2022MNRAS.512..439C

Query : 2022MNRAS.512..439C

2022MNRAS.512..439C - Mon. Not. R. Astron. Soc., 512, 439-454 (2022/May-1)

Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters.

CAO S., DAINOTTI M. and RATRA B.

Abstract (from CDS):

We show that the Platinum gamma-ray burst (GRB) data compilation, probing the redshift range 0.553 <= z <= 5.0, obeys a cosmological-model-independent three-parameter Fundamental Plane (Dainotti) correlation and so is standardizable. While they probe the largely unexplored z ∼ 2.3-5 part of cosmological redshift space, the GRB cosmological parameter constraints are consistent with, but less precise than, those from a combination of baryon acoustic oscillation (BAO) and Hubble parameter [H(z)] data. In order to increase the precision of GRB-only cosmological constraints, we exclude common GRBs from the larger Amati-correlated A118 data set composed of 118 GRBs and jointly analyse the remaining 101 Amati-correlated GRBs with the 50 Platinum GRBs. This joint 151 GRB data set probes the largely unexplored z ∼ 2.3-8.2 region; the resulting GRB-only cosmological constraints are more restrictive, and consistent with, but less precise than, those from H(z) + BAO data.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): cosmological parameters - cosmology: observations - dark energy - gamma-ray bursts

Simbad objects: 50

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Number of rows : 50
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 070110 gB 00 03 39.270 -52 58 27.00 21.8 21.9 21.2     ~ 220 0
2 GRB 150910A gB 00 22 40.14 +33 28 22.4           ~ 79 0
3 GRB 060708 gB 00 31 13.850 -33 45 32.40 19.07 19.79 17.37     ~ 109 0
4 Fermi bn081221681 gB 01 03 10.2 -24 32 53           ~ 186 0
5 GRB 190106A gB 01 59 31.23 +23 50 43.8           ~ 66 0
6 GRB 091018 gB 02 08 46 -57 33.0           ~ 169 0
7 GRB 060906 gB 02 43 00.900 +30 21 42.12     19.84     ~ 147 0
8 Fermi bn110213220 gB 02 51 51.37 +49 16 21.2           ~ 175 0
9 GRB 140509A gB 03 06 22.79 -62 38 20.9           ~ 31 0
10 GRB 091029 gB 04 00 40.00 -55 57 12.7           ~ 168 0
11 GRB 111008A gB 04 01 48.220 -32 42 34.09           ~ 127 0
12 GRB 190114A gB 04 22 10.54 +02 11 29.1           ~ 47 0
13 Fermi bn131105087 gB 04 43 53.50 -63 00 17.7           ~ 95 0
14 GRB 180329B gB 05 31 36.91 -23 41 27.4           ~ 49 0
15 GRB 160121A gB 07 16 21.15 -23 35 31.8           ~ 41 0
16 Fermi bn120118709 gB 08 19 29.05 -07 11 05.1           ~ 87 0
17 Fermi bn150314205 gB 08 26 40.82 +63 50 03.4           ~ 117 0
18 GRB 140419A gB 08 27 57.56 +46 14 25.3           ~ 95 0
19 Fermi bn140206304 gB 09 41 16.90 +66 45 42.7           ~ 149 0
20 GRB 160327A gB 09 46 48.56 +54 00 46.4           ~ 43 0
21 GRB 061121 gB 09 48 54.570 -13 11 42.68 17.19 17.71 17.02     ~ 350 0
22 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 222 1
23 GRB 170202A gB 10 10 06 +05 01.0           ~ 90 0
24 GRB 100219A gB 10 16 48.48 -12 34 00.0           ~ 130 0
25 GRB 080430 gB 11 01 14.63 +51 41 07.8           ~ 157 0
26 Fermi bn091020900 gB 11 42 55.20 +50 58 42.0           ~ 188 0
27 Fermi bn170705115 gB 12 49 +17.9           ~ 66 0
28 GRB 160227A gB 12 59 13.71 +78 40 45.1           ~ 69 0
29 Fermi bn120811649 gB 13 18 43.82 +62 18 02.8           ~ 113 0
30 GRB 080310 gB 14 40 13.89 -00 10 30.4           ~ 214 0
31 GRB 060814 gB 14 45 21.480 +20 35 11.80           ~ 241 0
32 GRB 080721A gB 14 57 55.76 -11 43 24.9           ~ 180 0
33 GRB 060714 gB 15 11 26.450 -06 33 58.30   20.21 18.54     ~ 209 0
34 Fermi bn120922939 gB 15 38 59.67 -20 10 55.0           ~ 88 0
35 GRB 120404A gB 15 40 02.29 +12 53 06.3           ~ 104 0
36 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
37 GRB 070521 gB 16 10 38.600 +30 15 22.70           ~ 164 0
38 GRB 140629A gB 16 35 54.44 +41 52 36.7           ~ 89 0
39 GRB 090418A gB 17 57 15.17 +33 24 21.1           ~ 101 0
40 Fermi bn151027166 gB 18 09 56.87 +61 21 12.3           ~ 143 0
41 Fermi bn140506880 gB 18 27 06.04 -55 38 08.7           ~ 113 0
42 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0
43 GRB 070529 gB 18 54 58.230 +20 39 34.00 20.38   17.25     ~ 98 0
44 Fermi bn121128212 gB 20 02 23.88 +54 17 59.1           ~ 128 0
45 GRB 150403A gB 20 46 01.17 -62 42 40.1           ~ 116 0
46 GRB 070508 gB 20 51 11.810 -78 23 04.88     19.62     ~ 144 0
47 Fermi bn110818860 gB 21 09 20.890 -63 58 51.80           ~ 92 0
48 GRB 060605 gB 21 28 37.320 -06 03 31.30   20.12 16.53     ~ 210 0
49 GRB 131030A gB 23 00 16.14 -05 22 05.2           ~ 126 0
50 GRB 061222A gB 23 53 03.419 +46 31 58.60           ~ 177 0

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