The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624 (2007)
D'Avanzo, Paolo, Filliatre, Philippe, Goldoni, P., Antonelli, L. Angelo, Campana, Sergio, Chincarini, Guido, ...
Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and hence for the use of...
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...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...
L'expérience embarquée en ballon Archeops a cartographié les anisotropies du Fond Diffus Cosmologique (CMB) avec une résolution angulaire de 10 minutes d'arc sur une portion du ciel de 30%. Elle...