International audience
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April 24, 2017 (v1)Conference paperUploaded on: December 4, 2022
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2021 (v1)Journal article
The current tension between the direct and the early-universe measurements of the Hubble constant, H 0, requires detailed scrutiny of all the data and methods used in the studies on both sides of the debate. The Cepheids in the Type Ia supernova (SN Ia) host galaxy NGC 5584 played a key role in the local measurement of H 0. The SH0ES project...
Uploaded on: December 4, 2022 -
January 8, 2020 (v1)Publication
Classical Cepheids (CCs) are at the heart of the empirical extragalactic distance ladder. Milky Way CCs are the only stars of this class accessible to trigonometric parallax measurements. Until recently, the most accurate trigonometric parallaxes of Milky Way CCs were the HST/FGS measurements collected by Benedict et al. (2002, 2007)....
Uploaded on: December 4, 2022 -
2022 (v1)Journal article
Context. Achernar, the closest and brightest classical Be star, presents rotational flattening, gravity darkening, occasional emission lines due to a gaseous disk, and an extended polar wind. It is also a member of a close binary system with an early A-type dwarf companion. Aims: We aim to determine the orbital parameters of the Achernar...
Uploaded on: December 3, 2022 -
August 2019 (v1)Journal article
International audience
Uploaded on: December 4, 2022