2022ApJ...940...56F

Query : 2022ApJ...940...56F

2022ApJ...940...56F - Astrophys. J., 940, 56 (2022/November-3)

Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets.

FONG W.-F., NUGENT A.E., DONG Y., BERGER E., PATERSON K., CHORNOCK R., LEVAN A., BLANCHARD P., ALEXANDER K.D., ANDREWS J., COBB B.E., CUCCHIARA A., FOX D., FRYER C.L., GORDON A.C., KILPATRICK C.D., LUNNAN R., MARGUTTI R., MILLER A., MILNE P., NICHOLL M., PERLEY D., RASTINEJAD J., ROUCO ESCORIAL A., SCHROEDER G., SMITH N., TANVIR N. and TERRERAN G.

Abstract (from CDS):

We present a comprehensive optical and near-infrared census of the fields of 90 short gamma-ray bursts (GRBs) discovered in 2005-2021, constituting all short GRBs for which host galaxy associations are feasible (≈60% of the total Swift short GRB population). We contribute 274 new multi-band imaging observations across 58 distinct GRBs and 26 spectra of their host galaxies. Supplemented by literature and archival survey data, the catalog contains 542 photometric and 42 spectroscopic data sets. The photometric catalog reaches 3σ depths of ≳24-27 mag and ≳23-26 mag for the optical and near-infrared bands, respectively. We identify host galaxies for 84 bursts, in which the most robust associations make up 56% (50/90) of events, while only a small fraction, 6.7%, have inconclusive host associations. Based on new spectroscopy, we determine 18 host spectroscopic redshifts with a range of z ≈ 0.15-1.5 and find that ≈23%-41% of Swift short GRBs originate from z > 1. We also present the galactocentric offset catalog for 84 short GRBs. Taking into account the large range of individual measurement uncertainties, we find a median of projected offset of ≈7.7 kpc, for which the bursts with the most robust associations have a smaller median of ≈4.8 kpc. Our catalog captures more high-redshift and low-luminosity hosts, and more highly offset bursts than previously found, thereby diversifying the population of known short GRB hosts and properties. In terms of locations and host luminosities, the populations of short GRBs with and without detectable extended emission are statistically indistinguishable. This suggests that they arise from the same progenitors, or from multiple progenitors, which form and evolve in similar environments. All of the data products are available on the Broadband Repository for Investigating Gamma-Ray Burst Host Traits website.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Stellar populations - Gamma-ray bursts - Gravitational wave sources

VizieR on-line data: <Available at CDS (J/ApJ/940/56): table2.dat tablea1.dat refs.dat>

Nomenclature: Fig. 2, Table 2: [FND2022] GRB YYMMDDA Host G N=85.

