2019A&A...623A..92S

Query : 2019A&A...623A..92S

2019A&A...623A..92S - Astronomy and Astrophysics, volume 623A, 92-92 (2019/3-1)

The X-shooter GRB afterglow legacy sample (XS-GRB).

SELSING J., MALESANI D., GOLDONI P., FYNBO J.P.U., KRUHLER T., ANTONELLI L.A., ARABSALMANI M., BOLMER J., CANO Z., CHRISTENSEN L., COVINO S., D'AVANZO P., D'ELIA V., DE CIA A., DE UGARTE POSTIGO A., FLORES H., FRIIS M., GOMBOC A., GREINER J., GROOT P., HAMMER F., HARTOOG O.E., HEINTZ K.E., HJORTH J., JAKOBSSON P., JAPELJ J., KANN D.A., KAPER L., LEDOUX C., LELOUDAS G., LEVAN A.J., MAIORANO E., MELANDRI A., MILVANG-JENSEN B., PALAZZI E., PALMERIO J.T., PERLEY D.A., PIAN E., PIRANOMONTE S., PUGLIESE G., SANCHEZ-RAMIREZ R., SAVAGLIO S., SCHADY P., SCHULZE S., SOLLERMAN J., SPARRE M., TAGLIAFERRI G., TANVIR N.R., THONE C.C., VERGANI S.D., VREESWIJK P., WATSON D., WIERSEMA K., WIJERS R., XU D. and ZAFAR T.

Abstract (from CDS):

In this work we present spectra of all γ-ray burst (GRB) afterglows that have been promptly observed with the X-shooter spectrograph until 31/03/2017.In total, we have obtained spectroscopic observations of 103 individual GRBs observed within 48 hours of the GRB trigger. Redshifts have been measured for 97 per cent of these, covering a redshift range from 0.059 to 7.84. Based on a set of observational selection criteria that minimise biases with regards to intrinsic properties of the GRBs, the follow-up effort has been focused on producing a homogeneously selected sample of 93 afterglow spectra for GRBs discovered by the Swift satellite. We here provide a public release of all the reduced spectra, including continuum estimates and telluric absorption corrections. For completeness, we also provide reductions for the 18 late-time observations of the underlying host galaxies. We provide an assessment of the degree of completeness with respect to the parent GRB population, in terms of the X-ray properties of the bursts in the sample and find that the sample presented here is representative of the full Swift sample. We have constrained the fraction of dark bursts to be <28 per cent and confirm previous results that higher optical darkness is correlated with increased X-ray absorption. For the 42 bursts for which it is possible, we have provided a measurement of the neutral hydrogen column density, increasing the total number of published HI column density measurements by ∼33 per cent. This dataset provides a unique resource to study theISM across cosmic time, from the local progenitor surroundings to the intervening Universe.

Abstract Copyright: © ESO 2019

Journal keyword(s): gamma-ray burst: general - galaxies: high-redshift - ISM: general - techniques: spectroscopic - catalogs - galaxies: star formation

