Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 418-418, 2016
DOI: 10.1017/s1743921317003337
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Photometric variability of the Be star population with the KELT survey
Journal article published in 2016 by
Jonathan Labadie-Bartz 
,
Joshua Pepper,
S. Drew Chojnowski,
M. Virginia McSwain
,
Joshua Pepper,
S. Drew Chojnowski,
M. Virginia McSwain
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractWe are using light curves from the KELT exoplanet transit survey (Pepper et al. 2007) to study the variability of hundreds of Be stars. Combining these light curves with simultaneous time-series spectra from the APOGEE survey (Majewski et al. 2015) provides a glimpse into how changes in the circumstellar environment are correlated to brightness variations.
