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1. D.J. Asher, Research Fellow
Next: M.E. Bailey, Director Up: Technical Research Summaries Previous: Technical Research Summaries . David Asher continued to work part time at Armagh Observatory and part time at the Bisei Spaceguard Center in Japan. ... With the most spectacular Leonid meteor displays of recent years now over, the Leonid meteor shower still continued to hold people's interest, with a modestly enhanced display visible in 2003 from parts of the world. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2003/node32.html -- 5.6 Кб -- 18.05.2004
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2. astro-ph
... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=Jr -- 12.6 Кб -- 06.02.2013
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3. PAUL J. GREEN - Contributing ConcepTests
I'm glad you're interested in collaborating on the ConcepTests for Astronomy WWW database project! ... I'm looking forward to your contributions! ... a) high luminosity, high temperature to low luminosity, low temperature . b) high luminosity, low temperature to low luminosity, low temperature . c) high luminosity, low temperature to low luminosity, high temperature . d) high luminosity, high temperature to low luminosity high temperature. ... Back to Paul Green's Peer Instruction page. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/educ/Contrib_oct01.html -- 8.4 Кб -- 01.10.2012
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4. ADASS 2002 Conference Proceedings
... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/P4-2/ -- 25.4 Кб -- 12.03.2003
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