A new type of high-energy binary system has been revealed by the INTEGRAL satellite. These sources are being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among...
A new type of high-energy binary system has been revealed by the INTEGRAL satellite. These sources are being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among...
A new type of high-energy binary system has been revealed by the INTEGRAL satellite. These sources are being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
Chaty, Sylvain, Rahoui, Farid, Foellmi, Cédric, Tomsick, John, Rodriguez, Jérôme, Walter, Roland
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations. Previous studies have shown that many...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
Chaty, Sylvain, Rahoui, Farid, Foellmi, Cédric, Tomsick, John, Rodriguez, Jérôme, Walter, Roland
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations. Previous studies have shown that many...
Chaty, Sylvain, Rahoui, Farid, Foellmi, Cédric, Tomsick, John, Rodriguez, Jérôme, Walter, Roland
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations. Previous studies have shown that many...
Chaty, Sylvain, Rahoui, Farid, Foellmi, Cédric, Tomsick, John, Rodriguez, Jérôme, Walter, Roland
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations. Previous studies have shown that many...
Des microquasars aux systèmes binaires enfouis: enquête dans l'Univers des astres extrêmes... (2008)
Introduction: Dans ce chapitre d'introduction je décris les caractéristiques générales, la formation et l'évolution des différentes familles de systèmes binaires de haute énergie, ainsi que...
Des microquasars aux systèmes binaires enfouis: enquête dans l'Univers des astres extrêmes... (2008)
Introduction: Dans ce chapitre d'introduction je décris les caractéristiques générales, la formation et l'évolution des différentes familles de systèmes binaires de haute énergie, ainsi que...
Des microquasars aux systèmes binaires enfouis: enquête dans l'Univers des astres extrêmes... (2008)
Introduction: Dans ce chapitre d'introduction je décris les caractéristiques générales, la formation et l'évolution des différentes familles de systèmes binaires de haute énergie, ainsi que...
Des microquasars aux systèmes binaires enfouis: enquête dans l'Univers des astres extrêmes... (2008)
Introduction: Dans ce chapitre d'introduction je décris les caractéristiques générales, la formation et l'évolution des différentes familles de systèmes binaires de haute énergie, ainsi que...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
(abridged) Context: The INTEGRAL mission has led to the discovery of a new type of Supergiant X-ray Binaries (SGXBs) whose physical properties differ from those of previously known SGXBs. Two classes...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in...
Chaty, Sylvain, Rahoui, Farid, Foellmi, Cédric, Tomsick, John A., Rodriguez, Jérôme, Walter, Roland
Context: The INTEGRAL hard X-ray observatory has revealed an emerging population of highly obscured X-ray binary systems through multi-wavelength observations. Previous studies have shown that many...
Rahoui, Farid, Chaty, Sylvain, Lagage, Pierre-Olivier, Pantin, Eric
(abridged) Context: The INTEGRAL mission has led to the discovery of a new type of Supergiant X-ray Binaries (SGXBs) whose physical properties differ from those of previously known SGXBs. Two classes...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared...
CGRaBS: An All-Sky Survey of Gamma-Ray Blazar Candidates (2007)
Healey, Stephen E., Romani, Roger W., Cotter, Garret, Michelson, Peter F., Schlafly, Edward F., Readhead, Anthony C. S., ...
We describe a uniform all-sky survey of bright blazars, selected primarily by their flat radio spectra, that is designed to provide a large catalog of likely gamma-ray AGN. The defined sample has...
To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the onset of...
To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the onset of...
To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the onset of...
Broad-band spectral changes of the microquasars Cygnus X-1 and SWIFT J1753.5-0127 (2006)
Cadolle Bel, Marion, Ribo, Marc, Rodriguez, Jerome, Chaty, Sylvain, Corbel, Stephane, Goldwurm, Andrea
We report high-energy results obtained with INTEGRAL and Rossi-XTE on two microquasars: the persistent high-mass system Cygnus X-1 and the transient low-mass binary SWIFT J1753.5-0127. INTEGRAL...
Broad-band spectral changes of the microquasars Cygnus X-1 and SWIFT J1753.5-0127 (2006)
Bel, Marion Cadolle, Ribo, Marc, Rodriguez, Jerome, Chaty, Sylvain, Corbel, Stephane, Goldwurm, Andrea
We report high-energy results obtained with INTEGRAL and Rossi-XTE on two microquasars: the persistent high-mass system Cygnus X-1 and the transient low-mass binary SWIFT J1753.5-0127. INTEGRAL...
