activity
20082012
most citedTests for Standard Accretion Disk Models by Variability in Active Galactic Nuclei

48 citations · 164 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2012★ 14 cited

Energy-Dependent GRB Pulse Width due to the Curvature Effect and Intrinsic Band Spectrum

Z. Y. Peng, X. H. Zhao, Y. Yin +2

Previous studies have found that the width of gamma-ray burst (GRB) pulse is energy dependent and that it decreases as a power-law function with increasing photon energy. In this w…

astro-ph.HE2011★ 17 cited

Spectral lag of gamma-ray burst caused by the intrinsic spectral evolution and the curvature effect

Z. Y. Peng, Y. Yin, X. W. Bi +2

Assuming an intrinsic `Band' shape spectrum and an intrinsic energy-independent emission profile we have investigated the connection between the evolution of the rest-frame spectra…

astro-ph.HE2010★ 14 cited

The Temporal and Spectral Characteristics of "Fast Rise and Exponential Decay" Gamma-Ray Burst Pulses

Z. Y. Peng, Y. Yin, X. W. Bi +4

In this paper we have analyzed the temporal and spectral behavior of 52 Fast Rise and Exponential Decay (FRED) pulses in 48 long-duration gamma-ray bursts (GRBs) observed by the CG…

astro-ph.CO2009★ 21 cited

Absorption of 10 Gev--1 Tev Gamma Rays from 3C 279

J. M. Bai, H. T. Liu, L. Ma

In this paper, we revisit gamma-ray--emitting region for 10 GeV--1 TeV gamma rays from 3C 279 through studying the photon-photon absorption optical depth due to the diffuse radiati…

astro-ph2008★ 10 cited

Spectral hardness evolution characteristics of tracking Gamma-ray Burst pulses

Z. Y. Peng, L. Ma, R. J. Lu +3

Employing a sample presented by Kaneko et al. (2006) and Kocevski et al. (2003), we select 42 individual tracking pulses (here we defined tracking as the cases in which the hardnes…

astro-ph2008★ 40 cited

Absorption of 10 Gev--1 Tev Gamma Rays by Radiation from Broad-Line Region in 3C 279

H. T. Liu, J. M. Bai, L. Ma

In this paper, we study the photon-photon pair production optical depth for 10 GeV--1 TeV gamma rays from 3C 279 due to the diffuse radiation of broad-line region (BLR). Assuming a…