2019ApJ...887...13F

Query : 2019ApJ...887...13F

2019ApJ...887...13F - Astrophys. J., 887, 13-13 (2019/December-2)

Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles.

FANA DIRIRSA F., RAZZAQUE S., PIRON F., ARIMOTO M., AXELSSON M., KOCEVSKI D., LONGO F., OHNO M. and ZHU S.

Abstract (from CDS):

Long duration gamma-ray bursts may serve as standard candles to constrain cosmological parameters by probing the Hubble diagram well beyond the range of redshift currently accessible using SNe Ia. The standardization of gamma-ray bursts (GRBs) is based on phenomenological relations between two or more parameters found from spectral modeling, one of which is strongly dependent on the cosmological model. The Amati relation links the source-frame energy Ei,p at which the prompt gamma-ray spectral energy distribution νFν peaks, and the isotropic-equivalent bolometric energy Eiso emitted during the prompt phase. We performed spectral analysis of 26 GRBs with known redshift that have been detected by the Fermi-Large Area Telescope (LAT) during its nine years of operations from 2008 July to 2017 September, thus extending the computation of Eiso to the 100 MeV range. Multiple components are required to fit the spectra of a number of GRBs. We found that the Amati relation is satisfied by the 25 LGRBs, with best-fit parameters similar to previous studies that used data from different satellite experiments, while the only short GRB with known redshift is an outlier. Using the Amati relation, we extend the Hubble diagram to redshift 4.35 and constrain the Hubble constant and dark-energy density in the ΛCDM model, with Fermi-LAT GRBs alone and together with another sample of 94 GRBs and with the latest Supernovae type-Ia data. Our results are consistent with the currently acceptable ranges of those cosmological parameters within errors.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Gamma-ray bursts - Cosmology - Astronomical radiation sources - Cosmological parameters

