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20042018
most citedThe Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts

148 citations · 799 across the 22 of their papers we have counts for

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astro-ph.HE2018★ 16 cited

Absolute Distances to Nearby Type Ia Supernovae via Light Curve Fitting Methods

J. Vinkó, A. Ordasi, T. Szalai +22

We present a comparative study of absolute distances to a sample of very nearby, bright Type Ia supernovae (SNe) derived from high cadence, high signal-to-noise, multi-band photome…

astro-ph.HE2015★ 30 cited

The early phases of the type Iax supernova SN 2011ay

Tamás Szalai, József Vinkó, Krisztián Sárneczky +7

We present a detailed study of the early phases of the peculiar supernova 2011ay based on BVRI photometry obtained at Konkoly Observatory, Hungary, and optical spectra taken with t…

astro-ph.HE2011

Photometry of Some Recent Gamma-ray Bursts

József Kóbori, János Kelemen, Péter Veres +2

We present the results of the optical, X-ray and gamma-ray analysis of some recent GRBs. The data were obtained by the automated P60 telescope and the Swift telescope (UVOT, XRT an…

astro-ph.HE2010★ 4 cited

Directional Anisotropy of Swift Gamma-Ray Bursts

Péter Veres, Zsolt Bagoly, István Horváth +3

Swift satellite measurements contributed substantially to the gamma-ray burst (GRB) redshift observations through fast slewing to the source of the GRBs. Still, a large number of b…

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.HE2009★ 148 cited

The Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts

S. B. Cenko, D. A. Frail, F. A. Harrison +22

Long-duration gamma-ray bursts (GRBs) are widely believed to be highly-collimated explosions (opening angle theta ~ 1-10 deg). As a result of this beaming factor, the true energy r…