2012ApJ...755...85M


C.D.S. - SIMBAD4 rel 1.7 - 2021.05.17CEST04:10:52

2012ApJ...755...85M - Astrophys. J., 755, 85 (2012/August-3)

The optically unbiased GRB host (TOUGH) survey. VI. Radio observations at z ≲ 1 and consistency with typical star-forming galaxies.

MICHALOWSKI M.J., KAMBLE A., HJORTH J., MALESANI D., REINFRANK R.F., BONAVERA L., CASTRO CERON J.M., IBAR E., DUNLOP J.S., FYNBO J.P.U., GARRETT M.A., JAKOBSSON P., KAPLAN D.L., KRUHLER T., LEVAN A.J., MASSARDI M., PAL S., SOLLERMAN J., TANVIR N.R., VAN DER HORST A.J., WATSON D. and WIERSEMA K.

Abstract (from CDS):

The objective of this paper is to determine the level of obscured star formation activity and dust attenuation in a sample of gamma-ray burst (GRB) hosts, and to test the hypothesis that GRB hosts have properties consistent with those of the general star-forming galaxy populations. We present a radio continuum survey of all z < 1 GRB hosts in The Optically Unbiased GRB Host (TOUGH) sample supplemented with radio data for all (mostly pre-Swift) GRB-SN hosts discovered before 2006 October. We present new radio data for 22 objects and have obtained a detection for three of them (GRB 980425, 021211, 031203; none in the TOUGH sample), increasing the number of radio-detected GRB hosts from two to five. The star formation rate (SFR) for the GRB 021211 host of ∼825 M/yr, the highest ever reported for a GRB host, places it in the category of ultraluminous infrared galaxies. We found that at least ∼63% of GRB hosts have SFR < 100 M/yr and at most ∼8% can have SFR > 500 M/yr. For the undetected hosts the mean radio flux (<35 µJy 3σ) corresponds to an average SFR < 15 M/yr. Moreover, ≳ 88% of the z ≲ 1 GRB hosts have ultraviolet dust attenuation AUV< 6.7 mag (visual attenuation AV< 3 mag). Hence, we did not find evidence for large dust obscuration in a majority of GRB hosts. Finally, we found that the distributions of SFRs and AUV of GRB hosts are consistent with those of Lyman break galaxies, Hα emitters at similar redshifts, and of galaxies from cosmological simulations. The similarity of the GRB population with other star-forming galaxies is consistent with the hypothesis that GRBs, a least at z ≲ 1, trace a large fraction of all star formation, and are therefore less biased indicators than once thought.

Abstract Copyright:

Journal keyword(s): dust, extinction - galaxies: evolution - galaxies: ISM - galaxies: star formation - gamma-ray burst: general - radio continuum: galaxies

