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Southern Astrophysical Research Telescope

Coordinates:30°14′17″S70°44′01″W / 30.238°S 70.73372°W /-30.238; -70.73372
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(Redirected fromSOAR Telescope)
Observatory in Chile
Southern Astrophysical Research Telescope
SOAR Telescope, as seen at evening twilight
Alternative namesSOAREdit this at Wikidata
Location(s)Vicuña,Elqui Province,Coquimbo Region, Chile
Coordinates30°14′17″S70°44′01″W / 30.238°S 70.73372°W /-30.238; -70.73372Edit this at Wikidata
Altitude2,738 m (8,983 ft)Edit this at Wikidata
Diameter4.1 m (13 ft 5 in)Edit this at Wikidata
Websitenoirlab.edu/science/programs/ctio/telescopes/soar-telescopeEdit this at Wikidata
Southern Astrophysical Research Telescope is located in Chile
Southern Astrophysical Research Telescope
Location of Southern Astrophysical Research Telescope
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TheSouthern Astrophysical Research (SOAR) telescope is a modern 4.1-meter-aperture (13 ft) optical andnear-infrared telescope located onCerro Pachón, Chile, at 2,738 metres (8,983 ft) elevation. It was commissioned in 2003, and is operated by a consortium including the countries ofBrazil andChile,Michigan State University, theCerro Tololo Inter-American Observatory (CTIO) (part of theNational Optical Astronomy Observatory, NOAO), and theUniversity of North Carolina at Chapel Hill. Partners have guaranteed shares varying from 10 to 30 percent of the observing time.

The telescope usesactive optics on its primary and secondary mirrors to attain median image quality 0.7 arcsec at a wavelength of 500 nm. Multiple instruments are available on standby, mounted at unusually high weight-capacityNasmyth foci and two lower capacity bent-Cassegrain foci. Switching is accomplished within a few minutes by rotating the 45° tertiary mirror. The pointing of this mirror is adjusted at high speed to prevent image blur from vibrations induced by wind-shake of the telescope structure.

Overview

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Its optical specifications are:

  • M1 total diameter 4300mm
  • Entrance Pupil Diameter4100mm
  • Pupil central Obstruction 980mm
  • M1working f/# 1.6855 (no prime focus is available)
  • Focal plane working f/# 16.625
  • Effective Focal Length 68176.3mm
  • Gamma ratio (dZ(foc)/dZ(M2))100.5
  • Zero-Vignetting Field Diameter14.4arcmin
  • Focal Plane Radius of curvature966.3mm
  • Sag w/r to Maximum Field10.59mm[1]

Instruments

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Current (5/2014) instruments are:

  • UV–optical 16-million pixel imager (SOI, CTIO)
  • near-infrared (1–2.4 μm wavelength) 1-million pixelHgCdTe imager and spectrograph (OSIRIS, Ohio State University/CTIO)
  • UV–optical 16-million pixel imager and spectrograph (Goodman Spectrograph, UNC)
  • near-infrared (1–2.4 μm wavelength) 16-million pixel HgCdTe imager (SPARTAN, MSU)
  • adaptive optics module (SAM, CTIO)

Additional facility instruments are being commissioned:

  • UV–optical 16-million pixel integral-field spectrograph (SIFS, Brazil)

User instruments are employed by individual astronomers or teams but not available to all users.

US astronomers access the telescope remotely over theInternet 2. Chilean and Brazilian astronomers use their high-speed networks. An on-site operator controls where the telescope points while the remote astronomer controls the instrument and data retrieval.

The SOAR telescope dome is a $2 million, 66-foot-diameter (20 m), weatherproof structure weighing over 70 tons.[2]

Gallery

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  • SOAR Below the Milky Way
    SOAR Below theMilky Way
  • This image shows stars appearing to "trail" around the south celestial pole (at the center of the circles) above the Southern Astrophysical Research Telescope
    This image shows stars appearing to "trail" around the south celestial pole (at the center of the circles) above the Southern Astrophysical Research Telescope

See also

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References

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  1. ^SOAR Telescope Official Site
  2. ^"FEA Roundup: Design, Simulation and Analysis Converge",Composites World, 4/1/2007, archived fromthe original on 2008-11-23

External links

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