Simbad objects: 126

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Number of rows : 126
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 GRB 150910A gB 00 22 40.14 +33 28 22.4           ~ 62 0
2 GRB 150206A gB 00 40 17.57 -63 10 56.0           ~ 38 0
3 Fermi bn131231198 gB 00 42 44.0 -01 29 40           ~ 88 0
4 SN 2010ma SN* 00 48 55.35 -34 33 59.5           SNIc 157 1
5 Fermi bn111117510 gB 00 50 46.220 +23 00 39.22           ~ 120 0
6 GRB 121201A gB 00 53 52.21 -42 56 34.5           ~ 40 0
7 SN 2011kl SN* 00 57 22.64 -46 48 03.6           SNSLSN 230 1
8 GRB 100625A gB 01 03 10.98 -39 05 18.3           ~ 106 0
9 Fermi bn100814160 gB 01 29 53.61 -17 59 43.6           ~ 192 0
10 GRB 100901A gB 01 49 03.56 +22 45 30.6           ~ 153 0
11 GRB 091018 gB 02 08 46 -57 33.0           ~ 143 0
12 GRB 131011A gB 02 10 06.11 -04 24 42.5           ~ 36 0
13 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 273 1
14 GRB 151029A gB 02 34 06.71 -35 23 07.8           ~ 31 0
15 GRB 120224A gB 02 43 46.17 -17 45 40.6           ~ 34 0
16 Fermi bn130925164 gB 02 44 42.38 -26 09 15.8           ~ 153 0
17 Fermi bn100728439 gB 02 56 13.44 +00 16 51.6           ~ 121 0
18 GRB 110808A gB 03 49 04.28 -44 11 40.3           ~ 56 0
19 GRB 111008A gB 04 01 48.220 -32 42 34.09           ~ 103 0
20 Fermi bn170113420 gB 04 06 59 -71 56.0           ~ 44 0
21 GRB 121027A gB 04 14 23.450 -58 49 47.17           ~ 113 0
22 GRB 140301A gB 04 38 13.81 -34 15 24.3           ~ 40 0
23 GRB 121024A gB 04 41 53.31 -12 17 26.1           ~ 120 0
24 Fermi bn131105087 gB 04 43 53.50 -63 00 17.7           ~ 74 0
25 Fermi bn161001045 gB 04 47 40.84 -57 15 39.9           ~ 27 0
26 GRB 101219A gB 04 58 20.45 -02 32 23.1           ~ 129 0
27 Fermi bn150514774 gB 04 59 30.45 -60 58 07.0           ~ 40 0
28 GRB 151027B gB 05 04 52.67 -06 27 00.7           ~ 49 0
29 GRB 151031A gB 05 32 47.02 -39 07 18.7           ~ 19 0
30 GRB 120211A gB 05 51 00.89 -24 46 30.8           ~ 36 0
31 Fermi bn150301818 gB 05 56 40.04 -57 58 10.4           ~ 47 0
32 SN 2016jca SN* 06 06 51.36 -26 47 29.7           SNIc 107 0
33 GRB 140430A gB 06 51 44.58 +23 01 25.5           ~ 62 0
34 GRB 161007A gB 06 53 38.17 +23 18 24.2           ~ 18 0
35 GRB 140213A gB 07 00 37.18 -73 08 14.1           ~ 78 0
36 GRB 160228A gB 07 09 15.90 +26 55 54.3           ~ 22 0
37 SN 2010bh SN* 07 10 30.63 -56 15 19.7           SNIc 287 1
38 GRB 160314A gB 07 31 09.80 +16 59 57.5           ~ 32 0
39 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 159 0
40 Fermi bn120118709 gB 08 19 29.05 -07 11 05.1           ~ 74 0
41 GRB 141031A gB 08 34 25.96 -59 10 05.8           ~ 30 0
42 Fermi bn111107035 gB 08 37 54.66 -66 31 12.3           ~ 82 0
43 GRB 160117B gB 08 48 46.71 -16 22 00.9           ~ 34 0
44 GRB 130408A gB 08 57 37.30 -32 21 38.9           ~ 82 0
45 SN 2012bz SN* 09 07 38.38 +14 01 07.5           SNIb/c 163 1
46 GRB 100205A gB 09 25 33.00 +31 44 25.8           ~ 35 0
47 GRB 141109A gB 09 38 07.40 -00 36 28.6           ~ 56 0
48 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 357 0
49 GRB 130418A gB 09 56 08.86 +13 40 01.8           ~ 63 0
50 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 165 0
51 GRB 160410A gB 10 02 44.37 +03 28 42.7           ~ 56 0
52 GRB 170202A gB 10 10 06 +05 01.0           ~ 64 0
53 GRB 111211A gB 10 12 21.700 +11 12 30.00           ~ 33 0
54 GRB 100219A gB 10 16 48.48 -12 34 00.0           ~ 112 0
55 GRB 111123A gB 10 19 23.17 -20 38 41.9           ~ 68 0
56 GRB 160203A gB 10 47 48.32 -24 47 20.4           ~ 40 0
57 GRB 100316B gB 10 54 00 -45 28.0           ~ 53 0
58 GRB 110709B gB 10 58 37.2 -23 27 18           ~ 83 0
59 GRB 160303A gB 11 14 48.16 +22 44 31.3           ~ 38 0
60 Fermi bn120712571 gB 11 18 21.16 -20 02 01.1           ~ 69 0
61 GRB 130603B gB 11 28 48.16 +17 04 18.2           ~ 346 0
62 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 513 1
