activity
20082025
most citedCosmology-Independent Distance Moduli of 42 Gamma-Ray Bursts between Redshift of 1.44 and 6.60

28 citations · 46 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2025

Decadal evolution of a repeating fast radio burst source

P. Wang, J. S. Zhang, Y. P. Yang +48

The origin of fast radio bursts (FRBs), the brightest cosmic radio explosions, is still unknown. Bearing critical clues to FRBs' origin, the long-term evolution of FRBs has yet to…

astro-ph.HE2009★ 2 cited

Analysis of the Swift Gamma-Ray Bursts duration

I. Horvath, L. G. Balazs, Z. Bagoly +3

Two classes of gamma-ray bursts have been identified in the BATSE catalogs characterized by durations shorter and longer than about 2 seconds. There are, however, some indications…

astro-ph.CO2009★ 1 cited

Combined Swift BAT-XRT Lightcurves

P. Veres, Z. Bagoly, J. Kelemen +4

In this paper we make an attempt to combine the two kinds of data from the Swift-XRT instrument (windowed timing and photon counting modes) and the from BAT. A thorough desription…

astro-ph2008★ 28 cited

Cosmology-Independent Distance Moduli of 42 Gamma-Ray Bursts between Redshift of 1.44 and 6.60

Nan Liang, Shuang Nan Zhang

This report is an update and extension of our paper accepted for publication in ApJ (arXiv:0802.4262). Since objects at the same redshift should have the same luminosity distance a…

astro-ph2008★ 14 cited

Temporal variability of GRB early X-ray afterglows and GRB080319B prompt emission

R. Margutti, C. Guidorzi, G. Chincarini +3

We performed the first systematic search for the minimum variability time scale between 0.3 and 10 keV studying the 28 brightest early (<3000 s) afterglows detected by Swift-XRT up…

astro-ph2008★ 1 cited

Non-thermal emission from supernova shock breakout and the origin of the X-ray transient associated with SN2008D

Xiang-Yu Wang, Zhuo Li, Eli Waxman +1

We suggest that non-thermal emission can be produced by multiple scatterings of the photons between the supernova ejecta and pre-shock material in supernova shock breakout. Such bu…