESI
window_69D1610E_D984_414F_41D5_9BFD9CADE12F.title = Andromeda Galaxy with DESI Overlay and Spectrum
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window_CC6EA5C2_42DE_675D_41C6_2033C1B8D3DE.title = Contreras Fire at KPNO
window_D0C3C717_42D6_24E3_41AD_CE68807A73A5.title = Contreras Fire at KPNO
window_D5FF8172_42D2_FF3D_41C4_A3123896A000.title = Contreras Fire at KPNO
window_6E304519_D9BC_C155_41C7_6BF5DDD5E843.title = Galactic Immigration in the Andromeda Galaxy
window_2246BAF7_7D2C_24BC_41B5_4DF291B59327.title = Kitt Peak National Observatory
window_1FA1E1F4_7DE5_E4B3_41DE_4079DB013677.title = Kitt Peak National Observatory
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window_11AAB3A9_7B1C_6554_41DA_D81C5E906B2B.title = SOLARIO
window_FAA3C335_872C_25BC_41CF_DDF76352A8F7.title = Solar Halo
window_3F2B0A65_4136_2D24_41A5_C58CE85BB4D9.title = Solar Halo
window_03B8C6F0_8725_ECB4_41CC_D0246F2D584F.title = Solar Halo
window_E3B88DF2_C862_CE08_41B7_D24CAB1A911C.title = The Dark Energy Spectroscopic Instrument (DESI)
window_E19D1197_C863_D637_419F_3C16691BF7D6.title = The Dark Energy Spectroscopic Instrument (DESI)
window_062211C8_8724_24D4_41D6_D6E11284EDDD.title = Visitor Center Levine 0.4-meter Telescope
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### Multiline Text
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letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Project Lead:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Joy Pollard</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Design &amp; Development:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Mahdi Zamani</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Photography:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Petr Horálek</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Tomáš Slovinský</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Theofanis Matsopoulos</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Joy Pollard</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Peter Michaud </SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Technical Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Mark Newhouse</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Content Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Manuel Paredes</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Joy Pollard</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Leonor Opazo</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Robert Sparks</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Peter Michaud</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Daniel Munizaga</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Andy Adamson</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Kristen Metzger</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Ranpal Gill</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Peter Marenfeld</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Jameeka Marshall</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Color Correction:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Maral Kosari</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Amirreza Kamkar</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Map Design:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Peter Marenfeld</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Text Editing:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Peter Grimley</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Web Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Enciso Systems</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Spanish translation:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Carolina Vargas</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Spanish Proofreading:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Leonor Opazo</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Manuel Paredes</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Executive Producer:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Lars Lindberg Christensen</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:0.6899999999999995vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;">━━━━━━━━━━━━━━━━━━━━━━━━━━━━</SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Powered by 3DVista</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:0.6899999999999995vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;">━━━━━━━━━━━━━━━━━━━━━━━━━━━━</SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">A special thank-you to the NOIRLab staff in all locations for their support of the photo expedition and for beta-testing the virtual tours.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:0.69vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Maunakea</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">The staff and researchers who use the Gemini North telescope in Hawai‘i are honored to have the opportunity to conduct astronomical research on Maunakea in Hawai‘i. We recognize and acknowledge the very significant cultural role and reverence that Maunakea has to the Native Hawaiian community.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Cerro Tololo and Cerro Pachón</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">The staff and researchers are honored to have the opportunity to conduct astronomical research on Cerro Pachón and Cerro Tololo. We recognize and acknowledge the significant cultural role that Cerro Tololo/Pachón has to the communities in Chile.