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Astrophysical Research Consortium Telescope | 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 | | | | 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 | observe celestial objects | 43° 39' N | altazimuth telescope | f/4, 30 | | Mount Pastukhov, Russia | 2100 m | LOMO | Special Astrophysical Obs. | LOMO | | concave hyperboloid | | 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 | convex hyperboloid | |
Gemini Telescope North | 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 | | concave hyperboloid | | 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 | | | convex hyperboloid | |
Gemini Telescope South | 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 | | concave hyperboloid | | 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 | | | convex hyperboloid | |
Gran Telescopio Canarias | 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 | concave hyperboloid | | 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 | | | convex hyperboloid | |
Hobby-Eberly Telescope | 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 | | | | 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 | | | | |
Keck | 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 | | concave hyperboloid | | 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) | | | convex hyperboloid | |
Large Binocular Telescope | 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 | concave paraboloid | | 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 | | | convex hyperboloid | |
Magellan Project | 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 | | | | 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 | 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 | | | | 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 | 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 | | | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | Cer-Vit | | 2.3 m | | | | | 1984 | | altazimuth | 149° 03' E | | | | |
New Technology Telescope | 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 | concave hyperboloid | | 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 | | | convex hyperboloid | |
Nordic Optical Telescope | 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 | concave paraboloid | | 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 | | | convex hyperboloid | |
Sloan Digital Sky Survey Telescope | 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 | concave hyperboloid | | 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 | convex hyperboloid | |
Southern African Large Telescope | 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 | | | 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 | 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 | | concave hyperboloid | | 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 | convex hyperboloid | |
Telescopio Nazionale Galileo | 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 | | concave hyperboloid | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | Zerodur | | 3.58 m | | | | | (1998) | | altazimuth | 17° 54'W | | Galileo | convex hyperboloid | |
Very Large Telescope | 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 | concave hyperboloid | | 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 | | | convex hyperboloid | 8.2 m |
William Herschel Telescope | 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 | | | 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 | 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 | | | | 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 | | |