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Xavier Haubois

Researcher at European Southern Observatory

Publications -  80
Citations -  3037

Xavier Haubois is an academic researcher from European Southern Observatory. The author has contributed to research in topics: Stars & Red supergiant. The author has an hindex of 20, co-authored 80 publications receiving 2178 citations. Previous affiliations of Xavier Haubois include University of São Paulo & Paris Diderot University.

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Journal ArticleDOI

Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

Roberto Abuter, +108 more
TL;DR: Eisenhauer et al. as mentioned in this paper detect the combined gravitational redshift and relativistic transverse Doppler effect for S2 of z = Δλ / λ ≈ 200 km s−1/c with different statistical analysis methods.
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First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer

Roberto Abuter, +138 more
TL;DR: GRAVITY as discussed by the authors is a new instrument to coherently combine the light of the European Southern Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 m diameter angular resolution and a collecting area of 200 m2.
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Detection of orbital motions near the last stable circular orbit of the massive black hole SgrA

TL;DR: In this article, the position centroids exhibit clockwise looped motion on the sky, on scales of typically 150 μ as over a few tens of minutes, corresponding to about 30% the speed of light.
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Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole

TL;DR: In this article, the first detection of the GR Schwarzschild precession (SP) in S2's orbit was reported, which is a kink between the pre-and post-pericentre directions of motion ≈±1 year around pericentre passage.
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Radiative hydrodynamics simulations of red supergiant stars - II. Simulations of convection on Betelgeuse match interferometric observations

TL;DR: In this paper, a 3D radiative-hydrodynamics (RHD) simulation is used to compute intensity maps in different filters and derive interferometric observables using the post-processing radiative transfer code OPTIM3D.