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';"><B>Kitt Peak</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:1.520912547528517vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="font-size:1.52vmin;font-family:'Quatro Medium';">Kitt Peak National Observatory sits atop I’oligam Du’ag. Astronomers are honored to be permitted to conduct scientific research on I’oligam Du’ag (Manzanita Bush Mountain), in the homeland of the Tohono O’odham Nation. We honor their past, present, and future generations, who have lived here for time immemorial and will forever call this place home.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:1.52vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:0.69vmin;font-family:Arial, Helvetica, sans-serif;"/></p></div>
HTMLText_11FA881A_3F90_3B3E_41C4_6253C5493BB6.html = <div style="text-align:left; color:#000; "><DIV STYLE="text-align:center;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro';">Pause/resume </SPAN></SPAN></DIV><DIV STYLE="line-height:130%;text-align:center;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro';">tour autoplay</SPAN></SPAN></DIV><DIV STYLE="line-height:130%;text-align:center;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro SemiBold';">│</SPAN></SPAN></DIV></div>
HTMLText_4C0C3CF8_5EE8_88BE_41D5_8EEACF3D5601.html = <div style="text-align:left; color:#000; "><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:6.666666666666668vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:6.67vmin;font-family:'Quatro SemiBold';"><B>NSF’s NOIRLab</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:6.666666666666668vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:6.67vmin;font-family:'Quatro SemiBold';"><B>Virtual Tour v2.0</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:6.67vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:4.4444444444444455vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#0069a7;font-size:4.44vmin;font-family:'Quatro';">Last Updated: 30 September, 2023</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:5.56vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Light';"><B>Communications, Education &amp; Engagement</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Project Lead:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Joy Pollard</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Design &amp; Development:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Mahdi Zamani</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Photography:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Petr Horálek</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Tomáš Slovinský </SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Theofanis Matsopoulos</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Joy Pollard</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Peter Michaud</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Technical Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Mark Newhouse</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Content Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Manuel Paredes</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Joy Pollard</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Leonor Opazo</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Robert Sparks</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Peter Michaud</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Daniel Munizaga</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Andy Adamson</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Kristen Metzger</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Ranpal Gill</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Peter Marenfeld</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Jameeka Marshall</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Color Correction:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Maral Kosari</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Amirreza Kamkar</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Map Design:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Peter Marenfeld</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Text Editing:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Peter Grimley</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Web Support:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Enciso Systems</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Spanish translation:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Carolina Vargas</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Spanish Proofreading:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Leonor Opazo</SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Manuel Paredes</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Executive Producer:</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">Lars Lindberg Christensen</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>―――</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Powered by 3DVista</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">―――</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">A special thank-you to the NOIRLab staff in all locations for their support of the photo expedition and for beta-testing the virtual tours.