activity
19962026
most citedGWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

1.8k citations · 15.1k across the 280 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2013★ 57 cited

Infrared identification of high-mass X-ray binaries discovered by INTEGRAL

Alexis Coleiro, Sylvain Chaty, Juan A. Zurita Heras +2

Since it started observing the sky, the INTEGRAL satellite has discovered new categories of high mass X-ray binaries (HMXB) in our Galaxy. These observations raise important questi…

astro-ph.HE2013★ 79 cited

Determination of the Point-Spread Function for the Fermi Large Area Telescope from On-orbit Data and Limits on Pair Halos of Active Galactic Nuclei

LAT Collaboration

The Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope is a pair-conversion telescope designed to detect photons with energies from 20 MeV to > 300 GeV. The pre-laun…

astro-ph.HE2013★ 16 cited

NIR and optical observations of the failed outbursts of black hole binary XTE J1550-564

P. A. Curran, S. Chaty

A number of low mass X-ray binaries (LMXBs) undergo "failed outbursts" in which, instead of evolving through the canonical states, they remain in a hard state throughout the outbur…

astro-ph.HE2013★ 837 cited

The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

LAT collaboration

This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half…

astro-ph.HE2013

Herschel views on ultra-luminous X-ray sources

Mathieu Servillat, Alexis Coleiro, Sylvain Chaty

The nature of ultra-luminous X-ray sources (ULXs), which are off-nuclear extragalactic X-ray sources that exceed the Eddington luminosity for a stellar-mass black hole, is still la…

astro-ph.HE2013

An INTEGRAL view of High Mass X-ray Binaries : their nature, formation and evolution

Sylvain Chaty

We describe here the nature, formation and evolution of the supergiant high mass X-ray binary (HMXB) population, i.e. systems accreting the stellar wind of supergiant stars. There…