activity
20152022
most citedThe Seven Sisters DANCe. I. Empirical isochrones, Luminosity and Mass Functions of the Pleiades cluster

82 citations · 105 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph.EP202223 cited

The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets. Project goals, target selection and stellar characterization

J. Lillo-Box, N. C. Santos, A. Santerne +33

The detection of habitable worlds is one of humanity's greatest endeavors. So far, astrobiological studies show that one of the most critical components for life development is liq…

astro-ph.SR2021

Fornacis cluster DANCe. Census of stars, structure, and kinematics of the cluster with Gaia-EDR3

P. A. B. Galli, H. Bouy, J. Olivares +4

Context: The Fornacis cluster (Alessi 13) is one of a few open clusters of its age and distance in the Solar neighbourhood that ought to benefit from more attention as it c…

astro-ph.IM2021

Miec: A Bayesian hierarchical model for the analysis of nearby young open clusters

J. Olivares, H. Bouy, L. M. Sarro +4

Context. The analysis of luminosity and mass distributions of young stellar clusters is essential to understanding the star-formation process. However, the gas and dust left over b…

astro-ph.IM2020

Kalkayotl: A cluster distance inference code

J. Olivares, L. M. Sarro, H. Bouy +5

Context: Stellar clusters are benchmarks for theories of star formation and evolution. The high precision parallax data of the Gaia mission allows significant improvements in the d…

astro-ph.GA2018

Gaia Data Release 2. Summary of the contents and survey properties

Gaia Collaboration, A. G. A. Brown, A. Vallenari +4

We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources…

astro-ph.IM2018

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…