Gaia DR2 documentation Chapter 7: Variability
- Autor(en)
- L. Eyer, L. Guy, E. Distefano, G. Clementini, N. Mowlavi, L. Rimoldini, M. Roelens, M. Audard, B. Holl, A. Lanzafame, T. Lebzelter, I. Lecoeur-Taïbi, L. Molnár, V. Ripepi, L. Sarro, G. Jevardat de Fombelle, K. Nienartowicz, J. De Ridder, Á. Juhász, R. Molinaro, E. Plachy, S. Regibo
- Abstrakt
This chapter of the Gaia DR2 documentation describes the models and methods used on the 22 months of data to produce the Gaia variable star results for Gaia DR2. The variability processing and analysis was based mostly on the calibrated G and integrated BP and RP photometry. The variability analysis approach to the Gaia data has been described in Eyer et al. (2017), and the Gaia DR2 results are presented in Holl et al. (2018). Detailed methods on specific topics will be published in a number of separate articles. Variability behaviour in the colour magnitude diagram is presented in Gaia Collaboration et al. (2018c).
- Organisation(en)
- Institut für Astrophysik
- Publikationsdatum
- 07-2018
- ÖFOS 2012
- 103004 Astrophysik, 103003 Astronomie
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/27de0f5a-5eab-42d9-ae0a-922ed85d05da