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Flux upper limit on gamma-ray emission by GRB 050713a from MAGIC telescope observations

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dc.contributor.authorAntoranz Canales, Pedro
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorLópez Moya, Marcos
dc.contributor.authorMiranda Pantoja, José Miguel
dc.date.accessioned2023-06-20T10:39:47Z
dc.date.available2023-06-20T10:39:47Z
dc.date.issued2006-04-10
dc.description© The American Astronomical Society. The construction of the MAGIC Telescope was mainly made possible by the support of the German Bundesministerium für Bildung und Forschung and Max-Planck-Gesellschaft, the Italian Istituto Nazionale de Fisica Nucleare, and the Spanish Comisión Interministerial de Ciencias y Tecnología, to whom goes our grateful acknowledgement. We are grateful for all the hard work done by the GCN team, especially Scott Barthelmy, and to all the people of the Swift Science Center, who kindly provided us with data and the tools to analyze them. In particular, we are indebted to Professor Guido Chincarini, Abe Falcone, and Professor David Burrows from the Swift collaboration. We are also grateful to Nicola Omodei for fruitful discussions on the physics of GRBs. We would also like to thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. This work was further supported by ETH Research Grant TH 34/04 3 and grant 1P03D01028 from the Polish Ministerstwo Nauki i Informatyzacji.
dc.description.abstractThe long-duration gamma-ray burst GRB 050713a was observed by the MAGIC Telescope 40 s after the burst onset and followed up for 37 minutes, until twilight. The observation, triggered by a Swift alert, covered energies above approximate to 175 GeV. Using standard MAGIC analysis, no evidence of a gamma-ray signal was found. As the redshift of the GRB was not measured directly, the flux upper limit estimated by MAGIC is still compatible with the assumption of an unbroken power-law spectrum extending from a few hundred keV to our energy range.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipGerman Bundesministerium für Bildung und Forschung
dc.description.sponsorshipMax-Planck-Gesellschaft
dc.description.sponsorshipItalian Istituto Nazionale de Fisica Nucleare
dc.description.sponsorshipSpanish Comisión Interministerial de Ciencias y Tecnología
dc.description.sponsorshipETH
dc.description.sponsorshipPolish Ministerstwo Nauki i Informatyzacji
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/24241
dc.identifier.doi10.1086/503767
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1086/503767
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/astro-ph/0602231
dc.identifier.urihttps://hdl.handle.net/20.500.14352/50934
dc.issue.number1 (Par
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.finalL12
dc.page.initialL9
dc.publisherIOP Publishing
dc.relation.projectIDTH 34/04 3
dc.relation.projectID1P03D01028
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordEnergy Cosmic-Rays
dc.subject.keywordVery-High-Energy
dc.subject.keywordBursts
dc.subject.keywordBatse
dc.subject.keywordGRS-941017
dc.subject.keywordAbsorption
dc.subject.keywordComponent
dc.subject.keywordSpectra
dc.subject.keywordModel.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleFlux upper limit on gamma-ray emission by GRB 050713a from MAGIC telescope observations
dc.typejournal article
dc.volume.number641
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