2022MNRAS.510.2928C


Query : 2022MNRAS.510.2928C

2022MNRAS.510.2928C - Mon. Not. R. Astron. Soc., 510, 2928-2947 (2022/February-3)

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

CAO S., KHADKA N. and RATRA B.

Abstract (from CDS):

We show that each of the three Dainotti-correlated gamma-ray burst (GRB) data sets recently compiled by Wang et al. and Hu et al., that together probe the redshift range 0.35 <= z <= 5.91, obey cosmological-model-independent Dainotti correlations and so are standardizable. We use these GRB data in conjunction with the best currently available Amati-correlated GRB data, that probe 0.3399 <= z <= 8.2, to constrain cosmological model parameters. The resulting cosmological constraints are weak, providing lower limits on the non-relativistic matter density parameter, mildly favouring non-zero spatial curvature, and largely consistent with currently accelerated cosmological expansion as well as with constraints determined from better-established data.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

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

Simbad objects: 6

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Number of rows : 6
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 091029 gB 04 00 40.00 -55 57 12.7           ~ 168 0
2 Fermi bn131105087 gB 04 43 53.50 -63 00 17.7           ~ 95 0
3 Fermi bn090516353 gB 09 12 59 -11 50.9           ~ 173 0
4 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
5 GRB 060526 gB 15 31 18.360 +00 17 04.90   18.31 17.16     ~ 288 0
6 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0

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