Were view someop en problems in theph ysics of afterglows, namely their polarization properties and the existence of dark/faint bursts. Polarization studies yield precious insights in the physical structure and dynamical evolution of GRB jets, revealing their magnetization properties and their energy profile. Polarimetric observations of GRB020813 already allowed to exclude a homogeneous jet for this event. We then present observations of faint/dark bursts, showing that some of them may be obscured by dust, while others are possibly just intrinsically dim
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRB...
The emission mechanism and the origin and structure of magnetic fields in gamma‐ray burst (GRB) jets...
We review some open problems in the physics of afterglows, namely their polarization properties and ...
I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRB...
We report polarization measurements and photometry for the optical afterglow of the gamma-ray burst ...
Gamma-Ray Burst afterglow polarization measurements, in spite of their intrinsic difficulties, have ...
We report the optical polarization of a gamma ray burst (GRB) afterglow, obtained 203 seconds after ...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
International audienceFollow-up observations of large numbers of gamma-ray burst (GRB) afterglows, f...
Many aspects of astrophysical jets can be studied by measuring the polarization of the prompt emissi...
The polarization of the optical afterglow (AG) of Gamma-Ray Bursts (GRBs) has only been measured in ...
Follow-up observations of large numbers of gamma-ray burst (GRB) afterglows, facilitated by the Swif...
Follow-up observations of large numbers of gamma-ray burst (GRB) afterglows, facilitated b...
Polarization measurements for the optical counterpart to GRB 020405 are presented and discussed. Our...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRB...
The emission mechanism and the origin and structure of magnetic fields in gamma‐ray burst (GRB) jets...
We review some open problems in the physics of afterglows, namely their polarization properties and ...
I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRB...
We report polarization measurements and photometry for the optical afterglow of the gamma-ray burst ...
Gamma-Ray Burst afterglow polarization measurements, in spite of their intrinsic difficulties, have ...
We report the optical polarization of a gamma ray burst (GRB) afterglow, obtained 203 seconds after ...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
International audienceFollow-up observations of large numbers of gamma-ray burst (GRB) afterglows, f...
Many aspects of astrophysical jets can be studied by measuring the polarization of the prompt emissi...
The polarization of the optical afterglow (AG) of Gamma-Ray Bursts (GRBs) has only been measured in ...
Follow-up observations of large numbers of gamma-ray burst (GRB) afterglows, facilitated by the Swif...
Follow-up observations of large numbers of gamma-ray burst (GRB) afterglows, facilitated b...
Polarization measurements for the optical counterpart to GRB 020405 are presented and discussed. Our...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
I review how polarization signals have been discussed in the research field of Gamma-Ray Bursts (GRB...
The emission mechanism and the origin and structure of magnetic fields in gamma‐ray burst (GRB) jets...