Photometric Variability in the Faint Sky Variability Survey

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dc.creatorMorales-Rueda, L.
dc.creatorGroot, P. J.
dc.creatorAugusteijn, T.
dc.creatorNelemans, G.
dc.creatorVreeswijk, P. M.
dc.creatorBesselaar, E. J. M. van den
dc.date2004-10-11
dc.date.accessioned2026-07-07T02:14:58Z
dc.date.available2026-07-07T02:14:58Z
dc.descriptionThe 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.
dc.description4 pages, 3 figures, to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler
dc.identifierhttps://arxiv.org/abs/astro-ph/0410262
dc.identifierhttp://arxiv.org/abs/astro-ph/0410262
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8345
dc.subjectAstrophysics
dc.titlePhotometric Variability in the Faint Sky Variability Survey
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