Simbad objects: 129

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Number of rows : 129
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 SDSS J002243.71-001657.5 G 00 22 43.71720 -00 16 57.5256           ~ 69 0
2 GRB 140930B gB 00 25 23.40 +24 17 41.7           ~ 52 0
3 [FND2022] GRB 140930B Host G G 00 25 23.4730 +24 17 37.930           ~ 1 0
4 GRB 200826A gB 00 27 08.47 +34 01 36.5           ~ 121 0
5 Fermi bn150120123 G 00 41 16.5630 +33 59 42.598           ~ 70 0
6 Fermi bn100117879 G 00 45 04.6610 -01 35 42.020           ~ 155 0
7 Fermi bn111117510 gB 00 50 46.220 +23 00 39.22           ~ 141 0
8 [FND2022] GRB 111117A Host G G 00 50 46.2680 +23 00 41.410           ~ 1 0
9 [FND2022] GRB 100625A Host G G 01 03 10.9180 -39 05 18.440           ~ 1 0
10 GRB 100625A gB 01 03 10.98 -39 05 18.3           ~ 124 0
11 [FND2022] GRB 170127B Host G G 01 19 54.4150 -30 21 29.615           ~ 1 0
12 Fermi bn170127634 gB 01 19 54.47 -30 21 28.6           ~ 36 0
13 GRB 180805B gB 01 43 07.59 -17 29 36.4           ~ 32 0
14 [FND2022] GRB 180805B Host G G 01 43 07.6550 -17 29 33.091           ~ 1 0
15 PSO J027.8085-18.5940 G 01 51 14.05011120 -18 35 38.4976680           ~ 192 0
16 GRB 130822A gB 01 51 41.27 -03 12 31.7           ~ 34 0
17 [FND2022] GRB 130822A Host G G 01 51 42.7080 -03 12 25.447           ~ 1 0
18 NGC 821 AG? 02 08 21.1358498040 +10 59 41.832436704   12.210 11.310 10.739 9.744 ~ 592 0
19 GRB 141212A G 02 36 29.9570 +18 08 47.228           ~ 70 0
20 PSO J047.1631+13.1580 G 03 08 39.14930640 +13 09 29.0253240           ~ 144 0
21 GRB 120305A gB 03 10 08.73 +28 29 30.9           ~ 56 0
22 [FND2022] GRB 120305A Host G G 03 10 08.7540 +28 29 35.870           ~ 1 0
23 [FND2022] GRB 130912A Host G G 03 10 22.2000 +13 59 48.740           ~ 1 0
24 Fermi bn130912358 gB 03 10 25.60 +13 59 55.7           ~ 57 0
25 [FND2022] GRB 200411A Host G G 03 10 39.1350 -52 18 59.545           ~ 1 0
26 GRB 200411A gB 03 10 39.39 -52 19 03.3           ~ 31 0
27 [FND2022] GRB 070729 Host G G 03 45 15.8080 -39 19 18.590           ~ 1 0
28 GRB 070729 gB 03 45 16.04 -39 19 19.9           ~ 81 0
29 GRB 070714B G 03 51 22.2720 +28 17 50.943           ~ 248 0
30 GRB 071227A G 03 52 31.0260 -55 59 00.890           ~ 201 0
31 [FND2022] GRB 170728A Host G G 03 55 33.1160 +12 10 51.040           ~ 1 0
32 GRB 170728A gB 03 55 36 +12 10.0           ~ 22 0
33 GRB 201006A gB 04 07 34.25 +65 09 52.8           ~ 30 0
34 GRB 060313 G 04 26 28.4020 -10 50 39.901 20.55 21.03 19.66     ~ 156 0
35 [FND2022] GRB 161001A Host G G 04 47 40.5300 -57 15 39.184           ~ 1 0
36 Fermi bn161001045 gB 04 47 40.84 -57 15 39.9           ~ 41 0
37 GRB 101219A gB 04 58 20.45 -02 32 23.1           ~ 152 0
38 [FND2022] GRB 101219A Host G G 04 58 20.4970 -02 32 22.450           ~ 1 0
39 [FND2022] GRB 161104A Host G G 05 11 34.3700 -51 27 36.290           ~ 1 0
40 GRB 161104A gB 05 11 34.45 -51 27 36.3           ~ 28 0
41 GRB 210919A gB 05 21 01.05 +01 18 42.1           ~ 41 0
42 [FND2022] GRB 210919A Host G G 05 21 01.9540 +01 18 40.022           ~ 1 0
