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Sökning: onr:"swepub:oai:DiVA.org:su-70079" > GRB 091127/SN 2009n...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004431naa a2200805 4500
001oai:DiVA.org:su-70079
003SwePub
008120117s2011 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-700792 URI
024a https://doi.org/10.1051/0004-6361/2011177262 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Vergani, S. D.4 aut
2451 0a GRB 091127/SN 2009nz and the VLT/X-shooter spectroscopy of its host galaxy :b probing the faint end of the mass-metallicity relation
264 c 2011-11-30
264 1b EDP Sciences,c 2011
338 a print2 rdacarrier
520 a We perform a detailed study of the gamma-ray burst GRB 091127/SN 2009nz host galaxy at z = 0.490 using the VLT/X-shooter spectrograph in slit and integral-field unit (IFU) mode. From the analysis of the optical and X-ray afterglow data obtained from ground-based telescopes and Swift-XRT, we confirm the presence of a bump associated with SN 2009nz and find evidence of a possible jet break in the afterglow lightcurve. The X-shooter afterglow spectra reveal several emission lines from the underlying host, from which we derive its integrated properties. These properties agree with those of previously studied GRB-SN hosts and, more generally, with those of the long GRB host population. We use the Hubble Space Telescope and ground-based images of the host to determine its stellar mass (M⋆). Our results extend to lower M⋆ values the M-Z plot derived for the sample of long GRB hosts at 0.3 < z < 1.0 adding new information to probe the faint end of the M-Z relation and the shift of the LGRB host M-Z relation from that found from emission-line galaxy surveys. Thanks to the IFU spectroscopy, we can build the two-dimensional (2D) velocity, velocity dispersion, and star formation rate (SFR) maps. They show that the host galaxy has perturbed rotation kinematics with evidence of a SFR enhancement consistent with the afterglow position. Based on observations made with ESO Telescopes at Paranal Observatory under programmes ID 084.A-0260 and 086.A-0874.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a gamma-ray burst: individual: GRB 091127
653 a supernovae: individual: SN 2009nz
653 a galaxies: ISM
653 a galaxies: evolution
700a Flores, H.4 aut
700a Covino, S.4 aut
700a Fugazza, D.4 aut
700a Gorosabel, J.4 aut
700a Levan, A. J.4 aut
700a Puech, M.4 aut
700a Salvaterra, R.4 aut
700a Tello, J. C.4 aut
700a de Ugarte Postigo, A.4 aut
700a D'Avanzo, P.4 aut
700a D'Elia, V.4 aut
700a Fernández, M.4 aut
700a Fynbo, J. P. U.4 aut
700a Ghirlanda, G.4 aut
700a Jelínek, M.4 aut
700a Lundgren, A.4 aut
700a Malesani, D.4 aut
700a Palazzi, E.4 aut
700a Piranomonte, S.4 aut
700a Rodrigues, M.4 aut
700a Sánchez-Ramírez, R.4 aut
700a Terrón, V.4 aut
700a Thöne, C. C.4 aut
700a Antonelli, L. A.4 aut
700a Campana, S.4 aut
700a Castro-Tirado, A. J.4 aut
700a Goldoni, P.4 aut
700a Hammer, F.4 aut
700a Hjorth, J.4 aut
700a Jakobsson, P.4 aut
700a Kaper, L.4 aut
700a Melandri, A.4 aut
700a Milvang-Jensen, B.4 aut
700a Sollerman, Jesperu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)solle
700a Tagliaferri, G.4 aut
700a Tanvir, N. R.4 aut
700a Wiersema, K.4 aut
700a Wijers, R. A. M. J.4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 535, s. A127-q 535<A127-x 0004-6361x 1432-0746
856u https://www.aanda.org/articles/aa/pdf/2011/11/aa17726-11.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-70079
8564 8u https://doi.org/10.1051/0004-6361/201117726

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