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The collimation-corrected gamma-ray burst energies correlate with the peak energy of their νFν spectrum
We consider all bursts with known redshift and νF ν peak energy, E. For a good fraction of
them an estimate of the jet opening angle is available from the achromatic break of their …
them an estimate of the jet opening angle is available from the achromatic break of their …
The Ep,i–Eiso correlation in gamma-ray bursts: updated observational status, re-analysis and main implications
The correlation between the cosmological rest-frame νFν spectrum peak energy, E p, i, and
the isotropic-equivalent radiated energy, E iso, discovered by in 2002 and …
the isotropic-equivalent radiated energy, E iso, discovered by in 2002 and …
Swift/UVOT: 18 Years of Long GRB Discoveries and Advances
S Oates - Universe, 2023 - mdpi.com
The Neil Gehrels Swift Observatory (Swift) has been in operation for 18 years. The Ultra-
Violet/Optical Telescope (UVOT) onboard Swift was designed to capture the earliest …
Violet/Optical Telescope (UVOT) onboard Swift was designed to capture the earliest …
Model-independent multivariable gamma-ray burst luminosity indicator and its possible cosmological implications
Without imposing any theoretical models and assumptions, we present a multivariable
regression analysis to several observable quantities for a sample of 15 gamma-ray bursts …
regression analysis to several observable quantities for a sample of 15 gamma-ray bursts …
Swift identification of dark gamma-ray bursts
We present an optical flux versus X-ray flux diagram for all known gamma-ray bursts (GRBs)
for which an X-ray afterglow has been detected. We propose an operational definition of …
for which an X-ray afterglow has been detected. We propose an operational definition of …
Evidence for supernova signatures in the spectrum of the late-time bump of the optical afterglow of GRB 021211
We present photometric and spectroscopic observations of the gamma-ray burst GRB
021211 obtained during the late stages of its afterglow. The light curve shows a …
021211 obtained during the late stages of its afterglow. The light curve shows a …
Toward a more standardized candle using gamma-ray burst energetics and spectra
The use of gamma-ray burst (GRB) energetics for cosmography has long been advanced as
a means to probe out to high redshifts, to the epoch of deceleration. However, although …
a means to probe out to high redshifts, to the epoch of deceleration. However, although …
The diversity of gamma-ray burst afterglows and the surroundings of massive stars
The finding of a Type Ic supernova connected with GRB 030329 showed a massive star
origin for this burst, supporting evidence for this association in previous bursts with light …
origin for this burst, supporting evidence for this association in previous bursts with light …
Lorentz-factor–isotropic-luminosity/energy correlations of gamma-ray bursts and their interpretation
The bulk Lorentz factor of the gamma-ray burst (GRB) ejecta (Γ 0) is a key parameter to
understanding GRB physics. Liang et al. have discovered a correlation between Γ 0 and …
understanding GRB physics. Liang et al. have discovered a correlation between Γ 0 and …
A unified treatment of the gamma-ray burst 021211 and its afterglow
The gamma-ray burst (GRB) 021211 had a simple light curve, containing only one peak and
the expected Poisson fluctuations. Such a burst may be attributed to an external shock …
the expected Poisson fluctuations. Such a burst may be attributed to an external shock …