2016A&A...593A..17G

Query : 2016A&A...593A..17G

2016A&A...593A..17G - Astronomy and Astrophysics, volume 593A17-17 (2016/9-1)

Probing dust-obscured star formation in the most massive gamma-ray burst host galaxies.

GREINER J., MICHALOWSKI M.J., KLOSE S., HUNT L.K., GENTILE G., KAMPHUIS P., HERRERO-ILLANA R., WIERINGA M., KRUHLER T., SCHADY P., ELLIOTT J., GRAHAM J.F., IBAR E., KNUST F., NICUESA GUELBENZU A., PALAZZI E., ROSSI A. and SAVAGLIO S.

Abstract (from CDS):

Context. As a result of their relation to massive stars, long-duration gamma-ray bursts (GRBs) allow the pinpointing of star formation in galaxies independent of redshift, dust obscuration, or galaxy mass/size, thus providing a unique tool to investigate star formation history over cosmic time.
Aims. About half of the optical afterglows of long-duration GRBs are missed owing to dust extinction and are primarily located in the most massive GRB hosts. It is important to investigate the amount of obscured star formation in these GRB host galaxies to understand this bias.
Methods. Radio emission of galaxies correlates with star formation, but does not suffer extinction as do the optical star formation estimators. We selected 11 GRB host galaxies with either large stellar mass or large UV-based and optical-based star formation rates (SFRs) and obtained radio observations of these with the Australia Telescope Compact Array and the Karl Jansky Very Large Array.
Results. Despite intentionally selecting GRB hosts with expected high SFRs, we do not find any radio emission related to star formation in any of our targets. Our upper limit for GRB 100621A implies that the earlier reported radio detection was due to afterglow emission. We detect radio emission from the position of GRB 020819B, but argue that it is in large part, if not completely, due to afterglow contamination.
Conclusions. Half of our sample has radio-derived SFR limits, which are only a factor 2-3 above the optically measured SFRs. This supports other recent studies that the majority of star formation in GRB hosts is not obscured by dust.

Abstract Copyright: © ESO, 2016

Journal keyword(s): galaxies: star formation - radio continuum: galaxies - gamma-ray burst: general