Simbad objects: 124

goto Full paper

goto View the references in ADS

Number of rows : 124
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 021004 gB 00 26 54.68 +18 55 41.6           ~ 560 0
2 Fermi bn131231198 gB 00 42 44.0 -01 29 40           ~ 103 0
3 GRB 050904 gB 00 54 50.794 +14 05 09.42           ~ 496 0
4 SN 2011kl SN* 00 57 22.64 -46 48 03.6           SNSLSN 268 1
5 Fermi bn100814160 gB 01 29 53.61 -17 59 43.6           ~ 219 0
6 GRB 081222 gB 01 30 57.76 -34 05 44.0           ~ 199 0
7 GRB 100906A gB 01 54 44.19 +55 37 49.8           ~ 233 0
8 Fermi bn091208410 gB 01 57 38.50 +16 52 50.7           ~ 220 0
9 GRB 060908 gB 02 07 18.360 +00 20 31.20 16.99 18.34 16.85     ~ 217 0
10 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
11 GRB 050603 gB 02 39 56.839 -25 10 54.92     18.48     ~ 174 0
12 Fermi bn110213220 gB 02 51 51.37 +49 16 21.2           ~ 175 0
13 SN 2013ez SN* 02 53 56.70 +13 23 13.6           ~ 118 0
14 GRB 120802A gB 02 59 22.04 +13 46 05.0           ~ 76 0
15 GRB 050318 gB 03 18 51.000 -46 23 43.61 18.10 18.68 17.58     ~ 189 0
16 GRB 060115 gB 03 36 08.400 +17 20 43.00           ~ 179 0
17 GRB 091029 gB 04 00 40.00 -55 57 12.7           ~ 168 0
18 GRB 111008A gB 04 01 48.220 -32 42 34.09           ~ 127 0
19 GRB 080913 gB 04 22 57.90 -25 07 38.6           ~ 213 0
20 Fermi bn131105087 gB 04 43 53.50 -63 00 17.7           ~ 95 0
21 Fermi bn150514774 gB 04 59 30.45 -60 58 07.0           ~ 51 0
22 GRB 060124 gB 05 08 25.900 +69 44 26.98   18.91 17.35     ~ 280 0
23 GRB 081118 gB 05 30 22.28 -43 18 03.1           ~ 79 0
24 Fermi bn100728095 gB 05 55 02.00 -15 15 20.2           ~ 157 0
25 GRB 081121 gB 05 57 07.70 -60 36 42.1           ~ 152 0
26 GRB 090328 gB 06 02 39.69 -41 52 55.1           ~ 194 1
27 GRB 000131 gB 06 13 31.08 -51 56 41.7     24.7     ~ 172 1
28 Fermi bn120711115 gB 06 18 42.839 -70 59 56.78           ~ 125 0
29 GRB 140213A gB 07 00 37.18 -73 08 14.1           ~ 102 0
30 GRB 110422A gB 07 28 11.21 +75 06 24.0           ~ 113 0
31 GRB 070125 gB 07 51 17.80 +31 09 04.8           ~ 188 0
32 GRB 071020 gB 07 58 39.65 +32 51 38.8           ~ 158 0
33 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
34 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 193 0
35 GRB 081028 gB 08 07 34.40 +02 18 16.8           ~ 125 0
36 GRB 020127 gB 08 15 05.8 +36 44 31           ~ 66 0
37 Fermi bn150314205 gB 08 26 40.82 +63 50 03.4           ~ 117 0
38 GRB 090102 gB 08 32 59.50 +33 06 25.7           ~ 253 0
39 Fermi bn111107035 gB 08 37 54.66 -66 31 12.3           ~ 97 0
40 GRB 110503A gB 08 51 06.31 +52 12 27.7           ~ 115 0
41 Fermi bn100704149 gB 08 54 33.92 -24 12 09.7           ~ 103 0
42 GRB 130408A gB 08 57 37.30 -32 21 38.9           ~ 98 0
43 Fermi bn090516353 gB 09 12 59 -11 50.9           ~ 173 0
44 GRB 130505A gB 09 17 21.9014988888 +01 42 03.426207768           ~ 94 0
45 GRB 020124 gB 09 32 50.8 -11 31 11           ~ 155 0
46 Fermi bn140206304 gB 09 41 16.90 +66 45 42.7           ~ 149 0
47 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 392 0
48 GRB 131108A gB 10 26 00.480 +09 39 44.05           ~ 96 0
49 GRB 110205A gB 10 58 31.12 +67 31 31.2           ~ 213 0
50 GRB 030323 gB 11 06 09.4 -21 46 13           ~ 138 1
51 GRB 011211 gB 11 15 16 -21 56.0           ~ 305 0
52 Fermi bn120624933 gB 11 23 31.98 +08 55 42.1           ~ 100 0
53 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
54 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 212 0
55 Fermi bn091020900 gB 11 42 55.20 +50 58 42.0           ~ 188 0
56 GRB 080603B gB 11 46 07.46 +68 03 38.5           ~ 153 0
57 GRB 971214 gB 11 56 26.4 +65 12 01           ~ 445 1
58 GRB 030328 gB 12 10 48.4 -09 20 51           ~ 148 0
59 GRB 030429 gB 12 13 07.495 -20 54 49.54     23.70     ~ 132 0
60 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
61 Fermi bn090323002 gB 12 42 50.28 +17 03 11.9           ~ 244 1
62 Fermi bn100414097 gB 12 48 30.0 +08 41 35           ~ 136 0
