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most citedColor Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data

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astro-ph.HE2015★ 17 cited

Exploring the canonical behaviour of long gamma-ray bursts using an intrinsic multi-wavelength afterglow correlation

S. R. Oates, J. L. Racusin, M. De Pasquale +6

In this paper we further investigate the relationship, reported by Oates et al., 2012, between the optical/UV afterglow luminosity (measured at restframe 200s) and average afterglo…

astro-ph.HE2015★ 41 cited

Gamma-Ray Bursts as Sources of Strong Magnetic Fields

Jonathan Granot, Tsvi Piran, Omer Bromberg +2

Gamma-Ray Bursts (GRBs) are the strongest explosions in the Universe, which due to their extreme character likely involve some of the strongest magnetic fields in nature. This revi…

astro-ph.HE2015★ 3 cited

The statistics of BAT-to-XRT flux ratio in GRB: Evidence for a characteristic value and its implications

Demosthenes Kazanas, Judith L. Racusin, Joseph Sultana +1

We present the statistics of the ratio, , between the prompt and afterglow "plateau" fluxes of GRB. This we define as the ratio between the mean prompt energy flux in {\e…

astro-ph.HE2015★ 88 cited

Towards a Better Understanding of the GRB Phenomenon: a New Model for GRB Prompt Emission and its effects on the New Non-Thermal L-E relation

S. Guiriec, C. Kouveliotou, F. Daigne +14

We reanalyze the prompt emission of two of the brightest Fermi GRBs (080916C and 090926A) with a new model composed of 3 components: (i) a thermal-like component--approximated with…

astro-ph.HE2015★ 1 cited

The Statistics of the Prompt-to-Afterglow GRB Flux Ratios and the Supercritical Pile GRB Model

D. Kazanas, J. L. Racusin, J. Sultana +1

We present the statistics of the ratio, , between the prompt and afterglow "plateau" fluxes of GRB. This we define as the ratio between the mean prompt energy flux in…