In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31/03/2017. In total, we have obtained spectroscopic observations of 103 individual GRBs observed within 48 hours of the GRB trigger. Redshifts have been measured for 97 per cent of these, covering a redshift range from 0.059 to 7.84. Based on a set of observational selection criteria that minimise biases with regards to intrinsic properties of the GRBs, the follow-up effort has been focused on producing a homogeneously selected sample of 93 afterglow spectra for GRBs discovered by the Swift satellite. We here provide a public release of all the reduced spectra, including continuum estimates and telluric...
International audienceGRB 100418A was an intermediate duration GRB detected by Swift. It showed an i...
We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ra...
International audienceContext. The reionisation of the Universe is a process that is thought to have...
In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
We present simultaneous optical and near-infrared (NIR) spectroscopy of 19 Swift γ-ray burst (GRB) h...
Gamma-ray burst (GRB) progenitors are observationally linked to the death of massive stars. X-ray st...
We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for whi...
Aims. We present a study of the environment of the Swift long gamma-ray burst GRB 120327A at z ≈ 2.8...
Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Lar...
International audienceGRB 100418A was an intermediate duration GRB detected by Swift. It showed an i...
We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ra...
International audienceContext. The reionisation of the Universe is a process that is thought to have...
In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
We present simultaneous optical and near-infrared (NIR) spectroscopy of 19 Swift γ-ray burst (GRB) h...
Gamma-ray burst (GRB) progenitors are observationally linked to the death of massive stars. X-ray st...
We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for whi...
Aims. We present a study of the environment of the Swift long gamma-ray burst GRB 120327A at z ≈ 2.8...
Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Lar...
International audienceGRB 100418A was an intermediate duration GRB detected by Swift. It showed an i...
We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ra...
International audienceContext. The reionisation of the Universe is a process that is thought to have...