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201. 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 . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/CCDast5.html -- 4.3 Кб -- 07.10.1996
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202. http://www.mso.anu.edu.au/~kcf/pubs_top20/94.pdf
... Printed in U.S.A. OPTICAL AND RADIO OBSERVATIONS OF THE AFTERGLOW FROM GRB 990510: EVIDENCE FOR A JET F. A. Harrison,1 J. S. Bloom,1 D. A. Frail,2 R. Sari,3 S. R. Kulkarni,1 S. G. Djorgovski,1 T. Axelrod ... . McConnell,5 P. J. McCarthy,6 B. E. Schaefer,7 R. G. McMahon,8 R. O. Markze,6 E. Firth,8 P. Soffitta,9 and L. Amati10 Received 1999 July 12; accepted 1999 August 2; published 1999 September 7 ABSTRACT We present multicolor optical and two-frequency ... 1999; Amati et al. ... 1999)...
[ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/94.pdf -- 76.2 Кб -- 16.10.2011
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203. ADASS 2002 Conference Proceedings
... New technologies have made it possible to construct an affordable radio telescope with collecting area of one square km: the SKA. ... In particular, there was a transition (about 1980) from large single dishes to arrays of smaller dishes. ... Figure 3: ATA in nulls, Bower(2002). ... The reduction in the cost and size of the electronics in telescopes of the future will allow radio astronomers to take increasing advantage of multibeaming through either focal plane or aperture plane arrays. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/O3-1/ -- 33.8 Кб -- 13.03.2003
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