Searching for Be star candidates within large databases
Universidad de los Andes, Departamento de Física, Cra.1 No.18A-10, Ed. Ip, A.A.4976, Bogotá, Colombia
Published online: 8 September 2017
Long time surveys yield many light curves among their byproducts, useful to identify candidate Be stars that can be confirmed by spectroscopic follow-ups. We present in this work different techniques we have used to find Be star candidates in the Galaxy, the Magellanic Clouds and the OGLE-IV Gaia South Ecliptic Pole Field.
© The Authors, published by EDP Sciences, 2017
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