Subject |
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2.3-meter Telescope | | astroweb | | observe celestial objects | 12° 35' N | Horseshoe equatorial telescope | f/3.25, 13, 43 | | | | Kavalur, Tamil Nadu, India | 725 m | Walchandnagar Industries | Vainu Bappu Observatory | Indian Inst. Astrophys. | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Zerodur | | | | | 2.33 m | | | | | | | | | | | 1985 | | | Horseshoe equatorial | 78° 50' E | | | | | Vainu Bappu 2.3 m | | | | |
3.5-meter Telescope | | astroweb | | observe celestial objects | 37° 13' N | Horseshoe equatorial telescope | f/3.5, 3.9, 10, 35 | | | | Calar Alto, Spain | 2168 m | Voith, Heidenheim; Zeiss (Ober.) | Calar Alto Observatory | Zeiss (Ober.) | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Zerodur | | | | | 3.50 m | | | | | | | | | | | 1984 | German-Spanish Astronomical Center | | Horseshoe equatorial | 2° 32' W | | | | | | | | | |
Anglo-Australian Telescope | | astroweb | | observe celestial objects | 31° 17' S | Horseshoe equatorial telescope | t/3.3. 8, 15. 36 | | | | Siding Spring Mtn., Australia | 1149 m | Mitsubishi | Anglo-Australian Observatory | Grubb-Parsons | | AAT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 3.893 m | | | | | | | | | | | 1975 | | | Horseshoe equatorial | 149° 04' E | | | | | | | | | |
Astrophysical Research Consortium Telescope | | astroweb | | observe celestial objects | 32° 47' N | altazimuth telescope | f/1.75 | | | | New Mexico, US | 2800 m | the person, company or institution that constructed the mounting | Apache Point | R. Angel, B. Martin | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | spin-cast borosilicate honey-comb | | | | | 3.5 m | | | | | | | | | | | 1994 | | | altazimuth | 105° 49' W | | | | | ARC 3.5 m | | | | |
Bol'shoi Teleskop Azimutal'nyi | | astroweb | | observe celestial objects | 43° 39' N | altazimuth telescope | f/4, 30 | | | | Mount Pastukhov, Russia | 2100 m | LOMO | Special Astrophysical Obs. | LOMO | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Sitall glass | | | | | 6.00 m | | | | | | | | Primary mirror replaced in about 1984, and a third made of Sitall glass was figured in 1992 | | | 1975 | | | altazimuth | 41° 26'E | | | | | 6 m | | | | |
Byurakan 2.6-meter Reflector | | astroweb | | observe celestial objects | 40° 20' N | Fork equatorial telescope | f/3.6, 16, 40 | | | | Mount Aragatz, Armenia | 1500 m | LOMO | Byurakan Observatory | the person, company or institution that created the mirror | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 2.64 m | | | | | | | | | | | 1976 | | | equatorial fork | 44° 18' E | | | | | Byurakan 102 inch | | | | |
C. Donald Shane Telescope | | astroweb | | observe celestial objects | 37° 21' N | Fork equatorial telescope | f/5, 17, 36 | | | | Mount Hamilton, Calif., US | 1290 m | Judson Pacific-Murphy Corp. | Lick Observatory | Don O. Hendrix | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Pyrex | | | | | 3.05 m | | | | | | | | | | | 1959 | | | equatorial fork | 121° 38' W | | | | | 120 inch | | | | |
Canada-France-Hawaii Telescope | | astroweb | | observe celestial objects | 19° 49' N | Horseshoe equatorial telescope | f/3.8, 8, 20, 35 | | | | Mauna Kea, Hawaii, US | 4200 m | SNACRP | Canada-France-Hawaii Telescope Corp. | Dominion Astrophys. Obs. | | CFHT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 3.58 m | | | | | | | | | | | 1979 | | | Horseshoe equatorial | 155° 28' W | | | | | | | | | |
ESO 3.6-meter Telescope | | astroweb | | observe celestial objects | 29° 16' S | Horseshoe equatorial telescope | f/3.0, 8.1, 32 | | | | La Silla, Chile | 2387 m | Creusot-Loire | European Southern Observatory | REOSC | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Fused-silica | | | | | 3.57 m | | | | | | | | | | | 1977 | | | Horseshoe equatorial | 70° 44' W | | | | | ESO 3.6 m | | | | |