43 GRB 200907B G 05 56 06.9510 +06 54 22.637           ~ 24 0
44 GRB 061006 G 07 24 07.8080 -79 11 55.188           ~ 214 0
45 [FND2022] GRB 091109B Host G G 07 30 56.5500 -54 05 23.220           ~ 1 0
46 GRB 091109B gB 07 30 59.90 -54 05 30.6           ~ 57 0
47 Fermi bn081226044 G 08 02 00.4500 -69 01 49.500           ~ 63 0
48 [FND2022] GRB 160408A Host G G 08 10 29.5800 +71 07 45.030           ~ 1 0
49 Fermi bn160408268 gB 08 10 29.93 +71 07 41.7           ~ 45 0
50 NAME GRB 060121 HOST Galaxy G 09 09 52.0260 +45 39 45.538       26.6   ~ 127 0
51 SDSS J093805.33+153719.0 G 09 38 05.33384 +15 37 19.0406           ~ 146 0
52 GRB 160525B G 09 57 32.2460 +51 12 24.600           ~ 30 0
53 GRB 160410A gB 10 02 44.37 +03 28 42.7           ~ 75 0
54 GRB 150424A gB 10 09 13.35 -26 37 51.2           ~ 94 0
55 [FND2022] GRB 150424A Host G G 10 09 13.4060 -26 37 51.745           ~ 1 0
56 [FND2022] GRB 090515 Host G G 10 56 35.8470 +14 26 42.840           ~ 1 0
57 GRB 090515 gB 10 56 41.0 +14 27 22           ~ 122 0
58 GRB 121226A G 11 14 34.1210 -30 24 22.840           ~ 44 0
59 [FND2022] GRB 160303A Host G G 11 14 48.1190 +22 44 33.420           ~ 1 0
60 GRB 160303A gB 11 14 48.16 +22 44 31.3           ~ 47 0
61 Fermi bn180618030 G 11 19 45.8010 +73 50 15.030           ~ 38 0
62 Fermi bn180418281 G 11 20 29.2100 +24 55 58.734           ~ 57 0
63 GRB 211023B G 11 21 14.3110 +39 08 08.360           ~ 32 0
64 [FND2022] GRB 201221D Host G G 11 24 14.0640 +42 08 40.047           ~ 1 0
65 GRB 201221D gB 11 24 14.19 +42 08 35.5           ~ 48 0
66 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0
67 Fermi bn130716442 gB 11 58 17.69 +63 03 11.6           ~ 27 0
68 [FND2022] GRB 130716A Host G G 11 58 17.8620 +63 03 15.350           ~ 1 0
69 GRB 181123B G 12 17 27.9100 +14 35 52.270           ~ 47 0
70 GALEX J123205.0-105600 Bz? 12 32 04.9717245480 -10 56 00.722548932         16.421 ~ 186 0
71 SDSS J123612.87+285858.8 BiC 12 36 12.8803407000 +28 58 58.780075656           ~ 328 1
72 GRB 090426 G 12 36 18.0470 +32 59 09.460           ~ 237 0
73 GRB 210726A G 12 53 09.8200 +19 11 25.032           ~ 36 0
74 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
75 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
76 PSO J203.7673-22.1424 G 13 35 04.16044560 -22 08 32.8717680           ~ 178 0
77 SDSS J140910.47+275320.8 G 14 09 10.47535 +27 53 20.8393           ~ 279 0
78 GRB 060801 G 14 12 01.2620 +16 58 55.970           ~ 172 0
79 GRB 150831A gB 14 44 05.84 -25 38 06.3           ~ 38 0
80 [FND2022] GRB 150831A Host G G 14 44 05.9390 -25 38 05.780           ~ 1 0
81 GRB 150423A gB 14 46 18.96 +12 17 00.6           ~ 79 0
82 GRB 120804A G 15 35 47.5100 -28 46 56.110           ~ 99 0
83 GRB 160601A G 15 39 43.9490 +64 32 30.604           ~ 34 0
84 Fermi bn170728961 G 15 51 55.5290 +70 07 22.038           ~ 54 0
85 GRB 140903A G 15 52 03.2650 +27 36 10.710           ~ 138 0
86 GRB 090305 G 16 07 07.5960 -31 33 22.540           ~ 53 0