Broad-band spectral changes of the microquasars Cygnus X-1 and SWIFT J1753.5-0127 (2006)
Cadolle Bel, Marion, Ribo, Marc, Rodriguez, Jerome, Chaty, Sylvain, Corbel, Stephane, Goldwurm, Andrea
We report high-energy results obtained with INTEGRAL and Rossi-XTE on two microquasars: the persistent high-mass system Cygnus X-1 and the transient low-mass binary SWIFT J1753.5-0127. INTEGRAL...
A new type of sources has been discovered by INTEGRAL. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among the...
A new type of sources has been discovered by INTEGRAL. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among the...
A new type of sources has been discovered by INTEGRAL. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among the...
A new type of sources has been discovered by INTEGRAL. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among the...
A new type of sources has been discovered by INTEGRAL. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among the...
The role of microquasars in astroparticle physics (2006)
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena...
The role of microquasars in astroparticle physics (2006)
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena...
The role of microquasars in astroparticle physics (2006)
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Chaty, Sylvain, Bessolaz, Nicolas
Aims: To gain a better understanding of high-energy Galactic sources, we observed the Galactic X-ray binary and black hole candidate XTE J1720-318 in the optical and near-infrared, just after the...
Identifications of Four INTEGRAL Sources in the Galactic Plane via Chandra Localizations (2006)
Tomsick, John A., Chaty, Sylvain, Rodriguez, Jerome, Foschini, Luigi, Walter, Roland, Kaaret, Philip
Hard X-ray imaging of the Galactic plane by the INTEGRAL satellite is uncovering large numbers of 20-100 keV "IGR" sources. We present results from Chandra, INTEGRAL, optical, and IR observations of...
The role of microquasars in astroparticle physics (2006)
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena...
The role of microquasars in astroparticle physics (2006)
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena...
Chaty, Sylvain, Mignani, Roberto, Israel, Gianluca
We had reported in Chaty, Mignani, Israel (2002) on the near-infrared (NIR) identification of a possible counterpart to the black hole candidate XTE J1908+094 obtained with the ESO/NTT. Here, we...
Chaty, Sylvain, Mignani, Roberto, Israel, Gianluca
We had reported in Chaty, Mignani, Israel (2002) on the near-infrared (NIR) identification of a possible counterpart to the black hole candidate XTE J1908+094 obtained with the ESO/NTT. Here, we...
Chaty, Sylvain, Mignani, Roberto, Israel, Gianluca
We had reported in Chaty, Mignani, Israel (2002) on the near-infrared (NIR) identification of a possible counterpart to the black hole candidate XTE J1908+094 obtained with the ESO/NTT. Here, we...
Chaty, Sylvain, Mignani, Roberto P., Israel, Gianluca
We had reported in Chaty, Mignani, Israel (2002) on the near-infrared (NIR) identification of a possible counterpart to the black hole candidate XTE J1908+094 obtained with the ESO/NTT. Here, we...
Chaty, Sylvain, Mignani, Roberto, Israel, Gianluca
We had reported in Chaty, Mignani, Israel (2002) on the near-infrared (NIR) identification of a possible counterpart to the black hole candidate XTE J1908+094 obtained with the ESO/NTT. Here, we...
Negueruela, Ignacio, Smith, David M., Reig, Pablo, Chaty, Sylvain, Torrejon, Jose Miguel
INTEGRAL monitoring of the Galactic Plane is revealing a growing number of recurrent X-ray transients, characterised by short outbursts with very fast rise times (~ tens of minutes) and typical...
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena....
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena....
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena....
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena....
I present an overview of past, present and future research on microquasars and jets, showing that microquasars, i.e. galactic jet sources, are among the best laboratories for high energy phenomena....
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO...
Revealing the nature of the highly obscured galactic source IGR J16318-4848 (2004)
Chaty, Sylvain, Filliatre, Philippe
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. We carried out optical and near-infrared (NIR) observations at the European Southern Observatory (ESO...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
VLT search for the infrared counterpart of 1E 1740.7-2942 (2000)
Marti, Josep, Mirabel, I. Felix, Chaty, Sylvain, Rodriguez, Luis F.
We report the results of our search for the near infrared counterpart of the microquasar 1E 1740.7-2942 using the VLT (Based on observations collected at the European Southern Observatory, Chile (ESO...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Cette thèse est consacrée à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...
Microquasars et objets compacts observés en infrarouge (1994)
Ce rapport de DEA est consacré à l'étude des microquasars, des sources binaires de haute énergie appartenant à notre Galaxie, analogues morphologiquement aux quasars, mais sur des échelles de...