Gemini Telescope North | | astroweb | | observe celestial objects | 19° 49' N | altazimuth telescope | f/1.8, 16IR, 19.6 | | | | Mauna Kea, Hawaii, US | 4100: m | the person, company or institution that constructed the mounting | Joint Astronomy Center | the person, company or institution that created the mirror | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 8.1 m | | | | | | | | Coming ULE meniscus primary mirror; this northem instrument is to be optimized for IR work | | | (1999) | | | altazimuth | 155° 28' W | | | | | | | | | |
Gemini Telescope South | | astroweb | | observe celestial objects | 30° 21' S | altazimuth telescope | f/1.8, 6 | | | | Cerro Pachon, Chile | 2725 m | the person, company or institution that constructed the mounting | Cerro Tololo Inter-American Obs. | the person, company or institution that created the mirror | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 8.1 m | | | | | | | | Partners in the Gemini project are the US, UK, Canada, Chile, Brazil, and Argentina | | | (2000) | | | altazimuth | 70° 49' W | | | | | | | | | |
George Ellery Hale Telescope | | astroweb | | observe celestial objects | 33° 21' N | Horseshoe equatorial telescope | f/3.3. 16, 30 | | | | Palomar Mountain, Calif., US | 1706 m | Westinghouse | Palomar Observatory | J.A. Anderson | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | ribbed Corning Pyrex | | | | | 5.08 m | | | | | | | | | | | 1948 | California Institute of Technology | | Horseshoe yoke mount | 116° 52' W | | | | | 200 inch | | | | |
Gran Telescopio Canarias | | astroweb | | observe celestial objects | 28° 45' N | altazimuth telescope | f/1.75. 15, 25 | | | | La Palma, Canary Islands | 2400 m | the person, company or institution that constructed the mounting | Obs. del Roque de los Muchachos | the person, company or institution that created the mirror | | GTC | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 10 m | | | | | | | | Design similar to that of the Keck instruments; funded by Spain with international partners | | | 2003 | | | altazimuth | 17°54' W | | | | | | | | | |
Harlan J. Smith Telescope | | astroweb | | observe celestial objects | 30° 4d N | Cross-axis equatorial telescope | f/3.9, 8.8, 18 | | | | Mount Locke, Texas, US | 2075 m | Westinghouse | McDonald Observatory | Davidson Optronics | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Fused-silica | | | | | 2.72 m | | | | | | | | | | | 1969 | | | Cross-axis equatorial | 104° 01' W | | | | | 107 inch | | | | |
Hiltner Telescope | | astroweb | | observe celestial objects | 31° 57' N | Fork equatorial telescope | f/2.07, 13.5 | | | | Kitt Peak, Arizona, US | 1938 m | DFM Engineering, L & F Industries | Michigan-Dartmouth-MIT Obs. | Contraves (USA) | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 2.34 m | | | | | | | | Mirrors repolished 1991 | | | 1986 | | | Equatorial fork, friction-disk drives | 111° 37' W | | | | | Hiltner 2.3 m | | | | |
Hobby-Eberly Telescope | | astroweb | | spectroscopic survey telescope | 30° 41' N | altazimuth telescope | (f/1.4) f/4.7 | | | | Mount Fowlkes, Texas, US | 2002 m | the person, company or institution that constructed the mounting | University of Texas | Univ. of Texas, Penn. State | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 9.2 m equivalent | | | Spherical figure | | | | | A project of five universities in US and Germany; 91 spherical mirrors with combined focus for spectroscopy | | | 1997 | | | altazimuth fixed in altitude but rotates in azimuth | 104° 01' W | | | | | | | | | |
Hooker Telescope | | astroweb | | observe celestial objects | 34° 13' N | English equatorial telescope | f/5, 16, 30 | | | | Mount Wilson, Calif., US | 1742 m | FG. Pease and Fore River Shipyards | Mount Wilson Observatory | G.W. Ritchey from Saint-Gobain (Paris) | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | plate-glass | | | | | 2.5 m | | | | | | | | telescope out of service 1985-92 | | | 1917 | | | English equatorial | 118° 03' W | | | | | 100 inch | | | | |
