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Query : 2019A&A...623A..26P |
2019A&A...623A..26P - Astronomy and Astrophysics, volume 623A, 26-26 (2019/3-1)
Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift/BAT6 complete sample of bright LGRBs. III. Stellar masses, star formation rates, and metallicities at z > 1.
PALMERIO J.T., VERGANI S.D., SALVATERRA R., SANDERS R.L., JAPELJ J., VIDAL-GARCIA A., D'AVANZO P., CORRE D., PERLEY D.A., SHAPLEY A.E., BOISSIER S., GREINER J., LE FLOC'H E. and WISEMAN P.
Abstract (from CDS):
Abstract Copyright: © J. T. Palmerio et al. 2019
Journal keyword(s): gamma-ray burst: general - galaxies: star formation - galaxies: abundances
Simbad objects: 29
Number of rows : 29 |
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 | NAME SMC | G | 00 52 38.0 | -72 48 01 | 2.79 | 2.2 | ~ | 11149 | 1 | |||
2 | Fermi bn081221681 | gB | 01 03 10.2 | -24 32 53 | ~ | 157 | 0 | |||||
3 | GRB 080602 | gB | 01 16 42.18 | -09 13 55.4 | ~ | 55 | 0 | |||||
4 | GRB 081222 | gB | 01 30 57.76 | -34 05 44.0 | ~ | 176 | 0 | |||||
5 | Fermi bn091208410 | gB | 01 57 38.50 | +16 52 50.7 | ~ | 191 | 0 | |||||
6 | GRB 060908 | gB | 02 07 18.360 | +00 20 31.20 | 16.99 | 18.34 | 16.85 | ~ | 199 | 0 | ||
7 | GRB 060306 | gB | 02 44 22.830 | -02 08 55.00 | ~ | 108 | 0 | |||||
8 | Fermi bn100728439 | gB | 02 56 13.44 | +00 16 51.6 | ~ | 121 | 0 | |||||
9 | Fermi bn090926914 | gB | 03 05 14.30 | -38 59 50.9 | ~ | 131 | 1 | |||||
10 | GRB 061007 | gB | 03 05 19.510 | -50 30 02.50 | 14.28 | 14.40 | 12.95 | ~ | 289 | 1 | ||
11 | GRB 050318 | gB | 03 18 51.000 | -46 23 43.61 | 18.10 | 18.68 | 17.58 | ~ | 178 | 0 | ||
12 | GRB 070328 | gB | 04 20 27.680 | -34 04 00.60 | 20.29 | ~ | 87 | 0 | ||||
13 | GRB 081121 | gB | 05 57 07.70 | -60 36 42.1 | ~ | 132 | 0 | |||||
14 | GRB 090201 | gB | 06 08 12.30 | -46 36 16.1 | ~ | 60 | 0 | |||||
15 | GRB 080517 | gB | 06 48 58.00 | +50 44 06.3 | ~ | 50 | 1 | |||||
16 | GRB 061121 | gB | 09 48 54.570 | -13 11 42.68 | 17.19 | 17.71 | 17.02 | ~ | 326 | 0 | ||
17 | GRB 070306 | gB | 09 52 23.220 | +10 28 55.20 | ~ | 206 | 1 | |||||
18 | Fermi bn100615083 | gB | 11 48 49.25 | -19 28 52.2 | ~ | 112 | 0 | |||||
19 | GRB 050802 | gB | 14 37 05.820 | +27 47 12.62 | 16.85 | 17.38 | 16.97 | ~ | 173 | 0 | ||
20 | GRB 060814 | gB | 14 45 21.480 | +20 35 11.80 | ~ | 218 | 0 | |||||
21 | GRB 080721A | gB | 14 57 55.76 | -11 43 24.9 | ~ | 164 | 0 | |||||
22 | GRB 050401 | gB | 16 31 28.84 | +02 11 14.5 | ~ | 335 | 0 | |||||
23 | GRB 080605 | gB | 17 28 30.04 | +04 00 56.9 | ~ | 176 | 0 | |||||
24 | SN 1998bw | SN* | 19 35 03.17 | -52 50 46.1 | 14.09 | SNIc | 1821 | 2 | ||||
25 | GRB 050922C | gB | 21 09 33.000 | -08 45 30.10 | 15.15 | 15.86 | 14.69 | ~ | 282 | 0 | ||
26 | GRB 080413B | gB | 21 44 34.62 | -19 58 51.2 | ~ | 168 | 0 | |||||
27 | Fermi bn080804972 | gB | 21 54 41.90 | -53 11 20.2 | ~ | 137 | 0 | |||||
28 | GRB 071117 | gB | 22 20 10.40 | -63 26 36.6 | ~ | 101 | 0 | |||||
29 | GRB 090812 | gB | 23 32 48.5 | -10 36 17 | ~ | 143 | 0 |
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