GRB050904 at redshift 6.3:: observations of the oldest cosmic explosion after the Big Bang

被引:115
作者
Tagliaferri, G
Antonelli, LA
Chincarini, G
Fernández-Soto, A
Malesani, D
Della Valle, M
D'Avanzo, P
Grazian, A
Testa, V
Campana, S
Covino, S
Fiore, F
Stella, L
Castro-Tirado, AJ
Gorosabel, J
Burrows, DN
Capalbi, M
Cusumano, G
Conciatore, ML
D'Elia, V
Filliatre, P
Fugazza, D
Gehrels, N
Guetta, D
Guziy, S
Held, EV
Hurley, K
Israel, GL
Jelínek, M
Lazzati, D
López-Echarri, A
Melandri, A
Mirabel, IF
Moles, M
Moretti, A
Mason, KO
Nousek, J
Osborne, J
Pellizza, LJ
Perna, R
Piranomonte, S
Piro, L
Postigo, AD
Romano, P
机构
[1] INAF, Osservatorio Astron Brera, I-23807 Merate, Lc, Italy
[2] INAF, Osservatorio Astron Roma, I-00040 Rome, Italy
[3] Univ Milano Bicocca, Dipartimento Fis, I-20126 Milan, Italy
[4] Univ Valencia, Astron Observ, Valencia 46071, Spain
[5] ISAS, SISSA, I-34014 Trieste, Italy
[6] INAF, Osservatorio Astrofis Arcetri, I-50125 Florence, Italy
[7] Univ Insubria, Dipartimento Matemat & Fis, I-22100 Como, Italy
[8] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[9] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[10] ASI Sci Data Ctr, I-00044 Frascati, Roma, Italy
[11] INAF, IASF, Sez Palermo, I-90146 Palermo, Italy
[12] Lab Astroparticule & Cosmol, UMR 7164, F-75231 Paris, France
[13] CEA Saclay, DAPNIA, DSM, Serv Astrophys, F-91911 Gif Sur Yvette, France
[14] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[15] INAF, Osservatorio Astron Padova, I-35122 Padua, Italy
[16] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[17] Univ Colorado, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
[18] Inst Astrofis Canarias, Tenerife 38200, Spain
[19] Univ Cagliari, Dipartimento Fis, I-09042 Monserrato, Ca, Italy
[20] European So Observ Vitacura, Santiago 19, Chile
[21] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[22] Univ Leicester, Dept Phys & Astron, Xray & Observat Astron Grp, Leicester LE1 7RH, Leics, England
[23] Univ Paris 07, CEA Saclay, Serv Astrophys, AIM,CNRS,UMR 7158, F-91191 Gif Sur Yvette, France
[24] INAF, IASF, Sez Roma, I-00133 Rome, Italy
来源
ASTRONOMY & ASTROPHYSICS | 2005年 / 443卷 / 01期
关键词
cosmology : observations; early Universe; gamma rays : bursts; gamma rays : individual : GRB 050904;
D O I
10.1051/0004-6361:200500196
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4 x 10(53) erg in the rest- frame 110 110- 1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at - t(b) = 2.6 +/- 1.0 d ( observer frame). If we assume this is the jet break, we derive a beaming-corrected energy E-gamma similar to (4 divided by 12) x 10(51) erg. This limit shows that GRB050904 is consistent with the Amati and Ghirlanda relations. This detection is consistent with the expected number of GRBs at z > 6 and shows that GRBs are a powerful tool to study the star formation history up to very high redshift.
引用
收藏
页码:L1 / L5
页数:5
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