https://doi.org/10.1051/epjconf/201715203015
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
* bsabogal@uniandes.edu.co
** josegarc@uniandes.edu.co
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
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
