2014MNRAS.442.2586V

Query : 2014MNRAS.442.2586V

2014MNRAS.442.2586V - Mon. Not. R. Astron. Soc., 442, 2586-2599 (2014/August-2)

GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z ∼ 2.8.

VOLNOVA A.A., POZANENKO A.S., GOROSABEL J., PERLEY D.A., FREDERIKS D.D., KANN D.A., RUMYANTSEV V.V., BIRYUKOV V.V., BURKHONOV O., CASTRO-TIRADO A.J., FERRERO P., GOLENETSKII S.V., KLOSE S., LOZNIKOV V.M., MINAEV P.Yu., STECKLUM B., SVINKIN D.S., TSVETKOVA A.E., DE UGARTE POSTIGO A. and ULANOV M.V.

Abstract (from CDS):

We present observations of the dark gamma-ray burst GRB 051008 provided by Swift/BAT, Swift/XRT, Konus-WIND, INTEGRAL/SPI-ACS in the high-energy domain and the Shajn, Swift/UVOT, Tautenburg, NOT, Gemini and Keck I telescopes in the optical and near-infrared bands. The burst was detected only in gamma- and X-rays and neither a prompt optical nor a radio afterglow was detected down to deep limits. We identified the host galaxy of the burst, which is a typical Lyman-break galaxy (LBG) with R-magnitude of 24.06±0.10 mag. A redshift of the galaxy of z = 2.77_-0.20^+0.15 is measured photometrically due to the presence of a clear, strong Lyman-break feature. The host galaxy is a small starburst galaxy with moderate intrinsic extinction (AV = 0.3) and has a star formation rate of ∼ 60M☉/yr typical for LBGs. It is one of the few cases where a GRB host has been found to be a classical LBG. Using the redshift we estimate the isotropic-equivalent radiated energy of the burst to be Eiso = (1.15±0.20)x1054 erg. We also provide evidence in favour of the hypothesis that the darkness of GRB 051008 is due to local absorption resulting from a dense circumburst medium.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): gamma-ray burst: individual: dark - galaxies: distances and redshifts - galaxies: high-redshift - galaxies: photometry

Nomenclature: Table 7, Fig. 6: [VPG2014] IdN (Nos 1-5).

CDS comments: Galaxies Id1, 2, 4 and 5 are not in Simbad (no coordinates).

Simbad objects: 51

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Number of rows : 51
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 Fermi bn081221681 gB 01 03 10.2 -24 32 53           ~ 186 0
3 GRB 060719 gB 01 13 43.380 -48 22 55.09           ~ 107 0
4 GRB 000210 gB 01 59 15 -40 40.0           ~ 175 0
5 GRB 060202 gB 02 23 22.940 +38 23 03.70           ~ 102 0
6 GRB 070802 gB 02 27 35.91 -55 31 39.1           ~ 168 0
7 GRB 060306 gB 02 44 22.830 -02 08 55.00           ~ 119 0
8 Fermi bn090926914 gB 03 05 14.30 -38 59 50.9           ~ 149 1
9 GRB 060210 gB 03 50 57.370 +27 01 34.40   20.27       ~ 275 0
10 GRB 080913 gB 04 22 57.90 -25 07 38.6           ~ 213 0
11 GRB 090407 gB 04 35 54.98 -12 40 45.5           ~ 87 0
12 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
13 GRB 050915A gB 05 26 44.804 -28 00 59.27           ~ 88 0
14 GRB 980828 gB 09 37 +22.7           ~ 16 1
15 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 222 1
16 GRB 100219A gB 10 16 48.48 -12 34 00.0           ~ 130 0
17 GRB 110709B gB 10 58 37.2 -23 27 18           ~ 92 0
18 GRB 030115 gB 11 18 32.6 +15 02 59           ~ 90 1
19 GRB 060319 gB 11 45 33.050 +60 00 39.61 20.10         ~ 73 0
20 GRB 990506 gB 11 54 41 -26 45.0           ~ 169 1
21 GRB 080607A gB 12 59 47.14 +15 55 09.6           ~ 257 0
22 HD 117710 PM* 13 31 15.7663471680 +42 06 22.152472848   7.158 6.065     K2III 52 0
23 GRB 051008 gB 13 31 28.100 +42 08 05.01 17.06   14.11     ~ 90 0
24 [VPG2014] Id3 G 13 31 29.510 +42 05 53.67 25.32 25.20 24.45 24.07 23.88 ~ 1 0
25 2MASS J13313142+4206470 * 13 31 31.4282862048 +42 06 47.390997204           ~ 1 0
26 SDSS J133133.59+420401.4 * 13 31 33.5847653976 +42 04 01.397678052           ~ 1 0
27 SDSS J133137.89+420705.5 * 13 31 37.8956114760 +42 07 05.461042044           ~ 1 0
28 SDSS J133138.56+420443.6 * 13 31 38.5718782536 +42 04 43.596604740           ~ 1 0
29 SDSS J133141.93+420803.1 * 13 31 41.9325040680 +42 08 03.087117744           ~ 1 0
30 SDSS J133145.91+420730.4 * 13 31 45.9095163504 +42 07 30.418009032           ~ 1 0
31 SDSS J133146.39+420825.9 * 13 31 46.3914144288 +42 08 25.935080208           ~ 1 0
32 SDSS J133153.53+420304.7 * 13 31 53.5439501640 +42 03 04.692674664           ~ 1 0
33 GRB 080207 gB 13 50 03.02 +07 30 08.0           ~ 114 0
34 GRB 090417B gB 13 58 44.8 +47 00 55           ~ 119 1
35 GRB 060814 gB 14 45 21.480 +20 35 11.80           ~ 241 0
36 GRB 090404 gB 15 56 55.80 +35 31 03.4           ~ 79 0
37 GRB 070521 gB 16 10 38.600 +30 15 22.70           ~ 164 0
38 GRB 060923A gB 16 58 28.150 +12 21 38.90           ~ 70 0
39 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
40 GRB 970828 gB 18 08 31.6 +59 18 51           ~ 353 1
41 GRB 080325 gB 18 31 34.40 +36 31 26.1           ~ 76 0
42 GRB 090709A gB 19 19 46.70 +60 43 40.8           ~ 125 0
43 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
44 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
45 EGGR 150 WD* 21 52 25.3789636654 +02 23 19.576176425 11.942 12.732 12.743 12.839 12.938 DA2.8 213 0
46 Fermi bn081109293 gB 22 03 11.50 -54 42 40.5           ~ 125 1
47 GRB 071021 gB 22 42 34.33 +23 43 05.4           ~ 104 0
48 GRB 020819 gB 23 00 12 -43 00.7           ~ 135 1
49 GRB 111215A gB 23 18 13.33 +32 29 38.5           ~ 68 0
50 GRB 061222A gB 23 53 03.419 +46 31 58.60           ~ 177 0
51 GRB 051022A gB 23 56 04.200 +19 36 32.30           ~ 194 1

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