papers

Publications (6)

astro-ph.SR2018

Gaia Data Release 2: Summary of the variability processing & analysis results

B. Holl, M. Audard, K. Nienartowicz +60

The Gaia Data Release 2 (DR2): we summarise the processing and results of the identification of variable source candidates of RR Lyrae stars, Cepheids, long period variables (LPVs)…

astro-ph.SR2016

Gaia Data Release 1 - The Cepheid & RR Lyrae star pipeline and its application to the south ecliptic pole region

G. Clementini, V. Ripepi, S. Leccia +24

We present an overview of the Specific Objects Study (SOS) pipeline developed within the Coordination Unit 7 (CU7) of the Gaia Data Processing and Analysis Consortium (DPAC), the c…

astro-ph.IM2017

Gaia Data Release 1: The variability processing & analysis and its application to the south ecliptic pole region

L. Eyer, N. Mowlavi, D. W. Evans +70

The ESA Gaia mission provides a unique time-domain survey for more than one billion sources brighter than G=20.7 mag. Gaia offers the unprecedented opportunity to study variability…

astro-ph.SR2017

Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

Gaia Collaboration, G. Clementini, L. Eyer +588

Parallaxes for 331 classical Cepheids, 31 Type II Cepheids and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release…

astro-ph.SR2017

Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects

Gaia Collaboration, F. van Leeuwen, A. Vallenari +589

Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a subset of about 2 million stars for which, besides the position and photometry,…

astro-ph.IM2017

Gaia eclipsing binary and multiple systems. Two-Gaussian models applied to OGLE-III eclipsing binary light curves in the Large Magellanic Cloud

N. Mowlavi, I. Lecoeur-Taïbi, B. Holl +11

The advent of large scale multi-epoch surveys raises the need for automated light curve (LC) processing. This is particularly true for eclipsing binaries (EBs), which form one of t…