Simbad objects: 115

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Number of rows : 115
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 GRB 060912A gB 00 21 08.11 +20 58 18.9           ~ 116 1
2 [LJH2007] 1 G 00 21 08.16 +20 58 17.8           ~ 4 1
3 GRB 050824 gB 00 48 56.100 +22 36 32.00 19.66 21.03 20.46 23.70   ~ 184 0
4 [SKP2006] GRB 041006 Host G G 00 54 50.17 +01 14 07.0           ~ 5 0
5 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 202 2
6 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2924 2
7 QSO B0142-278 Bla 01 45 03.3949333872 -27 33 34.327137060   19.0 19.0 17.43   ~ 149 1
8 GRB 100901A gB 01 49 03.56 +22 45 30.6           ~ 170 0
9 ICRF J015537.0-404842 Sy2 01 55 37.05930363 -40 48 42.3570102   18.5       ~ 53 1
10 Fermi bn091208410 gB 01 57 38.50 +16 52 50.7           ~ 220 0
11 GRB 000210 gB 01 59 15 -40 40.0           ~ 175 0
12 [LDM2003] GRB J015915.5-403933 G 01 59 15.61 -40 39 33.1           ~ 13 0
13 [WSR2004] Host G G 02 06 22.52 +16 08 48.8           ~ 7 1
14 GRB 040924 gB 02 06 22.52 +16 08 48.8           ~ 169 1
15 Fermi bn090113778 gB 02 08 16.00 +33 26 08.4           ~ 92 0
16 GRB 110918A gB 02 10 09.39 -27 06 19.6           ~ 83 0
17 [PBK2002] GRB 000911 Host Galaxy G 02 18 34.360 +07 44 27.65           ~ 7 0
18 GRB 000911 gB 02 18 42 +07 48.0           ~ 163 0
19 QSO B0220-349 Bla 02 22 56.40164366 -34 41 28.7302247   21.39   21.10   ~ 79 1
20 QSO B0237-2322 QSO 02 40 08.1743783856 -23 09 15.729012036   16.78 16.63     ~ 516 1
21 [KGS2011] GRB 090926B host G G 03 05 13.91 -39 00 22.6 23.71         ~ 4 0
22 Fermi bn090926914 gB 03 05 14.30 -38 59 50.9           ~ 149 1
23 GRB 070318 gB 03 13 56.830 -42 56 46.30 18.27 16.23 15.49     ~ 170 0
24 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
25 2XMM J032139.6+165202 G 03 21 39.693 +16 52 01.74           ~ 18 1
26 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
27 [LDM2003] GRB J050146.7+114654 G 05 01 46.7 +11 46 54           ~ 10 1
28 GRB 990705 gB 05 09 54.5 -72 07 53           ~ 229 1
29 [LDM2002] J050954.8-720754 G 05 09 54.8 -72 07 54           ~ 15 1
30 GRB 050915 gB 05 26 44.81 -28 01 00.3           ~ 15 0
31 GRB 051117B gB 05 40 43.260 -19 16 26.10           ~ 77 0
32 ICRF J054236.1+495107 Sy1 05 42 36.13789710 +49 51 07.2337139   18.45 17.80 17.210   ~ 1573 1
33 2XMM J062131.8-622212 X 06 21 31.8 -62 22 12           ~ 1 0
34 GRB 060729 gB 06 21 31.850 -62 22 12.69           ~ 303 0
35 GRB 080517 gB 06 48 58.00 +50 44 06.3           ~ 52 1
36 GALEXASC J064858.00+504407.9 UV 06 48 58.00 +50 44 07.9           ~ 4 1
37 SN 2010bh SN* 07 10 30.63 -56 15 19.7           SNIc 336 1
38 Anon J071031-5615 G 07 10 31 -56 15.3           ~ 7 0
39 GRB 051006 gB 07 23 13.520 +09 30 24.48           ~ 74 0
40 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
41 Anon J080230-3951 G 08 02 30.20 -39 51 03.0 22.31 22.32 20.53 20.44 19.40 ~ 20 0
42 Anon J080859+0643 G 08 08 59.0 +06 43 37           ~ 3 1
43 SN 2002lt SN* 08 08 59.858 +06 43 37.52           SNIc: 363 1
44 [F2002] B16 G 08 15 01.42 +36 46 33.9         23.56 ~ 5 0
45 GRB 020127 gB 08 15 05.8 +36 44 31           ~ 66 0
46 4C 39.23A Bla 08 24 55.48385834 +39 16 41.9040476   18.55 18.21 17.20   ~ 238 1
47 ICRF J082526.8-501038 QSO 08 25 26.8673494560 -50 10 38.484054768   20.94       ~ 139 1
48 GRB 051016B gB 08 48 27.810 +13 39 20.00 20.45         ~ 153 0
49 GRB 061021 gB 09 40 36.120 -21 57 05.40 18.21 19.20 16.82     ~ 160 0
50 GRB 061121 gB 09 48 54.570 -13 11 42.68 17.19 17.71 17.02     ~ 350 0
51 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 222 1
52 SDSS J095223.31+102855.4 G 09 52 23.32 +10 28 55.4       23.00   ~ 7 0
53 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
54 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
55 GRB 050219 gB 11 05 39.03 -40 41 00.8           ~ 11 0
56 QSO B1104-445 Bla 11 07 08.69412105 -44 49 07.6183013   17.84 18.2 17.37   ~ 260 1
57 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 286 1
