Photometric Variability in the Faint Sky Variability Survey

L. Morales-Rueda; P. J. Groot; T. Augusteijn; G. Nelemans; P. M. Vreeswijk; E. J. M. van den Besselaar

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Photometric Variability in the Faint Sky Variability Survey

L. Morales-Rueda·P. J. Groot·T. Augusteijn·G. Nelemans·P. M. Vreeswijk·E. J. M. van den Besselaar

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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$^2$, 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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L. Morales-Rueda, P. J. Groot, T. Augusteijn, G. Nelemans, P. M. Vreeswijk, E. J. M. van den Besselaar. 2004-10-11. Photometric Variability in the Faint Sky Variability Survey. https://arxiv.org/abs/astro-ph/0410262

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