RS Puppis
RS Puppis as imaged with the ESO NTT (from Kervella et al. 2008)
RS Puppis as imaged with the ESO NTT (from Kervella et al. 2008)
The American Association of Variable Star Observers
Nova Search Section
Search Area Location Chart
Search area location charts will help you organize your nova search observing program. Each area is numbered and represents an area of the Milky Way whose dimensions are approximately 10 degrees of declination by one hour of right ascension. Use these charts to document areas of the heavens you are searching.
The following article is a reprint from the Journal of the AAVSO, Vol. 7, No. 2. We acknowledge and thank the editor of the Journal of the AAVSO for graciously allowing us to reprint this article for the benefit of our observers and readers.
Peter L. Collins
Mt. Hopkins Observatory
Tucson, AZ 85721
Abstract
The following article is a reprint from the Journal of the AAVSO, Vol. 10, No. 1, 25, 1981. We acknowledge and thank the editor of the Journal of the AAVSO for graciously allowing us to reprint this article for the benefit of our observers and readers. Kenneth C. Beckmann
201 West Springfield
Union, Missouri 63084
Abstract
1994
Editor:Reverend K.C. Beckmann
Lewiston, Michigan
Volume 1, Number 1
Excerpts From AAVSO Newsletter Number 10, January 1993.
For more information on novae searching, please contact Committee Chairperson Kenneth C. Beckmann, kennethbeckmann@yahoo.com.
A number of papers have been written discussing visual magnitude estimates in comparison to photometry. Multiple studies have shown that visual magnitude estimates compare very favorably with instrumental photometry in terms of sensitivity and consistency. As with all data, care must be taken to understand what visual magnitude estimates represent, what their bandpass is, and when their use is appropriate.
Contributed by Tom Fleming (FLET)
Reports and observations submitted to the AAVSO use the following ratings for atmospheric turbulence (Seeing): Poor, Fair, Good and Excellent.