58 Anon J113429-7601 G 11 34 29.88 -76 01 41.6           ~ 9 0
59 [BCK2003] G1 G 12 25 19.3 +20 06 11           ~ 19 0
60 GRB 000418 gB 12 25 21 +20 05.0           ~ 219 0
61 [CKG2005] Host G G 12 33 54.6 +21 03 27           ~ 5 1
62 GRB 050416 gB 12 33 54.600 +21 03 26.69     19.12     ~ 300 1
63 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
64 GRB 050801 gB 13 36 35.000 -21 55 41.00 15.03 15.82 15.46     ~ 164 0
65 [RKF2012] GRB080207 B G 13 50 02.97 +07 30 07.2       26.49   ~ 6 0
66 GRB 080207 gB 13 50 03.02 +07 30 08.0           ~ 114 0
67 [MPP2003] GRB 020405 abs 0.6908 G 13 58 03.01 -31 22 24.7           ~ 7 1
68 GRB 020405 gB 13 58 03.12 -31 22 22.2   21.9 21.5     ~ 259 1
69 3C 295 Sy1 14 11 20.6 +52 12 09   22.34 20.80 18.54   ~ 1021 4
70 GRB 060814 gB 14 45 21.480 +20 35 11.80           ~ 241 0
71 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
72 GRB 111005A gB 14 53 15.60 -19 43 19.1           ~ 78 0
73 [LDM2003] GRB J163353.5+462721 G 16 33 53.5 +46 27 21           ~ 10 1
74 GRB 991208 gB 16 33 53.51 +46 27 21.5           ~ 269 1
75 ICRF J163828.2+623444 Sy2 16 38 28.22535940 +62 34 44.3168151   20.7 20.7     ~ 167 2
76 QSO J1700-2610 QSO 17 00 53.15406418 -26 10 51.7253944   16.50       ~ 119 2
77 GRB 030528 gB 17 04 00.3 -22 37 10           ~ 90 1
78 [RSG2005] GRB 030528 Host G G 17 04 02 -22 39.0           ~ 4 1
79 GRB 080319C gB 17 15 55.48 +55 23 31.7           ~ 174 0
80 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
81 [KGS2011] GRB 080605 host G G 17 28 30.05 +04 00 56.0           ~ 3 0
82 4C 09.57 BLL 17 51 32.81857326 +09 39 00.7284066   17.46 16.78 15.57   ~ 1007 1
83 GRB 050223 gB 18 05 32.200 -62 28 20.40           ~ 109 0
84 SN 2005nc SN* 18 32 32.560 +26 20 22.34           SNIc: 400 1
85 Anon J183232+2620 G 18 32 32.58 +26 20 22.6           ~ 7 0
86 [TSC98] Host G G 19 34 54 -52 49.9           ~ 20 1
87 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
88 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1332 2
89 GRB 071003 gB 20 07 24.50 +10 56 48.8           ~ 181 0
90 PKS J2009-4849 BLL 20 09 25.3903899240 -48 49 53.725051056   15.75 12.81 11.41   ~ 604 1
91 [UNN2010] GRB 100621A host G G 21 01 13.08 -51 06 22.5           ~ 3 0
92 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
93 [PBF2006d] Host Galaxy G 21 23 27.0 -53 02 02           ~ 15 1
94 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
95 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0
96 [KGS2011] GRB 081109 host G G 22 03 09.63 -54 42 39.9 23.23   22.85   21.96 ~ 3 0
97 Fermi bn081109293 gB 22 03 11.50 -54 42 40.5           ~ 125 1
98 GRB 060505 gB 22 07 03.440 -27 48 51.89           ~ 286 1
99 2dFGRS TGS173Z112 G 22 07 03.5 -27 48 57 18.43 18.89 18.27 17.90 17.51 ~ 18 1
100 GRB 061110A gB 22 25 09.800 -02 15 30.70 21.43         ~ 134 0
101 GRB 990712 gB 22 31 53.061 -73 24 28.58           ~ 268 1
102 [LDM2003] GRB J223153.1-732429 G 22 31 53.1 -73 24 29           ~ 14 1
103 QSO B2232-488 Bla 22 35 13.23657823 -48 35 58.7945202   17.61 17.2     ~ 150 1
104 SN 2008hw SN* 22 39 50.39 -40 08 49.1           SNIc 197 1
105 APMUKS (BJ) B224600.67-210204.6 G 22 48 42.3391 -20 46 08.945   20.7 20.8     ~ 12 1
106 GRB 020903 gB 22 48 42.34 -20 46 09.3           ~ 248 1
107 GRB 010921 gB 22 55 59.90 +40 55 52.9           ~ 173 1
108 [LDM2003] GRB J225559.9+405553 G 22 55 59.9 +40 55 53           ~ 12 1
109 GRB 020819 gB 23 00 12 -43 00.7           ~ 135 1
110 [FB2003] J232719.475+061555.95 rG 23 27 19.475 +06 15 55.95           ~ 11 1
111 4C 09.74 Bla 23 46 36.8384562240 +09 30 45.514903032   16.23 15.97 15.99   ~ 332 2
112 [CDB2005b] B G 23 56 04.10 +19 36 24.2           ~ 12 1
113 GRB 051022A gB 23 56 04.200 +19 36 32.30           ~ 194 1
114 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 453 1
115 [LDM2003] GRB J235906.7+083507 G 23 59 06.7 +08 35 07   23.04 23.02     ~ 23 1

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