Gamma-ray bursts (GRBs) are the most luminous electromagnetic explosions in the
Universe, which emit up to 8.8× 10 54 erg isotropic equivalent energy in the hard X-ray …

Context. Gamma-ray bursts (GRBs) are the most energetics explosions in the Universe.
They are detectable up to very high redshifts. They may therefore be used to study the …

We study eight different gamma-ray burst (GRB) data sets to examine whether current GRB
measurements—that probe a largely unexplored part of cosmological redshift (z) space …

In this paper, we calibrate the Amati relation (the E p–E iso correlation) of gamma-ray bursts
(GRBs) in a cosmology-independent way. By using a Gaussian process to reconstruct the …

We calculate durations and spectral parameters for 218 Swift bursts detected by the BAT
instrument between and including gamma-ray bursts (GRBs) 041220 and 070509, including …

We use a nearly complete sample of gamma-ray bursts (GRBs) detected by the Swift
satellite to study the correlations between the spectral peak energy E peak of the prompt …

An important concern in the application of gamma-ray bursts (GRBs) to cosmology is that the
calibration of GRB luminosity/energy relations depends on the cosmological model, due to …

In this paper, we present two improved Amati correlations of gamma-ray burst (GRB) data
via a powerful statistical tool called copula. After calibrating with the low-redshift GRB data …

The current Swift sample of gamma-ray bursts (GRBs) with measured redshifts allows us to
test the assumption that GRBs trace star formation in the Universe. Some authors have …

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 …