Simbad objects: 60

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Number of rows : 60

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 GRB 060912A gB 00 21 08.11 +20 58 18.9           ~ 90 1
2 ICRF J002225.4+001456 BiC 00 22 25.4258623 +00 14 56.161217   21.1       ~ 105 1
3 GRB 070808 gB 00 27 03.40 +01 10 35.4           ~ 48 0
4 ICRF J002914.2+345632 AGN 00 29 14.24246572 +34 56 32.2471186   20.2       ~ 122 1
5 GRB 050824 gB 00 48 56.100 +22 36 32.00 19.66 21.03 20.46 23.70   ~ 158 0
6 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9793 1
7 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 188 2
8 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2585 2
9 GRB 040924 gB 02 06 22.52 +16 08 48.8           ~ 149 1
10 GRB 000911 gB 02 18 42 +07 48.0           ~ 147 0
11 GRB 070318 gB 03 13 56.830 -42 56 46.30 18.27 16.23 15.49     ~ 147 0
12 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 850 1
13 QSO B0405-385 QSO 04 06 59.03533560 -38 26 28.0423567   19.55 18.0     ~ 212 2
14 QSO B0451-281 QSO 04 53 14.6470717184 -28 07 37.332338460   18.23 18.2 17.83   ~ 181 1
15 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 627 1
16 PKS 0515-674 Rad 05 15 37.30 -67 21 28.0           ~ 20 1
17 GRB 050915A gB 05 26 44.804 -28 00 59.27           ~ 69 0
18 QSO B0537-286 QSO 05 39 54.28147645 -28 39 55.9478122   19.70 20.0 18.789   ~ 250 1
19 GRB 051117B gB 05 40 43.260 -19 16 26.10           ~ 64 0
20 ICRF J054236.1+495107 Sy1 05 42 36.13789843 +49 51 07.2337251   18.45 17.80 17.210   ~ 1314 1
21 TXS 0542+498 Rad 05 45 57.91 +49 51 14.9           ~ 1 0
22 QSO B0607-157 QSO 06 09 40.9477650070 -15 42 40.649794982   18.47 18.0 19.90   ~ 294 1
23 GRB 060729 gB 06 21 31.850 -62 22 12.69           ~ 260 0
24 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 514 0
25 PMN J0808+0514 Rad 08 08 38.84780 +05 14 39.9410           ~ 3 0
26 SN 2002lt SN* 08 08 59.858 +06 43 37.52           SNIc: 339 1
27 GRB 020127 gB 08 15 05.8 +36 44 31           ~ 60 0
28 QSO B0826-373 QSO 08 28 04.78022012 -37 31 06.2809892   16       ~ 46 0
29 GRB 051016B gB 08 48 27.810 +13 39 20.00 20.45         ~ 125 0
30 QSO B0919-260 QSO 09 21 29.3546683923 -26 18 43.380586532   18.46 18.41 18.01   ~ 124 1
31 GRB 061021 gB 09 40 36.120 -21 57 05.40 18.21 19.20 16.82     ~ 127 0
32 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 182 1
33 M 82 IG 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 5453 6
34 GRB 980613 gB 10 17 57.8 +71 27 26           ~ 199 1
35 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1136 1
36 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 258 1
37 GRB 000418 gB 12 25 21 +20 05.0           ~ 202 0
38 GRB 050416 gB 12 33 54.600 +21 03 26.69     19.12     ~ 255 1
39 3C 286 Sy1 13 31 08.2885060664 +30 30 32.960825107   17.51 17.25     ~ 3866 2
40 GRB 080207 gB 13 50 03.02 +07 30 08.0           ~ 91 0
41 GRB 020405 gB 13 58 03.12 -31 22 22.2   21.9 21.5     ~ 239 1
42 GRB 060814 gB 14 45 21.480 +20 35 11.80           ~ 191 0
43 IC 4553 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 2745 4
44 GRB 991208 gB 16 33 53.51 +46 27 21.5           ~ 246 1
45 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 156 0
46 GRB 080325 gB 18 31 34.40 +36 31 26.1           ~ 64 0
47 SN 2005nc SN* 18 32 32.560 +26 20 22.34           SNIc: 353 1
48 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1686 2
49 ICRF J193925.0-634245 Sy2 19 39 25.02671 -63 42 45.6255   18.87 18.37 17.64   ~ 1013 1
50 GRB 060614 gB 21 23 32.140 -53 01 36.10 18.89 20.12 19.54     ~ 523 1
51 QSO B2155-152 QSO 21 58 06.28190211 -15 01 09.3278616   18.63 17.5 17.79   ~ 299 1
52 GRB 060505 gB 22 07 03.440 -27 48 51.89           ~ 230 1
53 GRB 061110A gB 22 25 09.800 -02 15 30.70 21.43         ~ 118 0
54 GRB 990712 gB 22 31 53.061 -73 24 28.58           ~ 253 1
55 QSO B2240-260 BLL 22 43 26.4091014700 -25 44 30.684062905   18.59   16.80   ~ 170 1
56 GRB 020903 gB 22 48 42.34 -20 46 09.3           ~ 218 1
57 GRB 010921 gB 22 55 59.90 +40 55 52.9           ~ 162 1
58 GRB 020819 gB 23 00 12 -43 00.7           ~ 120 1
59 GRB 051022A gB 23 56 04.200 +19 36 32.30           ~ 168 1
60 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 426 1

    Equat.    Gal    SGal    Ecl

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2021.05.17-04:10:52

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