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20052018
most citedGaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

101 citations · 675 across the 16 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2018★ 88 cited

Gaia Data Release 2: The first Gaia catalogue of long-period variable candidates

N. Mowlavi, I. Lecoeur-Taïbi, T. Lebzelter +13

Gaia DR2 provides a unique all-sky catalogue of 550'737 variable stars, of which 151'761 are long-period variable (LPV) candidates with G variability amplitudes larger than 0.2 mag…

astro-ph.SR2018★ 71 cited

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.SR2017★ 101 cited

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★ 17 cited

A comprehensive study of young B stars in NGC 2264: I. Space photometry and asteroseismology

K. Zwintz, E. Moravveji, P. I. Papics +9

Space photometric time series of the most massive members of the young open cluster NGC 2264 allow us to study their different sources of variability down to the millimagnitude lev…

astro-ph.SR2015★ 10 cited

The 2003-4 multisite photometric campaign for the Beta Cephei and eclipsing star 16 (EN) Lacertae with an Appendix on 2 Andromedae, the variable comparison star

M. Jerzykiewicz, G. Handler, J. Daszynska-Daszkiewicz +26

A multisite photometric campaign for the Beta Cephei and eclipsing variable 16 Lacertae is reported. 749 h of high-quality differential photoelectric Stromgren, Johnson and Geneva…

astro-ph.SR2014★ 65 cited

Echography of young stars reveals their evolution

K. Zwintz, L. Fossati, T. Ryabchikova +17

We demonstrate that a seismic analysis of stars in their earliest evolutionary phases is a powerful method to identify young stars and distinguish their evolutionary states. The ea…