2022ApJ...924...97W


Query : 2022ApJ...924...97W

2022ApJ...924...97W - Astrophys. J., 924, 97-97 (2022/January-2)

Standardized long gamma-ray bursts as a cosmic distance indicator.

WANG F.Y., HU J.P., ZHANG G.Q. and DAI Z.G.

Abstract (from CDS):

Gamma-ray bursts (GRBs) are the most luminous explosions in and can be detectable out to the edge of the universe. They have long been thought to be able to extend the Hubble diagram to very high redshifts. Several correlations between temporal or spectral properties and GRB luminosities have been proposed to make GRBs cosmological tools. However, those correlations cannot be properly standardized. In this paper, we select a long-GRB sample with X-ray plateau phases produced by electromagnetic dipole emissions from central newborn magnetars. A tight correlation is found between the plateau luminosity and the end time of the plateau in the X-ray afterglows out to the redshift z = 5.91. We standardize these long-GRB X-ray light curves to a universal behavior through this correlation, with a luminosity dispersion of 0.5 dex. The derived distance-redshift relation of GRBs is in agreement with the standard ΛCDM model both at low and high redshifts. The evidence for an accelerating universe from this GRB sample is 3σ, which is the highest statistical significance from GRBs to date.

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

Journal keyword(s): Gamma-ray bursts - Cosmological parameters - Magnetars

Simbad objects: 31

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Number of rows : 31
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 151112A gB 00 08 12.84 -61 39 47.7           ~ 37 0
2 GRB 190106A gB 01 59 31.23 +23 50 43.8           ~ 66 0
3 GRB 060906 gB 02 43 00.900 +30 21 42.12     19.84     ~ 147 0
4 GRB 141026A gB 02 56 20.29 +26 55 42.4           ~ 60 0
5 GRB 190114A gB 04 22 10.54 +02 11 29.1           ~ 47 0
6 GRB 090407 gB 04 35 54.98 -12 40 45.5           ~ 87 0
7 GRB 180329B gB 05 31 36.91 -23 41 27.4           ~ 49 0
8 GRB 160121A gB 07 16 21.15 -23 35 31.8           ~ 41 0
9 Fermi bn090516353 gB 09 12 59 -11 50.9           ~ 173 0
10 GRB 050505 gB 09 27 03.300 +30 16 23.70     20.74     ~ 206 0
11 Fermi bn161017745 gB 09 31 04.53 +43 07 35.0           ~ 75 0
12 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 222 1
13 GRB 171222A gB 09 53 06.69 +35 37 36.1           ~ 57 0
14 GRB 050319 gB 10 16 47.900 +43 32 53.80   18.02 17.01     ~ 274 0
15 GRB 111123A gB 10 19 23.17 -20 38 41.9           ~ 83 0
16 GRB 160227A gB 12 59 13.71 +78 40 45.1           ~ 69 0
17 GRB 051008 gB 13 31 28.100 +42 08 05.01 17.06   14.11     ~ 90 0
18 GRB 100424A gB 13 57 47.46 +01 32 20.3           ~ 71 0
19 GRB 080310 gB 14 40 13.89 -00 10 30.4           ~ 214 0
20 GRB 090205 gB 14 43 40.00 -27 50 51.4           ~ 99 0
21 GRB 140518A gB 15 09 00.60 +42 25 05.6           ~ 68 0
22 GRB 060526 gB 15 31 18.360 +00 17 04.90   18.31 17.16     ~ 288 0
23 GRB 120404A gB 15 40 02.29 +12 53 06.3           ~ 104 0
24 GRB 190719C gB 16 00 49.50 +13 00 00.6           ~ 43 0
25 GRB 130606A gB 16 37 35.12 +29 47 46.4           ~ 185 0
26 GRB 050814 gB 17 36 45.390 +46 20 21.60           ~ 166 0
27 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0
28 GRB 050315 gB 20 25 54.100 -42 36 02.19           ~ 225 0
29 GRB 060605 gB 21 28 37.320 -06 03 31.30   20.12 16.53     ~ 210 0
30 GRB 161014A gB 22 10 35.42 +07 28 07.6           ~ 69 0
31 GRB 061222A gB 23 53 03.419 +46 31 58.60           ~ 177 0

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