Hubble Space Telescope | 1986 | Hubble Space Telescope from CADC | | observe celestial objects | | optical telescope | f/12.9, 30, 48, 96 | | | | Earth orbit | | Lockheed | Space Telescope Science Institute | Perkin Elmer | | HST | | 500 km altitude, 35 degree inclination | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Corning ULE glass | | | | 0.05 arcseconds | 2.4 m | | Earth | | | | 2.1 meters | | | | 300 to 1000 nanometers | 1990 | | | 3-axis-stabilized spacecraft | | | | | | | | Hubble Space Telescope. A space-based reflecting telescope with a primary mirror diameter of 2.4 m (94 in) capable of high-resolution imaging from the far ultraviolet to the near infrared. A joint NASA/ESA mission. Launched in 1990 with a planned lifetime of 15 years. Encountered reduced performance when the mirror was found to have spherical aberration. Solved by the installation of corrective optics (COSTAR) in 1994. | | |
Irénée du Pont Telescope | | astroweb | | observe celestial objects | 29° 00' S | Fork equatorial telescope | f/3.0 | | 1.45 degrees | | Las Campanas, Chile | 2282 m | Bruce H. Rule | Las Campanas Observatory | Donald A. Loomis | 0.0924 mm/arcsec | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | 741 mm | fused-silica | | | 19050 mm | | 2.54 m | 9.042 mm | | | 1013 mm | | | | | 953 mm | | 1976 | Carnegie Inst. of Washington | 826 mm | equatorial fork | 70° 42' W | | | 3% | 5153 mm | du Pont 100 inch | 7620 mm | | | 2540 mm |
Isaac Newton Telescope | | astroweb | | observe celestial objects | 28° 46' N | Polar-disk equatorial telescope | f/3, 15 | | | | La Palma, Canary Islands | 2336 m | Grubb-Parsons | Obs. del Roque de Ins Muchachos | Grubb-Parsons | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 2.5 m mirror | | | | | | | | originally set up in England in 1967 | | | 1984 | Royal Greenwich Observatory | | equatorial with polar-disk | 17° 53' W | | | | | Isaac Newton 98 inch | | | | |
Keck | | astroweb | | observe celestial objects | in degrees, minutes, seconds (N or S) | | f/1.75, 15, 25 IR | | | | Mauna Kea, Hawaii, US | height above sea level in meters | TIW Systems | W.M. Keck Observatory | Itek, Tinsley | | | ambient | | | 9.82 m | | Zerodur | 36 | | | | or primary mirror diameter | | | | | | | Ritchey-Chrétien | Uses 36 hexagonal mirror segments. Plans include using both Keck I and Keck II as an optical interferometer | | | 1991 | Univ. of California and Calif. Institute of Technology | | altazimuth | in degrees, minutes, seconds (E or W) | | | | | | | | | |
Large Binocular Telescope | | astroweb | | observe celestial objects | 32° 42' N | altazimuth telescope | f/1.14, 5.4, 15 (each) | | | | Mount Graham, Arizona, US | 3170 m | the person, company or institution that constructed the mounting | Columbus Project | R. Angel, B. Martin | | LBT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 11.8 m | | | | | | | | Twin 8.4-m reflectors; a project of Univ. of Arizona, Arcetri Astrophysical Obs., and Research Corp. (Tucson) | | | 2004 | | | altazimuth "two-shooter" with telescopes 14.4 m apart (center to center) | 109° 51' W | | | | | | | | | |
Magellan Project | | astroweb | | observe celestial objects | 29° 00' S | altazimuth telescope | f/1.25, 11, 15 | | | | Las Campanas, Chile | 2300 m | L & F Industries | Las Campanes Observatory | R. Angel, B. Martin | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 6.5 m | | | Cassegrain and Gregorian | | | | | a twin, Magellan II is to be built in 2001 | | | (1999) | Carnegie Institution of Washington | | altazimuth | 70° 42' W | | | | | Magellan I | | | | |
MMT Telescope | | astroweb | | observe celestial objects | 31° 41' N | altazimuth telescope | f/1.25, 5.4, 9, 15 | | | | Mount Hopkins, Arizona, US | 2608 m | de Bartolomeis | MMT Observatory | R. Angel, B. Martin | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Spin-cast borosilicate honey-comb | | | | | 6.5 m | | | | | | | | | | | (1999) | Smithsonian Institution and Univ. of Arizona | | altazimuth | 110° 53' W | | | | | | | | | |
Mount Stromlo 2.3-meter | | astroweb | | observe celestial objects | 31 ° 16' S | altazimuth telescope | f/2.09, 18 | | | | Siding Spring Mtn., Australia | 1149 m | Australian National Univ., Newcastle Dockyard | Mt. Stromlo and Siding Spring Obs. | Norman Cole | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 2.3 m | | | | | | | | | | | 1984 | | | altazimuth | 149° 03' E | | | | | | | | | |
