Studying the SN-GRB connection with X-shooter: The GRB 100316D / SN 2010bh case
arXiv:1103.5298 · doi:10.1002/asna.201111531
Abstract
During the last ten years, observations of long-duration gamma-ray bursts brought to the conclusion that at least a fraction of them is associated with bright supernovae of type Ib/c. In this talk, after a short review on the previously observed GRB-SN connection cases, we present the recent case of GRB 100316/SN 2010bh. In particular, during the observational campaign of SN 2010bh, a pivotal role was played by VLT/X-shooter, sampling with unique high quality data the spectral energy distribution of the early evolution phases from the UV to the K band.
4 pages, 2 figure. Proceedings of the workshop "The first year with X-shooter" October 19-22 2010, Como, Italy. References added
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Cited by in corpus (10)
- A Comprehensive Study of Gamma-Ray Burst Optical Emission: I. Flares and Early Shallow Decay Component
- XRF 100316D / SN 2010bh and the Nature of Gamma Ray Burst Supernovae
- Spectroscopic evidence for SN 2010ma associated with GRB 101219B
- The Fast Evolution of SN 2010bh associated with XRF 100316D
- Metallicity in the GRB 100316D/SN 2010bh Host Complex
- The Needle in the 100 deg2 Haystack: Uncovering Afterglows of Fermi GRBs with the Palomar Transient Factory
- Multicolour modelling of SN 2013dx associated with GRB 130702A
- Near-extremal black holes as initial conditions of long GRB-supernovae and probes of their gravitational wave emission
- Prospects for multi-messenger extended emission from core-collapse supernovae in the Local Universe
- Electromagnetic priors for black hole spindown in searches for gravitational-waves from supernovae and long GRBs