activity
20122018
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 10k across the 10 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

6 papers · 1 filter

astro-ph.IM2018★ 20 cited

Gaia Data Release 2. Short-timescale variability processing and analysis

M. Roelens, L. Eyer, N. Mowlavi +13

The Gaia DR2 sample of short-timescale variable candidates results from the investigation of the first 22 months of Gaia photometry for a subsample of sources at the Gaia faint end…

astro-ph.IM2018★ 211 cited

Gaia Data Release 2: Properties and validation of the radial velocities

D. Katz, P. Sartoretti, M. Cropper +51

For Gaia DR2 (GDR2), 280 million spectra, collected by the RVS instrument on-board Gaia, were processed and median radial velocities were derived for 9.8 million sources brighter t…

astro-ph.IM2018★ 756 cited

Gaia Data Release 2: Photometric content and validation

D. W. Evans, M. Riello, F. De Angeli +9

Aims. We describe the photometric content of the second data release of the Gaia project (Gaia DR2) and its validation along with the quality of the data. Methods. The validation w…

astro-ph.IM2014★ 53 cited

Overview and stellar statistics of the expected Gaia Catalogue using the Gaia Object Generator

X. Luri, M. Palmer, F. Arenou +13

Aims: An effort has been undertaken to simulate the expected Gaia Catalogue, including the effect of observational errors. A statistical analysis of this simulated Gaia data is per…

astro-ph.IM2013★ 6 cited

An approach to the analysis of SDSS spectroscopic outliers based on Self-Organizing Maps

D. Fustes, M. Manteiga, C. Dafonte +5

Aims. A new method is applied to the segmentation, and further analysis of the outliers resulting from the classification of astronomical objects in large databases is discussed. T…

astro-ph.IM2012★ 64 cited

The expected performance of stellar parametrization with Gaia spectrophotometry

C. Liu, C. A. L. Bailer-Jones, R. Sordo +4

Gaia will obtain astrometry and spectrophotometry for essentially all sources in the sky down to a broad band magnitude limit of G=20, an expected yield of 10^9 stars. Its main sci…