Photometric Variability in the Faint Sky Variability Survey
Astrophysics
2007-05-23 v1
Abstract
The Faint Sky Variability Survey (FSVS) is aimed at finding photometric and/or astrometric variable objects between 16th and 24th mag on time-scales between tens of minutes and years with photometric precisions ranging from 3 millimag to 0.2 mag. An area of 23 deg, located at mid and high Galactic latitudes, was covered using the Wide Field Camera (WFC) on the 2.5-m Isaac Newton Telescope (INT) on La Palma. Here we present some preliminary results on the variability of sources in the FSVS.
Keywords
Cite
@article{arxiv.astro-ph/0410262,
title = {Photometric Variability in the Faint Sky Variability Survey},
author = {L. Morales-Rueda and P. J. Groot and T. Augusteijn and G. Nelemans and P. M. Vreeswijk and E. J. M. van den Besselaar},
journal= {arXiv preprint arXiv:astro-ph/0410262},
year = {2007}
}
Comments
4 pages, 3 figures, to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler