Gaia Data Release 2

α 2 Canum Venaticorum, α Cygni, β Cephei, cataclysmic, classical Cepheids, δ Scuti, γ Cassiopeiae, γ Doradus, Mira, ellipsoidal, RR Lyrae of Bailey’s type ab and c,

A comparison between periods derived by the SOS pipeline and periods published in the literature for a sample of 37 941 RR Lyrae stars in common between Gaia and the OGLE catalogues

In particular, 550 737 variable stars are published (as summarised in Holl et al. 2018 ), among which 363 969 objects are identified by the all-sky classification pipeline (see

The Gaia-RVS standards: a new full-sky list of 1420 stars with reliable Radial

Left panel: Current status of the number of observations available per candidate standard star observed with the SOPHIE, CORALIE and NARVAL instruments (995 distinct stars).. Black

We compared the results on the Rb abundance derived from the 794 nm line from MyGIsFOS and the fitting procedure of the observed line profile: the abundances we derive are very

férents motifs géométriques, de même que le lissage des couvertures en laine et, en poils de chameaux à rayures et motifs berbères très variés. I.a teint tire des laines,

3Deportment of Soil Science of Temperate Ecosystems, lJniversity of Gottingen, Gdttingen, Germony 4Chair of Soil Physics, lJniversity of Bayreuth, Bayreuth,