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Maunakea</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">The staff and researchers who use the Gemini North telescope in Hawai‘i are honored to have the opportunity to conduct astronomical research on Maunakea in Hawai‘i. We recognize and acknowledge the very significant cultural role and reverence that Maunakea has to the Native Hawaiian community.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Cerro Tololo and Cerro Pachón</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';">The staff and researchers are honored to have the opportunity to conduct astronomical research on Cerro Pachón and Cerro Tololo. We recognize and acknowledge the significant cultural role that Cerro Tololo/Pachón has to the communities in Chile.</SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Kitt Peak</B></SPAN></SPAN></DIV><DIV STYLE="text-align:center;font-size:3.333333333333334vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:3.33vmin;font-family:'Quatro Medium';"><B>Kitt Peak National Observatory sits atop I’oligam Du’ag. Astronomers are honored to be permitted to conduct scientific research on I’oligam Du’ag (Manzanita Bush Mountain), in the homeland of the Tohono O’odham Nation. We honor their past, present, and future generations, who have lived here for time immemorial and will forever call this place home.</B></SPAN></SPAN></DIV><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p><p STYLE="margin:0; line-height:3.33vmin;"><BR STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-size:2.52vmin;font-family:Arial, Helvetica, sans-serif;"/></p></div>
HTMLText_3175CC17_3E88_DAD5_41B4_3BE7C68F82BE.html = <div style="text-align:left; color:#000; "><DIV STYLE="line-height:100%;text-align:left;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro SemiBold';">│</SPAN></SPAN></DIV><DIV STYLE="line-height:100%;text-align:left;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro SemiBold';">│</SPAN></SPAN></DIV><DIV STYLE="line-height:115%;text-align:left;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro';"> Click on the logos </SPAN></SPAN></DIV><DIV STYLE="line-height:115%;text-align:left;font-size:1.6717325227963522vmin;"><SPAN STYLE="display:inline-block; letter-spacing:0vmin; white-space:pre-wrap;color:#000000;font-family:Arial, Helvetica, sans-serif;"><SPAN STYLE="color:#ffffff;font-size:1.67vmin;font-family:'Quatro';"> for a simple view</SPAN></SPAN></DIV></div>
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### Tab Panel
TabPanelPage_57928E48_58AC_7842_417B_35944656D9FE.label = Google Map
TabPanelPage_03CAF617_147B_164D_419E_C39DA82D338B.label = Google Map
TabPanelPage_03CA5613_147B_1645_4197_6AF41ACC169D.label = NOIRLab Map
TabPanelPage_57924E43_58AC_7846_41C2_544CE9795D47.label = NOIRLab Map

### Tooltip
IconButton_CE59CE95_D6AB_20AD_41EA_6B3A9E7BE00D_mobile.toolTip = Change Language
IconButton_D823699D_D6AD_20DC_41E7_19B70E3771F4.toolTip = Change Language
Image_9BDDACF3_8F77_FFC6_41BF_808FF2086761.toolTip = Click for a simple view
CloseButton_841D7B8C_9230_2967_41B7_07A02287AB32.toolTip = Close Map
IconButton_2B90E40F_3593_B9CB_41B4_408768336038.toolTip = Credits & Tutorial
IconButton_CE106960_D6D7_2063_41D4_19FDACC73DD9_mobile.toolTip = English
IconButton_D9101C1B_D6B5_67A5_41D1_69B0AC8A05F2.toolTip = English
IconButton_D9117C1E_D6B5_67DF_41AD_A53451A16104.toolTip = Español
IconButton_CE13A961_D6D7_2065_41D2_AA2140708E65_mobile.toolTip = Español
IconButton_2B90A410_3593_B9D5_41B7_0B5CCA80EF0F.toolTip = Google Maps Version
IconButton_5EDC17A6_604A_587C_41CE_0915E511670B.toolTip = Gyroscope Freeze
IconButton_EE9FBAB2_E389_8E06_41D7_903ABEDD153A.toolTip = Gyroscope Freeze
IconButton_DB0435A4_ED2A_2632_41E7_1439E3141256.toolTip = Hide/Show Hotspots
IconButton_1AF35943_2D07_479B_41AF_FBC8A1477882.toolTip = Hide/Show side bar
IconButton_2B917411_3593_B9D7_41C6_8D1102463EC5.toolTip = Kitt Peak image gallery
IconButton_2A159B11_35B0_EFD6_41C9_DF408F8120FF.toolTip = Kitt Peak video gallery
ProgressBar_710F1F4B_654C_178E_41D0_77FB38325D47.toolTip = Loading Full Resolution 
ProgressBar_2F751036_3E99_4AD7_41CD_8291B56580B2.toolTip = Loading Full Resolution 
IconButton_95EE7A9C_8F09_53F8_41D1_7CB6714A3C00.toolTip = Map
IconButton_5EDC27A6_604A_587C_41C8_D1CC8B401FB7.toolTip = Mute / Disable Text to Speech
IconButton_EED073D3_E38A_9E06_41E1_6CCC9722545D.toolTip = Mute / Disable Text to Speech
Container_D977F156_D754_D883_41E6_472808BA6C70.toolTip = Navigation
Container_7033997C_654C_1B89_41A9_CC55029D5AFB.toolTip = Navigation
Image_0435F73B_2D0F_4BF4_4181_65F86A8DAC19.toolTip = Open program webpage
Image_772A13EA_655C_F6AA_41C3_821BE7A5A910.toolTip = Open website
IconButton_05821A49_1F4B_F689_418B_73E1575421A0.toolTip = Other NOIRLab Virtual Tours
IconButton_18872D79_17E2_54D6_41B6_DE5222FF2E91.toolTip = Other NOIRLab Virtual Tours
ThumbnailList_995B2C0C_8F97_21F9_41D7_C89980C1A418.toolTip = Select the place you want to visit.  \
Scroll down to see more.
IconButton_EED5213F_E3B9_7A7D_41D8_1B642C004521.toolTip = Share view on Facebook
IconButton_EE5807F6_E3BE_860E_41E7_431DDDA54BAC.toolTip = Share view on Twitter
IconButton_EF7806FA_E38F_8606_41E5_5C4557EBCACB.toolTip = VR mode

## Tour

### Description

### Title
tour.name = Kitt Peak National Observatory, Arizona V2.0