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Jerome Rodriguez

Researcher at Paris Diderot University

Publications -  147
Citations -  4324

Jerome Rodriguez is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Luminosity & X-ray binary. The author has an hindex of 36, co-authored 145 publications receiving 3966 citations. Previous affiliations of Jerome Rodriguez include University of Paris & Commissariat à l'énergie atomique et aux énergies alternatives.

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Journal ArticleDOI

Polarized Gamma-Ray Emission from the Galactic Black Hole Cygnus X-1

TL;DR: This gamma-ray emission originates from a jet of relativistic particles that is formed in close proximity to the black hole, and is measured with the International Gamma-Ray Astrophysics Laboratory Imager on Board the Integral Satellite (INTEGRAL/IBIS) telescope.
Journal ArticleDOI

Radiatively efficient accreting black holes in the hard state: the case study of H1743-322

TL;DR: In this article, the radio and X-ray emission of H1743−322 were investigated and it was shown that the inner accretion flow is radiatively efficient during the hard state, in contrast to what is usually assumed for black hole Xray binaries in this spectral state.
Proceedings ArticleDOI

XIPE: the x-ray imaging polarimetry explorer

P. Soffitta, +421 more
- 01 Jan 2016 - 
TL;DR: The X-ray Imaging Polarimetry Explorer (XIPE) as discussed by the authors is a mission dedicated to Xray Astronomy which is in a competitive phase A as fourth medium size mission of ESA (M4).
Journal ArticleDOI

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. ⋆ I. The nature of the companion star

TL;DR: In this paper, mid-infrared (MIR) observations of the companion stars of SGXBs from these two classes were used to assess the contribution of the star and the material enshrouding the system to the total emission.
Journal ArticleDOI

Regulation of black-hole accretion by a disk wind during a violent outburst of V404 Cygni

TL;DR: Observations of a sustained outer accretion disk wind in V404 Cyg, which is unlike any seen hitherto, find that the outflowing wind is neutral, has a large covering factor, expands at one per cent of the speed of light and triggers a nebular phase once accretion drops sharply and the ejecta become optically thin.