63 GRB 080607A gB 12 59 47.14 +15 55 09.6           ~ 257 0
64 Fermi bn130420313 gB 13 04 25.49 +59 25 26.8           ~ 112 0
65 Fermi bn120811649 gB 13 18 43.82 +62 18 02.8           ~ 113 0
66 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
67 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 499 1
68 GRB 130907A gB 14 23 34.03 +45 36 27.1           ~ 120 0
69 SN 2013dx SN* 14 29 14.77 +15 46 26.6           ~ 178 0
70 Fermi bn170405777 gB 14 39 18.66 -25 14 36.9           ~ 75 0
71 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
72 Fermi bn130610133 gB 14 57 40.91 +28 12 25.8           ~ 89 0
73 GRB 080721A gB 14 57 55.76 -11 43 24.9           ~ 180 0
74 GRB 990123 gB 15 25 29 +44 45.0     8.95     ~ 1012 1
75 GRB 060526 gB 15 31 18.360 +00 17 04.90   18.31 17.16     ~ 288 0
76 GRB 081203A gB 15 32 07.6 +63 31 15           ~ 177 0
77 Fermi bn120922939 gB 15 38 59.67 -20 10 55.0           ~ 88 0
78 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
79 GRB 110715A gB 15 50 44.090 -46 14 06.53           ~ 120 0
80 GRB 120724A gB 16 20 46.0 +03 30 33           ~ 51 0
81 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
82 GRB 130606A gB 16 37 35.12 +29 47 46.4           ~ 185 0
83 GRB 090715B gB 16 45 21.59 +44 50 20.1           ~ 144 0
84 GRB 091003A gB 16 46 04.680 +36 37 31.08           ~ 135 0
85 GRB 000926 gB 17 04 15 +51 46.0           ~ 373 0
86 GRB 170214A gB 17 05 21.94 -01 53 14.9           ~ 54 0
87 GRB 080319C gB 17 15 55.48 +55 23 31.7           ~ 174 0
88 Fermi bn130612141 gB 17 19 10.63 +16 43 11.8           ~ 89 0
89 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
90 Fermi bn090902462 gB 17 39 45.26 +27 19 28.1           ~ 440 0
91 Fermi bn100413732 gB 17 44 53.22 +15 50 02.4           ~ 62 0
92 GRB 090418 gB 17 57 15.2 +33 24 22           ~ 27 0
93 Fermi bn120326056 gB 18 15 37.06 +69 15 35.4           ~ 188 0
94 GRB 120909A gB 18 22 56.81 -59 26 54.9           ~ 103 0
95 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0
96 Fermi bn110731465 gB 18 42 00.99 -28 32 13.8           ~ 193 0
97 GRB 080413A gB 19 09 11.73 -27 40 39.6           ~ 163 0
98 GRB 130514A gB 19 45 07.33 -07 58 41.1           ~ 82 0
99 Fermi bn121128212 gB 20 02 23.88 +54 17 59.1           ~ 128 0
100 GRB 071003 gB 20 07 24.50 +10 56 48.8           ~ 181 0
101 GRB 160625B gB 20 34 23.67 +06 55 11.1           ~ 235 0
102 GRB 150403A gB 20 46 01.17 -62 42 40.1           ~ 116 0
103 Fermi bn160509374 gB 20 47 00.90 +76 06 30.1           ~ 141 0
104 GRB 160623A gB 21 01 11.54 +42 13 15.5           ~ 73 0
105 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
106 Fermi bn110818860 gB 21 09 20.890 -63 58 51.80           ~ 92 0
107 GRB 050922C gB 21 09 33.000 -08 45 30.10 15.15 15.86 14.69     ~ 301 0
108 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 109 0
109 GRB 080514B gB 21 31 22.61 +00 42 30.3           ~ 69 0
110 GRB 060927A gB 21 58 11.930 +05 21 50.32           ~ 215 0
111 GRB 051109A gB 22 01 15.320 +40 49 23.70   20.09 20.14     ~ 190 0
112 GRB 131117A gB 22 09 19.47 -31 45 44.5           ~ 67 0
113 GRB 110721A gB 22 10 -38.6           ~ 155 0
114 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
115 GRB 050820A gB 22 29 38.110 +19 33 37.10 18.33 19.00 18.47     ~ 409 0
116 GRB 131030A gB 23 00 16.14 -05 22 05.2           ~ 126 0
117 GRB 090812 gB 23 32 48.5 -10 36 17           ~ 165 0
118 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0
119 GRB 130518A gB 23 42 39.79 +47 27 55.2           ~ 86 0
120 Fermi bn080810549 gB 23 47 08.00 +00 18 35.1           ~ 240 0
121 GRB 060707 gB 23 48 19.000 -17 54 17.00     19.79     ~ 170 0
122 GRB 130701A gB 23 48 55.05 +36 06 01.2           ~ 81 0
123 SN 2013fu SN* 23 54 29.91 +29 25 47.6           SNIb/c 144 1
124 GRB 040912 gB 23 56 43.0 -00 55 20           ~ 39 0

To bookmark this query, right click on this link: simbad:objects in 2019ApJ...887...13F and select 'bookmark this link' or equivalent in the popup menu