NASA Infrared Telescope Facility | | astroweb | | infrared work | 19° 50' N | English equatorial telescope | f/2.5, 35, 120 IR | | | | Mauna Kea, Hawaii, US | 4208 m | de Bartolomeis | Mauna Kea Observatory | KPNO Optical Shop | | NASA IRTF | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 3.00 m | | | | | | | | | | | 1979 | | | English equatorial | 155° 28' W | | | | | | | | | |
New Technology Telescope | | astroweb | | observe celestial objects | 29° 16' S | altazimuth telescope | U2.2, 11 | | | | La Silla, Chile | 2353 m | the person, company or institution that constructed the mounting | European Southern Observatory | Zeiss | | NTT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | thin Zerodur | | | | | 3.50 m | | | | | | | | mirror figure controlled by 78 active supports | | | 1989 | | | altazimuth | 70° 44' W | | | | | | | | | |
Nicholas U. Mayall Reflector | | astroweb | | observe celestial objects | 31° 58' N | Horseshoe equatorial telescope | f/2.7, 8, 15.7 IR, 190 | | | | Kitt Peak, Arizona, US | 2120 m | Western Gear Corp. | Kitt Peak National Observatory | KPNO Optical Shop | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Fused-quartz | | | | | 3.81 m | | | | | | | | | | | 1973 | | | Horseshoe equatorial | 111° 36' W | | | | | Kitt Peak 4 m | | | | |
Nordic Optical Telescope | | astroweb | | observe celestial objects | 28° 45' N | altazimuth telescope | (f/2.0), 11.0 | | | | La Palma, Canary Islands | 2382 m | the person, company or institution that constructed the mounting | Obs. del Roque de Ins Muchachos | Optics Labs (Tartu) | | NOT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Zerodur | | | | | 2.56 m | | | | | | | | | | | 1989 | | | altazimuth in rotating building | 17° 53'W | | | | | | | | | |
optical space telescope | | astroweb | | observe celestial objects | | | | | | | | | | | | | | | | | | | | | | | | | | a more massive physical object | | | | | optical telescope | | | 300 to 1000 nanometers | | | | | | | | | | | | | | |
reflector with corrector plate | | astroweb | | observe celestial objects | | | | | | | | | | | the person, company or institution that created the mirror | | | | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | or primary mirror diameter | | | | | | | optical telescope | | | | | | | | | | | | | | | | | |
refractor | | astroweb | the person, company or institution that created the lens | observe celestial objects | | | | | | | | | | | | | | | | | | | | | | | | | | | visual refractor | | | | optical telescope | | | | | | | | | doublet | | | | | | A device for gathering and amplifying light by means of a lens. | | |
Shajn 2.6-m Reflector | | astroweb | | observe celestial objects | 44° 44' N | Fork equatorial telescope | f/3.8, 15.7, 16.4, 40 | | | | Nauchny, Ukraine | height above sea level in meters | the person, company or institution that constructed the mounting | Crimean Astrophysical Obs. | the person, company or institution that created the mirror | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 2.64 m | | | | | | | | | | | 1960 | | | equatorial fork | 34° 00' E | | | | | Crimean 102 inch | | | | |
Sloan Digital Sky Survey Telescope | | astroweb | | observe celestial objects | 32° 47' N | altazimuth telescope | | | | | Apache Point, New Mexico, US | 2800 m | L & F Industries and University of Washington | Astrophys. Res. Consortium Obs. | the person, company or institution that created the mirror | | SDSS | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 2.5 m | | | | | | | | To take CCD imagery of a quarter of sky in 5 colors (u, g, r, i, z) and measure redshifts of 1 million galaxies | | | (1998) | | | altazimuth | 105° 49' W | | | | | Sloan 2.5 m | | | | |
