| Issue |
EAS Publications Series
Volume 61, 2013
Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe
|
|
|---|---|---|
| Page(s) | 267 - 269 | |
| Section | Chapter V: Afterglow Emission-I Long GRBs (Observations) | |
| DOI | https://doi.org/10.1051/eas/1361042 | |
| Published online | 22 July 2013 | |
A.J. Castro-Tirado, J.Gorosabel and I.H. Park (eds)
EAS Publications Series, 61 (2013) 267-269
GRB 110715A: Multiwavelength study of the first gamma-ray burst observed with ALMA
1
Instituto de Astrofísica de Andalucía, IAA-CSIC,
Glorieta de la Astronomía s/n,
18008,
Spain
2
Sydney Institute for Astronomy, School of Physics, The University
of Sydney, NSW
2006, Australia
3
Dark Cosmology Centre, Niels Bohr Institute,
Juliane Maries Vej 30,
2100
Copenhagen Ø,
Danemark
4
Unidad Asociada Grupo Ciencia Planetarias UPV/EHU-IAA/CSIC,
Departamento de Física Aplicada I, E.T.S. Ingeniería, Universidad del País Vasco
UPV/EHU, Alameda de Urquijo
s/n, 48013
Bilbao,
Spain
5
Ikerbasque, Basque Foundation for Science,
Alameda de Urquijo 36-5,
48008
Bilbao,
Spain
6
Thüringer Landessternwarte Tautenburg,
Sternwarte 5, 07778
Tautenburg,
Germany
7
MPI für extraterrestrische Physik, 85740
Garching,
Germany
8
European Southern Observatory, Vitacura Casilla 19001, Santiago de Chile 19,
Chile
9
Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura, Santiago, Chile
10
Harvard-Smithsonian Center for Astrophysics,
60 Garden St., Cambridge, MA
02138,
USA
11
Mullard Space Science Laboratory, University College
London, Holmbury St. Mary,
Dorking, Surrey
RH5 6NT,
UK
Abstract
GRB 110715A had a bright afterglow that was obscured in the optical by a high Galactic extinction. We discovered the submillimeter counterpart with APEX and followed it in radio with ATCA for over 2 months. Additional submm observations were performed with ALMA as a test of the ToO procedures during commissioning, becoming the first GRB afterglow to be detected by the observatory. UV, optical and NIR observations were performed with Swift/UVOT and 2.2 m/GROND in La Silla and X-ray data were obtained by Swift/XRT. The dataset is complemented with spectroscopic data from the VLT/X-shooter spectrograph. The absorption features present in the intermediate resolution optical/nIR spectra reveal a redshift of 0.8224 and a host galaxy environment with low ionization. We fit in the host galaxy absorption features two velocity components separated by 30 km/s, implying a host galaxy with low dynamical activity.
© EAS, EDP Sciences 2013
