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arXiv · 1406.6727

Stellar Variability in the VVV Survey: An Update

M. Catelan·I. Dekany·M. Hempel·D. Minniti
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Abstract

The Vista Variables in the Via Lactea (VVV) ESO Public Survey consists in a near-infrared time-series survey of the Galactic bulge and inner disk, covering 562 square degrees of the sky, over a total timespan of more than 5 years. In this paper, we provide an updated account of the current status of the survey, especially in the context of stellar variability studies. In this sense, we give a first description of our efforts towards the construction of the VVV Variable Star Catalog (VVV-VSC).

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M. Catelan, I. Dekany, M. Hempel, D. Minniti. 2014-06-25. Stellar Variability in the VVV Survey: An Update. https://arxiv.org/abs/1406.6727

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