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dc.contributor.authorSanchez-Ramirez, R.
dc.contributor.authorHancock, Paul
dc.contributor.authorMurphy, T.
dc.contributor.authorde Ugarte Postigo, A.
dc.contributor.authorGorosabel, J.
dc.contributor.authorKann, D.
dc.contributor.authorThöne, C.
dc.contributor.authorLundgren, A.
dc.contributor.authorKamble, A.
dc.contributor.authorOates, S.
dc.contributor.authorFynbo, J.
dc.contributor.authorde Gregorio Monsalvo, I.
dc.contributor.authorGarcia-Appadoo, D.
dc.contributor.authorMartin, S.
dc.contributor.authorKuin, N.
dc.contributor.authorGreiner, J.
dc.contributor.authorCastro-Tirado, A.
dc.contributor.editorA.J. Castro-Tirado
dc.contributor.editorJ. Gorosabel
dc.contributor.editorI.H. Park
dc.date.accessioned2017-01-30T11:44:46Z
dc.date.available2017-01-30T11:44:46Z
dc.date.created2015-03-03T03:51:00Z
dc.date.issued2013
dc.identifier.citationSanchez-Ramirez, R. and Hancock, P. and Murphy, T. and de Ugarte Postigo, A. and Gorosabel, J. and Kann, D. and Thöne, C. et al. 2013. GRB 110715A: Multiwavelength study of the first gamma-ray burst observed with ALMA, in Castro-Tirado , A.J. and Gorosabel, J. and Park, I.H. (ed), 2012 Gamma-Ray Burst Symposium, Oct 8-12 2012, pp. 267-269. Malaga, Spain: European Astronomical Society.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/14602
dc.identifier.doi10.1051/eas/1361042
dc.description.abstract

GRB 110715A had a bright afterglow that was obscured inthe optical by a high Galactic extinction. We discovered the submillimetercounterpart with APEX and followed it in radio with ATCAfor over 2 months. Additional submm observations were performedwith 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/UVOTand 2.2 m/GROND in La Silla and X-ray data were obtained bySwift/XRT. The dataset is complemented with spectroscopic data fromthe VLT/X-shooter spectrograph. The absorption features presentin the intermediate resolution optical/nIR spectra reveal a redshiftof 0.8224 and a host galaxy environment with low ionization. We fit inthe host galaxy absorption features two velocity components separatedby 30 km/s, implying a host galaxy with low dynamical activity.

dc.publisherEuropean Astronomical Society
dc.titleGRB 110715A: Multiwavelength study of the first gamma-ray burst observed with ALMA
dc.typeConference Paper
dcterms.source.startPage267
dcterms.source.endPage269
dcterms.source.issn1633-4760
dcterms.source.titleGamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe
dcterms.source.seriesGamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe
dcterms.source.conference2012 Gamma-Ray Burst Symposium
dcterms.source.conference-start-dateOct 8 2012
dcterms.source.conferencelocationMalaga; Spain
dcterms.source.placeFrance
curtin.accessStatusFulltext not available


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