Optical Astronomy
Our best articles related to Optical astronomy
Previous, UTAS owned, observatory on Mt. Canopus was heavily light-polluted by nearby city of Hobart, this lead a need for choosing new site for the astronomical observations from Tasmania. Location in Southern Midlands region of Tasmania was chosen, under Dr John Greenhill's advisory, for it's...
The main focus of dome design is its thermal properties - the aim is to maximally lower air turbulence generated by the building and the telescope and to ensure the telescope temperature is as close to ambient temperature as possible. The dome has low thermal capacity with forced ventilation....
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Previous, UTAS owned, observatory on Mt. Canopus was heavily light-polluted by nearby city of Hobart, this lead a need for choosing new site for the astronomical observations from Tasmania. Location in Southern Midlands region of Tasmania was chosen, under Dr ...
Bisdee Tier Optical Astronomy Observatory is an astronomical facility being build by the University of Tasmania (UTAS) on Bisdee Tier, Spring Hill, Tasmania. The observatory will be a host for 1.27 m optical telescope. Adapted from the Wikipedia article Bisdee ...
* In 2011 mosaic 8192×8192 pixels OGLE-III camera will be installed with collaboration with Optical Gravitational Lensing Experiment (OGLE) team in the primary folded Cassegrain focus. Camera consist of 8 thin SITe 2048×4096 CCD chips. The pixel scale is 0.27 ...
National Optical Astronomy Observatory (NOAO) is the United States public access observatory for ground based nighttime astronomy. The National Science Foundation (NSF) funds NOAO to provide forefront astronomical research facilities for US astronomers. However, professional astronomers from any country in ...
The main focus of dome design is its thermal properties – the aim is to maximally lower air turbulence generated by the building and the telescope and to ensure the telescope temperature is as close to ambient temperature as possible. ...
The telescope has a diameter of 1.27 m (50 inches). The primary mirror made from fused silica 8″ thick. The mount for the telescope is equatorial. Design consist of a folded Cassegrain reflector with f/9 and 40 arcminute of corrected ...
NOAO operates world class research telescopes in both the northern and southern hemispheres. These telescopes are located at Kitt Peak and Cerro Tololo in the US and Chile, respectively. Complemented with similar astronomical instruments, the two sites allow US astronomers ...
National Astronomy Observatory of China (NAOC, the acronym was officially claimed as standing for National Astronomical Observatories, Chinese Academy of Sciences) was founded on April 25, 2001 through the merging of four CAS observatories, three CAS observing stations and one ...
astronomical interferometer is an array of telescopes or mirror segments acting together to probe structures with higher resolution by means of interferometry. Astronomical interferometers are widely used for optical astronomy, infrared astronomy, submillimetre astronomy and radio astronomy. Aperture synthesis can ... At the beginning of the new millennium, the National Academy of Sciences published its report on Astronomy and Astrophysics in the coming decade. Among other high priorities, the committee responsible for the report concluded [4]: “U.S. ground-based optical and infrared ...
reflecting telescope (also called a reflector) is an optical telescope which uses a single or combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century as an alternative to the ...
Leuschner Observatory, originally called the Students’ Observatory, is an observatory operated by the University of California, Berkeley. The observatory was built in 1886 on the Berkeley campus. For many years, it was directed by Armin Otto Leuschner, for whom the ...
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