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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 | | Zerodur | | | 2.33 m | | | | 1985 | | Horseshoe equatorial | 78° 50' E | Vainu Bappu 2.3 m | | |
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 | | 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 | | spin-cast borosilicate honey-comb | | | 3.5 m | | | | 1994 | | altazimuth | 105° 49' W | ARC 3.5 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 | | material and other engineering details | | | 2.64 m | | | | 1976 | | equatorial fork | 44° 18' E | Byurakan 102 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 | | Cer-Vit | | | 3.58 m | | | | 1979 | | Horseshoe equatorial | 155° 28' W | | | |
Cassegrain | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | concave paraboloid | material and other engineering details | | | or primary mirror diameter | Cassegrain | reflector | | | | | | | convex hyperboloid | Telescope devised by Cassegrain in which an auxiliary convex mirror reflects the magnified image, upside down, through a hole in the center of the main objective mirror - i.e., through the end of the telescope itself. It was, however, no improvement on the gregorian telescope invented probably slightly earlier. |
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 | | Fused-silica | | | 3.57 m | | | | 1977 | | Horseshoe equatorial | 70° 44' W | ESO 3.6 m | | |
Gregorian | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | | material and other engineering details | | | or primary mirror diameter | | reflector | | | | | | | concave | Telescope devised - but never constructed - by James Gregory, in which an auxiliary concave mirror reflects the magnified image, the right way up, through a hole in the centre of the main objective mirror, i.e., through the end of the telescope itself. The Cassegrain telescope is similar but produces an inverted image. |
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 | | 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 | | | |
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 | | 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 | | |
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 | | 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 | | |
Maksutov telescope | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | concave spheroid | material and other engineering details | | | or primary mirror diameter | | reflector | | | | | | | | A reflector whose primary mirror is spheroidal instead of parabolic. The light initially passes through a large concave lens to remove the spherical aberration. |
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 | | 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 | | Cer-Vit | | | 2.3 m | | | | 1984 | | altazimuth | 149° 03' E | | | |
Newtonian | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | concave paraboloidal | material and other engineering details | | | or primary mirror diameter | | reflector | | | | | | | plane | A class of reflecting telescope developed by Sir Issac Newton with a paraboloidal primary mirror and a small, plane secondary mirror at 45°; to deflect the focus of the primary to a position outside the tube near the top of the telescope. |
reflector with corrector plate | astroweb | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | | material and other engineering details | | | or primary mirror diameter | | optical telescope | | | | | | | | |
Ritchey-Chrétien | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | concave hyperboloid | material and other engineering details | | | or primary mirror diameter | Ritchey-Chrétien | reflector | | | | | | | convex hyperboloid | A system of two mirrors, aspherized to give an image at the secondary (Cassegrain) focus free from spherical aberration and coma. |
Schmidt | | observe celestial objects | in degrees, minutes, seconds (N or S) | | | | height above sea level in meters | the person, company or institution that constructed the mounting | | the person, company or institution that created the mirror | | ambient | concave spheroid | material and other engineering details | | | or primary mirror diameter | Schmidt | equatorial telescope | | | | equatorial | in degrees, minutes, seconds (E or W) | | none | A type of reflecting telescope (more accurately, a large camera) in which the coma produced by a spherical concave mirror is compensated for by a thin correcting lens placed at the opening of the telescope tube. The Schmidt has a usable field of 0°.6. |
segmented mirror telescope | | observe celestial objects | | | | | | | | the person, company or institution that created the mirror | | | | material and other engineering details | | | or primary mirror diameter | | reflector | | | | | | | | a reflecting telescope whose mirror is composed of multiple segments |
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 | | material and other engineering details | | | 2.64 m | | | | 1960 | | equatorial fork | 34° 00' E | Crimean 102 inch | | |
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 | | 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 | | | |
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 | | 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 | | 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 | | |