Color and Variability Characteristics of Point Sources in the Faint Sky Variability Survey

dc.creatorHuber, M. E.
dc.creatorEverett, M. E.
dc.creatorHowell, S. B.
dc.date2006-04-20
dc.date.accessioned2026-07-07T11:25:31Z
dc.date.available2026-07-07T11:25:31Z
dc.descriptionWe present an analysis of the color and variability characteristics for point sources in the Faint Sky Variability Survey (FSVS). The FSVS cataloged ~23 square degrees in BVI filters from ~16--24 mag to investigate variability in faint sources at moderate to high Galactic latitudes. Point source completeness is found to be >83% for a selected representative sample (V=17.5--22.0 mag, B-V=0.0--1.5) containing both photometric B, V detections and 80% of the time-sampled V data available compared to a basic internal source completeness of 99%. Multi-epoch (10--30) observations in V spanning minutes to years modeled by light curve simulations reveal amplitude sensitivities to 0.015--0.075 mag over a representative V=18--22 mag range. Periodicity determinations appear viable to time-scales of an order 1 day or less using the most sampled fields (~30 epochs). The fraction of point sources is found to be generally variable at 5--8% over V=17.5--22.0 mag. For V brighter than 19 mag, the variable population is dominated by low amplitude (<0.05 mag) and blue (B-V<0.35) sources, possibly representing a population of gamma Doradus stars. Overall, the dominant population of variable sources are bluer than B-V=0.65 and have Main Sequence colors, likely reflecting larger populations of RR Lyrae, SX Phe, gamma Doradus, and W UMa variables.
dc.description34 pages, 16 figures, accepted in AJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0604449
dc.identifierhttp://arxiv.org/abs/astro-ph/0604449
dc.identifierAstron.J.132:633-649,2006
dc.identifierdoi:10.1086/505300
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195532
dc.subjectAstrophysics
dc.titleColor and Variability Characteristics of Point Sources in the Faint Sky Variability Survey
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