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Gaia Data Release 2 Summary of the variability processing and analysis results

Gaia Collaboration: Pawlak, M.

Context. The Gaia Data Release 2 (DR2) contains more than half a million sources that are identified as variable stars.
Aims. We summarise the processing and results of the identification of variable source candidates of RR Lyrae stars, Cepheids, longperiod variables (LPVs), rotation modulation (BY Dra-type) stars, δ Scuti and SX Phoenicis stars, and short-timescale variables. In
this release we aim to provide useful but not necessarily complete samples of candidates.
Methods. The processed Gaia data consist of the G, GBP, and GRP photometry during the first 22 months of operations as well as
positions and parallaxes. Various methods from classical statistics, data mining, and time-series analysis were applied and tailored to
the specific properties of Gaia data, as were various visualisation tools to interpret the data.
Results. The DR2 variability release contains 228 904 RR Lyrae stars, 11 438 Cepheids, 151 761 LPVs, 147 535 stars with rotation
modulation, 8882 δ Scuti and SX Phoenicis stars, and 3018 short-timescale variables. These results are distributed over a classification
and various Specific Object Studies tables in the Gaia archive, along with the three-band time series and associated statistics for the
underlying 550 737 unique sources. We estimate that about half of them are newly identified variables. The variability type completeness varies strongly as a function of sky position as a result of the non-uniform sky coverage and intermediate calibration level of these
data. The probabilistic and automated nature of this work implies certain completeness and contamination rates that are quantified so
that users can anticipate their effects. This means that even well-known variable sources can be missed or misidentified in the published
data.
Conclusions. The DR2 variability release only represents a small subset of the processed data. Future releases will include more
variable sources and data products; however, DR2 shows the (already) very high quality of the data and great promise for variability
studies
type:article
journal:Astronomy & Astrophysics Special Issue
volume:A30
pages:618
year:2018
grants:Teorie a pozorování astronomických tranzientů: supernovy z hmotných hvězd a splynutí hvězd, Primus/17/SCI/17; 2017-2019; hlavní řešitel: Ondřej Pejcha
files:
aa32892-18.pdf (6220.26 kB)

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