2012ApJ...761...50T


Query : 2012ApJ...761...50T

2012ApJ...761...50T - Astrophys. J., 761, 50 (2012/December-2)

Broadband study of GRB 091127: a sub-energetic burst at higher redshift?

TROJA E., SAKAMOTO T., GUIDORZI C., NORRIS J.P., PANAITESCU A., KOBAYASHI S., OMODEI N., BROWN J.C., BURROWS D.N., EVANS P.A., GEHRELS N., MARSHALL F.E., MAWSON N., MELANDRI A., MUNDELL C.G., OATES S.R., PAL'SHIN V., PREECE R.D., RACUSIN J.L., STEELE I.A., TANVIR N.R., VASILEIOU V., WILSON-HODGE C. and YAMAOKA K.

Abstract (from CDS):

GRB 091127 is a bright gamma-ray burst (GRB) detected by Swift at a redshift z = 0.49 and associated with SN 2009nz. We present the broadband analysis of the GRB prompt and afterglow emission and study its high-energy properties in the context of the GRB/SN association. While the high luminosity of the prompt emission and standard afterglow behavior are typical of cosmological long GRBs, its low-energy release (Eγ< 3x1049 erg), soft spectrum, and unusual spectral lag connect this GRB to the class of sub-energetic bursts. We discuss the suppression of high-energy emission in this burst, and investigate whether this behavior could be connected with the sub-energetic nature of the explosion.

Abstract Copyright: ∼

Journal keyword(s): gamma-ray burst: individual: GRB 091127

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
3 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
4 GRB 080913 gB 04 22 57.90 -25 07 38.6           ~ 213 0
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
6 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
7 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 392 0
8 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
9 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2

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