The optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801A

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dc.contributor.authorLipunov, V. M.
dc.contributor.authorGorosabel, J.
dc.contributor.authorPruzhinskaya, M. V.
dc.contributor.authorde Ugarte Postigo, A.
dc.contributor.authorPelassa, V.
dc.contributor.authorTsvetkova, A. E.
dc.contributor.authorSokolov, I. V.
dc.contributor.authorKann, D. A.
dc.contributor.authorXu, Dong
dc.contributor.authorGorbovskoy, E. S.
dc.contributor.authorKrushinski, V. V.
dc.contributor.authorKornilov, V. G.
dc.contributor.authorBalanutsa, P. V.
dc.contributor.authorBoronina, S. V.
dc.contributor.authorBudnev, N. M.
dc.contributor.authorCano, Z.
dc.contributor.authorCastro Tirado, A. J.
dc.contributor.authorChazov, V. V.
dc.contributor.authorConnaughton, V.
dc.contributor.authorDelvaux, C.
dc.contributor.authorFrederiks, D. D.
dc.contributor.authorFynbo, J. F. U.
dc.contributor.authorGabovich, A. V.
dc.contributor.authorGoldstein, A.
dc.contributor.authorGreiner, J.
dc.contributor.authorGress, O. A.
dc.contributor.authorIvanov, K. I.
dc.contributor.authorJakobsson, P.
dc.contributor.authorKlose, S.
dc.contributor.authorKnust, F.
dc.contributor.authorKomarova, V. N.
dc.contributor.authorKonstantinov, E.
dc.contributor.authorKrylov, A. V.
dc.contributor.authorKuvshinov, D. A.
dc.contributor.authorKuznetsov, A. S.
dc.contributor.authorLipunova, G. V.
dc.contributor.authorMoskvitin, A. S.
dc.contributor.authorPal'shin, V. D.
dc.contributor.authorPandey, S. B.
dc.contributor.authorPoleshchuk, V. A.
dc.contributor.authorSchmidl, S.
dc.contributor.authorSergienko, Yu. P.
dc.contributor.authorSinyakov, E. V.
dc.contributor.authorSchulze, S.
dc.contributor.authorSokolov, V. V.
dc.contributor.authorSokolova, T. N.
dc.contributor.authorSparre, M.
dc.contributor.authorThoene, C. C.
dc.contributor.authorTlatov, A. G.
dc.contributor.authorTyurina, N. V.
dc.contributor.authorUlanov, M. V.
dc.contributor.authorYazev, S. A.
dc.contributor.authorYurkov, V. V.
dc.date.accessioned2024-01-10T13:43:53Z
dc.date.available2024-01-10T13:43:53Z
dc.date.issued2016
dc.description.abstractWe report the early discovery of the optical afterglow of gamma-ray burst (GRB) 140801A in the 137 deg(2) 3-sigma error-box of the Fermi Gamma-ray Burst Monitor (GBM). MASTER is the only observatory that automatically reacts to all Fermi alerts. GRB 140801A is one of the few GRBs whose optical counterpart was discovered solely from its GBM localization. The optical afterglow of GRB 140801A was found by MASTER Global Robotic Net 53 s after receiving the alert, making it the fastest optical detection of a GRB from a GBM error-box. Spectroscopy obtained with the 10.4-m Gran Telescopio Canarias and the 6-m Big Telescope Alt-azimuth of the Special Astrophysical Observatory of the Russian Academy of Sciences reveals a redshift of z = 1.32. We performed optical and near-infrared photometry of GRB 140801A using different telescopes with apertures ranging from 0.4 to 10.4 m. GRB 140801A is a typical burst in many ways. The rest-frame bolometric isotropic energy release and peak energy of the burst are E-iso = 5.54(-0.24)(+0.26) x 10(52) erg and E-p,E- rest similar or equal to 280 keV, respectively, which is consistent with the Amati relation. The absence of a jet break in the optical light curve provides a lower limit on the half-opening angle of the jet theta = 6 degrees.1. The observed E-peak is consistent with the limit derived from the Ghirlanda relation. The joint Fermi GBM and Konus-Wind analysis show that GRB 140801A could belong to the class of intermediate duration. The rapid detection of the optical counterpart of GRB 140801A is especially important regarding the upcoming experiments with large coordinate error-box areas.
dc.description.funderDevelopment Programme of Lomonosov Moscow State University
dc.description.funderRFBR
dc.description.funderRussian Federation Ministry of Education and Science
dc.description.funderNASA
dc.description.funderRussian Foundation of Fundamental Research
dc.description.funderRussian Space Agency, RFBR
dc.description.funderDFG
dc.description.funderSpanish Ministry Grant
dc.description.funderEXTraS from European Union
dc.description.funderThuringer Ministerium fur Bildung, Wissenschaft und Kultur
dc.description.funderDivision of Physics, Russian Academy of Sciences
dc.description.funderRussian Federation
dc.description.funderCONICYT-Chile FONDECYT
dc.description.funderBasal-CATA
dc.description.funder'Millennium Institute of Astrophysics (MAS) of Iniciativa Cientifica Milenio del Ministerio de Economia, Fomento y Turismo'
dc.fechaingreso.objetodigital2024-04-29
dc.format.extent13 páginas
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stv2228
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stv2228
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/78780
dc.identifier.wosidWOS:000368005900082
dc.information.autorucFísica; Schulze S;S/I;237742
dc.issue.numero1
dc.language.isoen
dc.nota.accesocontenido parcial
dc.pagina.final724
dc.pagina.inicio712
dc.publisherOXFORD UNIV PRESS
dc.revistaMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.rightsacceso restringido
dc.subjectacceleration of particles
dc.subjectblack hole physics
dc.subjectmagnetic field
dc.subjectgamma-ray: general
dc.subjectX-ray: general
dc.subjectGAMMA-RAY BURSTS
dc.subjectCOMPLETE SAMPLE
dc.subjectLIGHT CURVES
dc.subjectAFTERGLOW
dc.subjectSPECTRA
dc.subjectMASTER
dc.subjectLUMINOSITY
dc.subjectCATALOG
dc.subjectNETWORK
dc.subjectENERGY
dc.subject.ods07 Affordable and Clean Energy
dc.subject.odspa07 Energía asequible y no contaminante
dc.titleThe optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801A
dc.typeartículo
dc.volumen455
sipa.codpersvinculados237742
sipa.indexWOS
sipa.indexScopus
sipa.trazabilidadCarga SIPA;09-01-2024
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