Southern African Large Telescope | | astroweb | | observe celestial objects | 32° 23' S | altazimuth telescope | (f/1.4) f/4.7 | | | | Sutherland, South Africa | 1798 m | the person, company or institution that constructed the mounting | South African Astronomical Obs. | the person, company or institution that created the mirror | | SALT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 9.1 m | | | Spherical figure | | | | | A twin of the Hobby-Eberly Telescope | | | (2004) | | | altazimuth fixed in altitude but rotates in azimuth | 20° 49'E | | | | | | | | | |
Subaru Telescope | | astroweb | | observe celestial objects | 19° 49' N | altazimuth telescope | f/1.8, 12.5, 35 | | | | Mauna Kea, Hawaii, US | 4215 m | Mitsubishi | National Astronomy Obs. (Japan) | the person, company or institution that created the mirror | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | material and other engineering details | | | | | 8.3 m | | | | | | | | Thin primary (Coming ULE) under active control | | | (1999) | | | altazimuth | 155° 28' W | | | | | Subaru | | | | |
Telescopio Nazionale Galileo | | astroweb | | observe celestial objects | 28° 45' N | altazimuth telescope | f/2.5, 6, 11 | | | | La Palma, Canary Islands | 2370 m | the person, company or institution that constructed the mounting | Obs. del Roque de los Muchachos | Zeiss | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Zerodur | | | | | 3.58 m | | | | | | | | | | | (1998) | | | altazimuth | 17° 54'W | | | | | Galileo | | | | |
UBC-Laval Telescope | | astroweb | | observe celestial objects | 49° 07' N | fixed vertical mount telescope | f/1.887 | views a 21' field at local zenith (centered on declination +49° 1) | | | Vancouver, BC, Canada | 50 m | Univ. of British Col. | Univ. of B.C. and Laval Univ. | P Hickson | | LMT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | rotating liquid mercury container | | | | | 2.7 m | | | Paraboloid, field corr. | | | | | | | | 1992 | | | fixed vertical | 122° 35' W | | | | | | | | | |
United Kingdom Infrared Telescope | | astroweb | | infrared work only | 19° 50' N | English equatorial telescope | f/2.5, 36 IR | | | | Mauna Kea, Hawaii, US | 4194 m | Hadfields Ltd. (Sheffield) | Joint Astronomy Centre | Grubb-Parsons | | UKIRT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 3.802 m | | | | | | | | | | | 1978 | | | English-yoke equatorial | 155° 28' W | | | | | | | | | |
Very Large Telescope | | astroweb | | observe celestial objects | 24° 51' S | array telescope | f/13.5, 15 (each mirror) | | | | Cerro Paranal, Chile | 2640 m | the person, company or institution that constructed the mounting | European Southern Observatory | REOSC | | VLT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Schott Zerodur, active optics | | | | | 16 m equivalent | | | | | 4 | | | Four separate telescopes and domes, first unit became operational in 1998 | | | 2001 | | | altazimuth | 70° 27' W | | | | | | | | 8.2 m | |
Victor M. Blanco Telescope | | astroweb | | observe celestial objects | 30° 10' S | Horseshoe equatorial telescope | f/2.8, 8.0 | | | | Cerro Tololo, Chile | 2215 m | Western Gear Corp. | Cerro Tololo Inter-American Obs. | KPNO Optical Shop | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Cer-Vit | | | | | 4.001 m | | | | | | | | | | | 1976 | | | Horseshoe equatorial | 70° 49' W | | | | | CTIO 4 meter | | | | |
William Herschel Telescope | | astroweb | | observe celestial objects | 28° 46' N | altazimuth telescope | 02.5, 11 | | | | La Palma, Canary Islands | 2332 m | Grubb-Parsons | Obs. del Roque de los Muchachos | Grubb-Parsons | | WHT | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Owens-Illinois Cer-Vit | | | | | 4.2 m | | | | | | | | | | | 1987 | Royal Greenwich Observatory | | altazimuth | 17° 53' W | | | | | | | | | |
Wisconsin-Indiana-Yale-NOAO Telescope | | astroweb | | observe celestial objects | 31° 57' N | altazimuth telescope | (f/1.75) f/6.3 | | | | Kitt Peak, Arizona. US | 2089 m | L & F Industries | WIYN Observatory | Charles Harmer/NOAO | | | ambient | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | spin-cast borosilicate honey-comb | | | | | 3.5 m | | | | | | | | mirror by Steward Observatory Mirror Lab (R. Angel) | | | 1994 | | | altazimuth | 111° 36' W | | | | | WIYN 3.5 m | | | | |