87 GRB 050813 gB 16 07 57.190 +11 14 57.80           ~ 147 0
88 [FND2022] GRB 050813 Host G GiC 16 07 57.2000 +11 14 53.090       23.43 22.43 ~ 5 0
89 UGCS J162444.39-273226.8 G 16 24 44.38275 -27 32 26.8381     19.70     ~ 469 1
90 GRB 140516A gB 16 51 57.40 +39 57 46.3           ~ 38 0
91 GRB 160927A gB 17 04 58.19 +17 19 55.3           ~ 34 0
92 NAME GRB 070707 HOST Galaxy G 17 50 58.5550 -68 55 27.600       27.3   ~ 63 0
93 [FND2022] GRB 160821B Host G G 18 39 53.9940 +62 23 34.427           ~ 2 0
94 Fermi bn160821937 gB 18 39 54.550 +62 23 30.35           ~ 190 0
95 [FND2022] GRB 191031D Host G G 18 53 09.5220 +47 38 40.130           ~ 1 0
96 GRB 191031D gB 18 53 09.57 +47 38 38.5           ~ 46 0
97 [FND2022] GRB 130515A Host G G 18 53 45.0210 -54 16 50.720           ~ 1 0
98 Fermi bn130515056 gB 18 53 45.65 -54 16 45.0           ~ 55 0
99 PSO J285.9246+45.7134 G 19 03 41.90914320 +45 42 48.4220520           ~ 63 0
100 GRB 080503 gB 19 06 28.74 +68 47 35.8           ~ 172 0
101 [FND2022] GRB 080503 Host G G 19 06 28.9010 +68 47 34.780           ~ 1 0
102 Fermi bn080905499 G 19 10 42.0450 -18 52 54.510           ~ 200 0
103 PSO J292.2283+33.9161 G 19 28 54.81164400 +33 54 58.1227560           ~ 25 0
104 [FND2022] GRB 131004A Host G G 19 44 27.0640 -02 57 30.429           ~ 1 0
105 Fermi bn131004904 gB 19 44 27.20 -02 57 31.0           ~ 113 0
106 GRB 140622A gB 21 08 41.56 -14 25 09.5           ~ 61 0
107 [FND2022] GRB 140622A Host G G 21 08 41.7440 -14 25 06.166           ~ 1 0
108 Fermi bn210323918 G 21 11 47.3200 +25 22 09.989           ~ 44 0
109 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
110 GRB 140129B G 21 47 01.6490 +26 12 23.270           ~ 30 0
111 GRB 070429B G 21 52 03.6910 -38 49 42.820           ~ 125 0
112 GRB 051221 G 21 54 48.626 +16 53 27.16 19.49         ~ 377 0
113 [FND2022] GRB 151229A Host G G 21 57 28.7010 -20 43 54.800           ~ 1 0
114 Fermi bn151229285 gB 21 57 28.78 -20 43 55.2           ~ 38 0
115 GRB 110112A gB 21 59 43.77 +26 27 24.4           ~ 47 0
116 GRB 170428A G 22 00 18.7100 +26 54 56.280           ~ 52 0
117 GRB 051210 gB 22 00 40.930 -57 36 47.10           ~ 138 0
118 [FND2022] GRB 051210 Host G G 22 00 40.9420 -57 36 47.063           ~ 1 0
119 SDSS J220046.14+293839.3 G 22 00 46.14864 +29 38 39.3144           ~ 2 0
120 Fermi bn160624477 gB 22 00 46.21 +29 38 37.8           ~ 69 0
121 GRB 061201 gB 22 08 32.060 -74 34 47.90           ~ 205 0
122 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
123 GRB 080123 gB 22 35 46.100 -64 54 03.24           ~ 98 0
124 [FND2022] GRB 080123 Host G G 22 35 46.9430 -64 53 54.973           ~ 1 0
125 Fermi bn200219317 G 22 50 33.1080 -59 07 11.579           ~ 42 0
126 GRB 211106A G 22 54 20.5410 -53 13 50.548           ~ 38 0
127 NVSS J230126-385839 rG 23 01 26.7650 -38 58 40.422   22.22 21.22 21   ~ 325 1
128 GRB 180727A G 23 06 40.0380 -63 03 07.088           ~ 29 0
129 Fermi bn160411062 G 23 17 25.3550 -40 14 30.560           ~ 34 0

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