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...
We present the spectral analysis of 14 gamma-ray bursts (GRB) X-ray afterglows in order to investiga...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed ...
In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed...
We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for whi...
Context. Long gamma-ray bursts (GRBs) are produced during the dramatic deaths of massive stars with ...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
We present the first results of a program to systematically study the optical-to-X-ray spectral ener...
Gamma-ray Bursts (GRBs) are the most powerful transients in the Universe, over– shining for a few s...
Context. The reionisation of the Universe is a process that is thought to have ended around z ~ 6, a...
International audienceAims. We present a study of the environment of the Swift long gamma-ray burst ...
Context. Long gamma-ray bursts (GRBs) give us the chance to study both their extreme physics and the...
Context: New information on short/hard gamma-ray bursts (GRBs) is being gathered thanks to the disc...
We present the spectral analysis of 14 gamma-ray bursts (GRB) X-ray afterglows in order to investiga...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed ...
In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed...
We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts (GRBs) for whi...
Context. Long gamma-ray bursts (GRBs) are produced during the dramatic deaths of massive stars with ...
The Swift satellite allows us to use gamma-ray bursts (GRBs) to peer through the hearts of star form...
We present the first results of a program to systematically study the optical-to-X-ray spectral ener...
Gamma-ray Bursts (GRBs) are the most powerful transients in the Universe, over– shining for a few s...
Context. The reionisation of the Universe is a process that is thought to have ended around z ~ 6, a...
International audienceAims. We present a study of the environment of the Swift long gamma-ray burst ...
Context. Long gamma-ray bursts (GRBs) give us the chance to study both their extreme physics and the...
Context: New information on short/hard gamma-ray bursts (GRBs) is being gathered thanks to the disc...
We present the spectral analysis of 14 gamma-ray bursts (GRB) X-ray afterglows in order to investiga...
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. T...
Gamma-ray bursts (GRBs), which are bright flashes of gamma rays from extragalactic sources followed ...