Photometric Variability in the Faint Sky Variability Survey

Details Photometric Variability in the Faint Sky Variability Survey Photometric Variability in the Faint Sky Variability Survey

2004-10-11

arxiv.org/abs/astro-ph/0410262v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler

Scientific paper

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$^2$, 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.

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