63 GRB 130131B gB 11 35 49.60 +15 01 59.3           ~ 46 0
64 Fermi bn100615083 gB 11 48 49.25 -19 28 52.2           ~ 112 0
65 GRB 090530 gB 11 57 36.00 +26 35 23.0           ~ 77 0
66 GRB 110407A gB 12 24 07.47 +15 42 42.1           ~ 38 0
67 GRB 140515A gB 12 24 15.48 +15 06 17.7           ~ 73 0
68 GRB 140114A gB 12 34 05.10 +27 57 02.6           ~ 49 0
69 GRB 150428A gB 12 34 09.22 +06 57 13.2           ~ 19 0
70 GRB 121229A gB 12 40 23.41 -50 35 37.2           ~ 51 0
71 Fermi bn110128073 gB 12 55 35.10 +28 03 54.1           ~ 71 0
72 GRB 100724A gB 12 58 10.38 -11 06 09.3           ~ 161 0
73 GRB 080607A gB 12 59 47.14 +15 55 09.6           ~ 235 0
74 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2000 0
75 GRB 090313 gB 13 13 36.00 +08 05 10.7           ~ 137 0
76 GRB 150727A gB 13 35 52.52 -18 19 32.7           ~ 43 0
77 QSO J1342+0928 QSO 13 42 08.100 +09 28 38.36           ~ 115 0
78 GRB 140311A gB 13 57 13.29 +00 38 31.7           ~ 69 0
79 GRB 100424A gB 13 57 47.46 +01 32 20.3           ~ 62 0
80 NAME EGSY8p7 G 14 20 08.50 +52 53 26.6           ~ 33 0
81 GRB 120805A gB 14 26 09.13 +05 49 30.4           ~ 31 0
82 GRB 150423A gB 14 46 18.96 +12 17 00.6           ~ 65 0
83 Fermi bn160804065 gB 14 46 31.20 +09 59 56.1           ~ 56 0
84 GRB 111005A gB 14 53 15.60 -19 43 19.1           ~ 64 0
85 GRB 120722A gB 15 21 58.0 +13 15 01           ~ 41 0
86 GRB 140614A gB 15 24 40.69 -79 07 43.8           ~ 33 0
87 GRB 150518A gB 15 36 48.22 +16 19 47.3           ~ 28 0
88 GRB 120404A gB 15 40 02.29 +12 53 06.3           ~ 84 0
89 GRB 110715A gB 15 50 44.090 -46 14 06.53           ~ 100 0
90 GRB 120327A gB 16 27 27.49 -29 24 53.8           ~ 95 0
91 GRB 130606A gB 16 37 35.12 +29 47 46.4           ~ 154 0
92 GRB 100418A gB 17 05 26.96 +11 27 41.9           ~ 180 0
93 Fermi bn130612141 gB 17 19 10.63 +16 43 11.8           ~ 75 0
94 GRB 120311A gB 18 12 22.160 +14 17 46.30           ~ 29 0
95 GRB 120815A gB 18 15 54.40 -52 07 29.0           ~ 85 0
96 GRB 130615A gB 18 19 19.12 -68 09 40.0           ~ 27 0
97 GRB 120909A gB 18 22 56.81 -59 26 54.9           ~ 82 0
98 Fermi bn140506880 gB 18 27 06.04 -55 38 08.7           ~ 84 0
99 GRB 160425A gB 18 41 18.56 -54 21 36.1           ~ 31 0
100 GRB 100425A gB 19 56 47.16 -26 25 50.5           ~ 75 0
101 GRB 120923A gB 20 15 10.73 +06 13 16.9           ~ 50 0
102 GRB 111129A gB 20 29 44.140 -52 42 46.48           ~ 25 0
103 GRB 160625B gB 20 34 23.67 +06 55 11.1           ~ 171 0
104 GRB 161023A gB 20 44 05.20 -47 39 48.7           ~ 40 0
105 GRB 150403A gB 20 46 01.17 -62 42 40.1           ~ 85 0
106 Fermi bn120716712 gB 20 52 12.17 +09 35 53.9           ~ 63 0
107 GRB 150616A gB 20 58 52.04 -53 23 37.1           ~ 15 0
108 GRB 130427B gB 20 59 36.00 -22 32 51.6           ~ 49 0
109 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 184 0
110 GRB 140622A gB 21 08 41.56 -14 25 09.5           ~ 48 0
111 Fermi bn110818860 gB 21 09 20.890 -63 58 51.80           ~ 75 0
112 GRB 150915A gB 21 18 37.88 -34 54 48.2           ~ 23 0
113 GRB 161117A gB 21 28 12.59 -29 36 49.9           ~ 49 0
114 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 92 0
115 GRB 090809 gB 21 54 43.2 -00 05 02           ~ 78 0
116 GRB 131117A gB 22 09 19.47 -31 45 44.5           ~ 56 0
117 GRB 110721A gB 22 10 -38.6           ~ 135 0
118 GRB 161014A gB 22 10 35.42 +07 28 07.6           ~ 51 0
119 GRB 151021A gB 22 30 34.43 -33 11 50.4           ~ 54 0
120 Fermi bn150821406 gB 22 47 39.15 -57 53 38.2           ~ 52 0
121 GRB 131030A gB 23 00 16.14 -05 22 05.2           ~ 106 0
122 GRB 131103A gB 23 15 40.55 -44 38 25.4           ~ 38 0
123 Fermi bn100816026 gB 23 26 57.56 +26 34 42.6           ~ 149 0
124 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 302 0
125 SN 2012eb SN* 23 41 38.35 -46 11 07.0           SNIb/c 49 1
126 GRB 130701A gB 23 48 55.05 +36 06 01.2           ~ 69 0

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