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201. http://site2010.sai.msu.ru/static/doc/DAfshari.pdf
Measurement of Sky Brightness at the Iranian National Observatory Davoud Afshari1 and Sadollah Nasiri1,2 1Physics Department, Zanjan University, Zanjan 45195-313, Iran; Institute for Advanced studies in Basic Science (IASBS), Zanjan 45195-1159, Iran; Measurement of light pollution 2 Introduction Among 34 candidate sites at the central part of the country, 5 sites namely Garkesh (in Kashan ), Kolahbarfi(in Kashan ), Deynava (in ... One of these is light pollution. ...
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Ссылки http://site2010.sai.msu.ru/static/doc/DAfshari.pdf -- 472.0 Кб -- 27.10.2010
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202. CCD Astronomy Magazine Article Page 5
Example 2: Figure 8 (90 Kbytes) shows an image of M31. While this is not a particularly spectacular image of M31 it is nevertheless unique as it was taken in a suburban backyard using a Lynxx CCD camera. The exposure is unfiltered. ... The image scale in this system is 41 arcseconds per pixel which yields a total field size of 2.2 x 1.9 square degrees. At this pixel resolution M32 blends into the light of M31, although NGC 205 (marked with a red arrow) is plainly visible. ... Page 6 . ...
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Ссылки http://zebu.uoregon.edu/CCDast5.html -- 4.3 Кб -- 07.10.1996
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203. http://www.atnf.csiro.au/nca/University%20Infrastructure.pdf
... Role of the Facility The Mt Pleasant and Ceduna antennas play an important role in the Australian Long Baseline Array, a national facility operated jointly by the Australia Telescope National Facility and the University of Tasmania. ... When not participating in VLBI observations the telescopes are in constant use for staff and student research projects and as a teaching facility for undergraduate students. ... It is envisioned that the wide-field optical telescope will be used in transit mode. ...
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Ссылки http://www.atnf.csiro.au/nca/University%20Infrastructure.pdf -- 401.5 Кб -- 20.09.2005
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