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NGC428 by Hubble Space Telescope. NGC 428 was discovered by William Herschel in December 1786. [3] A type Ia supernova designated SN2013ct was discovered May 11, 2013, within the galaxy by Stuart Parker of the Backyard Observatory Supernova Search (BOSS) project in Australia and New Zealand.
It is a part of the Mount Graham International Observatory. When using both 8.4 m (330 inch) wide mirrors, with centres 14.4 m apart, the LBT has the same light-gathering ability as an 11.8 m (464 inch) wide single circular telescope and the resolution of a 22.8 m (897 inch) wide one. [1]
This is a list of large optical telescopes. For telescopes larger than 3 meters in aperture see List of largest optical reflecting telescopes . This list combines large or expensive reflecting telescopes from any era, as what constitutes famous reflector has changed over time.
The Backyard Observatory Supernova Search (BOSS) is conducted by astronomers from Australia and New Zealand since mid 2008 to search for new supernovae in the southern hemisphere. [2] In 2022 the group won the Astronomical Society of Australia's Page Medal [ 3 ] for having found around 200 confirmed supernovas.
This table does not include all the largest mirrors manufactured. The Steward Observatory Mirror Lab produced the 6.5 metre f/1.25 collimator used in the Large Optical Test and Integration Site of Lockheed Martin, used for vacuum optical testing of other telescopes. Segmented mirrors are also referred to as mosaic mirrors. Single mirrors are ...
Big Bear Lake Solar Observatory: 1969 Big Bear City, California, US Bisdee Tier Optical Astronomy Observatory: 2010 Bisdee Tier, Spring Hill, Tasmania, Australia Black Moshannon Observatory (defunct) 1972 Pennsylvania, US Blackett Observatory: 1930s Wiltshire, England, UK Blue Mesa Observatory (defunct) 1967 New Mexico, US Boambee Observatory: 1987
Comparison of nominal sizes of apertures of the Overwhelmingly Large Telescope and some notable optical telescopes. The Overwhelmingly Large Telescope (OWL) was a conceptual design by the European Southern Observatory (ESO) organisation for an extremely large telescope, which was intended to have a single aperture of 100 metres in diameter.
The Wide Field Survey Telescope (WFST) is a Chinese telescope characterized by a 2.5-metre primary mirror, [1] dedicated to time-domain surveys, tracking objects that change during observation such as supernovae. [2] It saw first light on 17 September 2023 when the WFST imaged the Andromeda Galaxy. [3]