Stripe 82
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Stripe 82
Stripe 82 is a 300 deg2 equatorial field of sky that was imaged multiple times by the Sloan Digital Sky Survey from 2000 to 2008.Abazajian et al., ''THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY'', The Astrophysical Journal Supplement Series, 182:543–558, 2009 June It approximately covers the region with right ascension from 20:00h to 4:00h and declination from -1.26° to +1.26°. Stripe 82 has also been observed using many other telescopes and instruments, a list of which is given below. Current data available on Stripe 82 Imaging ;Optical/UV Imaging * SDSS Co-adds (Jiang, LSST, Huff, Annis) * Canada–France–Hawaii Telescope, CFHT i-band (CS82'') * CFHTLS * The Dark Energy Survey, DES * Subaru Telescope#Instruments, HSC * GALEX ;Near-IR * UKIRT Infrared Deep Sky Survey, UKIDSS * VHS * NEWFIRM (Jiang) * VICS82 (CFHT and VISTA) ;Mid-IR * SHELA * SpIES * Wide-field Infrared Survey Explorer, WISE * IRAC High-z quasars ;Far-IR * HELMS * vHerS ;Radio/mm ...
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Sloan Digital Sky Survey
The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. The project began in 2000 and was named after the Alfred P. Sloan Foundation, which contributed significant funding. A consortium of the University of Washington and Princeton University was established to conduct a redshift survey. The Astrophysical Research Consortium (ARC) was established in 1984 with the additional participation of New Mexico State University and Washington State University to manage activities at Apache Point. In 1991 the Sloan Foundation granted the ARC funding for survey efforts and the construction of equipment to carry out the work.. Background At the time of its design, the SDSS was a pioneering combination of novel instrumentation as well as data reduction and storage techniques that drove major advances in astronomical observations, di ...
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Telescope
A telescope is a device used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. Originally meaning only an optical instrument using lenses, curved mirrors, or a combination of both to observe distant objects, the word ''telescope'' now refers to a wide range of instruments capable of detecting different regions of the electromagnetic spectrum, and in some cases other types of detectors. The first known practical telescopes were refracting telescopes with glass lenses and were invented in the Netherlands at the beginning of the 17th century. They were used for both terrestrial applications and astronomy. The reflecting telescope, which uses mirrors to collect and focus light, was invented within a few decades of the first refracting telescope. In the 20th century, many new types of telescopes were invented, including radio telescopes in the 1930s and infrared telescopes in the 1960s. Etymology The word ''telescope'' was coin ...
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Canada–France–Hawaii Telescope
The Canada–France–Hawaii Telescope (CFHT) is located near the summit of Mauna Kea mountain on Hawaii's Big Island at an altitude of 4,204 meters (13,793 feet), part of the Mauna Kea Observatory. Operational since 1979, the telescope is a Prime Focus/ Cassegrain configuration with a usable aperture diameter of . CFHT currently planning a refurbishment to the facility in the 2020s. The facility will be reconstructed with a new 11-m telescope to produce the Maunakea Spectroscopic Explorer, retaining the same base building and infrastructure. First light is expected in 2029. Funding The corporation is bound by a tripartite agreement between the University of Hawaii at Manoa, in the United States, the National Research Council (NRC) in Canada and the Centre National de la Recherche Scientifique (CNRS) in France. CFHT also has partnerships with the National Astronomical Observatory of China (NAOC), the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) in Taiwan, t ...
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