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23 April 2024 |
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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
; | | Date: |
11 Oct 2004 | | Subject: | astro-ph | | Affiliation: | 3, 1), P. M. Vreeswijk , and E.J.M. van den Besselaar ( University of Nijmegen, Nordic Optical Telescope, Institute of Astronomy Cambridge, University of Amsterdam | | 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. | | Source: | arXiv, astro-ph/0410262 | | Services: | Forum | Review | PDF | Favorites | |
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