GRB 160821A is the third most energetic gamma-ray burst observed by the Fermi gamma-ray space telescope. Based on the observations made by the Cadmium Zinc Telluride Imager on board AstroSat, here we report the most conclusive evidence to date of (i) high linear polarization ( detection), and (ii) variation of polarization angle with time, occurring twice during the rise and decay phase of the burst at 3.5σ and 3.1σ detections, respectively. All confidence levels are reported for two parameters of interest. These observations strongly suggest synchrotron radiation produced in magnetic field lines that are highly ordered on angular scales of 1/Γ, where Γ is the Lorentz factor of the outflow
Measuring the polarization of the prompt gamma-ray emission from GRBs can significantly improve our ...
As we further our studies on Gamma-ray bursts (GRBs), both on theoretical models and observational t...
Núria Jordana-Mitjans explains how she uses linear polarization to unveil strong magnetic fields in ...
GRB 160821A is the third most energetic gamma-ray burst observed by the Fermi gamma-ray space telesc...
Aims. With the accumulation of polarization data in the gamma-ray burst (GRB) prompt phase, polariza...
We report on the polarization measure, obtained with IBIS on board INTEGRAL, of the prompt emission ...
Multipulsed GRB 190530A, detected by the Gamma-ray Burst Monitor (GBM) and Large Area Telescope onbo...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
The emission mechanism and the origin and structure of magnetic fields in gamma‐ray burst (GRB) jets...
Long gamma-ray burst GRB 191016A was a bright and slow rising burst that was detected by the Swift s...
Aims. With the accumulation of polarization data in the gamma-ray burst (GRB) prompt phase, polariza...
7 pages, 3 figuresPolarization measurements provide direct insight into the nature of astrophysical ...
We present photometric and polarimetric measurements of gamma-ray burst (GRB) optical afterglows obs...
The recent detection of linear polarization from GRB120206 has piqued the interest of the community ...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
Measuring the polarization of the prompt gamma-ray emission from GRBs can significantly improve our ...
As we further our studies on Gamma-ray bursts (GRBs), both on theoretical models and observational t...
Núria Jordana-Mitjans explains how she uses linear polarization to unveil strong magnetic fields in ...
GRB 160821A is the third most energetic gamma-ray burst observed by the Fermi gamma-ray space telesc...
Aims. With the accumulation of polarization data in the gamma-ray burst (GRB) prompt phase, polariza...
We report on the polarization measure, obtained with IBIS on board INTEGRAL, of the prompt emission ...
Multipulsed GRB 190530A, detected by the Gamma-ray Burst Monitor (GBM) and Large Area Telescope onbo...
Gamma-ray bursts (GRBs) are extremely energetic events of cosmological origin. Observed GRBs have hi...
The emission mechanism and the origin and structure of magnetic fields in gamma‐ray burst (GRB) jets...
Long gamma-ray burst GRB 191016A was a bright and slow rising burst that was detected by the Swift s...
Aims. With the accumulation of polarization data in the gamma-ray burst (GRB) prompt phase, polariza...
7 pages, 3 figuresPolarization measurements provide direct insight into the nature of astrophysical ...
We present photometric and polarimetric measurements of gamma-ray burst (GRB) optical afterglows obs...
The recent detection of linear polarization from GRB120206 has piqued the interest of the community ...
We present a catalog of early-time (~10^2-10^4s) photometry and polarimetry of all Gamma-Ray Burst (...
Measuring the polarization of the prompt gamma-ray emission from GRBs can significantly improve our ...
As we further our studies on Gamma-ray bursts (GRBs), both on theoretical models and observational t...
Núria Jordana-Mitjans explains how she uses linear polarization to unveil strong magnetic fields in ...