activity
20062017
most citedDiscerning the physical origins of cosmological Gamma-ray bursts based on multiple observational criteria: the cases of z=6.7 GRB 080913, z=8.3 GRB 090423, and some short/hard GRBs

440 citations · 1.6k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2017★ 7 cited

Colour variations in the GRB 120327A afterglow

A. Melandri, S. Covino, E. Zaninoni +42

We present a comprehensive temporal and spectral analysis of the long Swift GRB 120327A afterglow data to investigate the possible causes of the observed early time colour variatio…

astro-ph.HE2015★ 22 cited

Limits on optical polarization during the prompt phase of GRB 140430A

D. Kopac, C. G. Mundell, J. Japelj +17

Gamma-ray burst GRB 140430A was detected by the Swift satellite and observed promptly with the imaging polarimeter RINGO3 mounted on the Liverpool Telescope, with observations begi…

astro-ph.HE2015

Radio flares from gamma-ray bursts

D. Kopac, C. G. Mundell, S. Kobayashi +6

We present predictions of centimeter and millimeter radio emission from reverse shocks in the early afterglows of gamma-ray bursts with the goal of determining their detectability…

astro-ph.HE2014★ 26 cited

The nature of the late achromatic bump in GRB 120326A

A. Melandri, F. J. Virgili, C. Guidorzi +24

The long gamma-ray burst GRB 120326A at redshift exhibited a multi-band light curve with a striking feature: a late-time, long-lasting achromatic rebrighten…

astro-ph.HE2014★ 74 cited

Phenomenology of Reverse-Shock Emission in the Optical Afterglows of Gamma Ray Bursts

J. Japelj, D. Kopac, S. Kobayashi +6

We use a parent sample of 118 gamma-ray burst (GRB) afterglows, with known redshift and host galaxy extinction, to separate afterglows with and without signatures of dominant rever…

astro-ph.HE2013★ 18 cited

The optical rebrightening of GRB100814A: an interplay of forward and reverse shocks?

Massimiliano De Pasquale, N. P. M. Kuin, S. Oates +36

We present a wide dataset of gamma-ray, X-ray, UVOIR, and radio observations of the Swift GRB100814A. At the end of the slow decline phase of the X-ray and optical afterglow, this…

astro-ph.HE2013★ 35 cited

New constraints on GRB jet geometry and relativistic shock physics

C. Guidorzi, C. G. Mundell, R. Harrison +23

We use high--quality, multi-band observations of Swift GRB120404A, from gamma-ray to radio frequencies, together with the new hydrodynamics code of van Eerten et al. (2012) to test…

astro-ph.HE2013★ 134 cited

GRB 130427A: a Nearby Ordinary Monster

A. Maselli, A. Melandri, L. Nava +63

Long-duration Gamma-Ray Bursts (GRBs) are an extremely rare outcome of the collapse of massive stars, and are typically found in the distant Universe. Because of its intrinsic lumi…

astro-ph.HE2013★ 93 cited

GRB 091024A and the nature of ultra-long gamma-ray bursts

F. J. Virgili, C. G. Mundell, V. Pal'shin +30

We present a broadband study of gamma-ray burst (GRB) 091024A within the context of other ultra-long-duration GRBs. An unusually long burst detected by Konus-Wind, Swift, and Fermi…

astro-ph.HE2013★ 36 cited

GRB 090727 and gamma-ray bursts with early time optical emission

D. Kopac, S. Kobayashi, A. Gomboc +9

We present a multi-wavelength analysis of gamma-ray burst GRB 090727, for which optical emission was detected during the prompt gamma-ray emission by the 2-m autonomous robotic Liv…

astro-ph.HE2011★ 37 cited

Spectral and temporal analysis of the joint Swift/BAT-Fermi/GBM GRB sample

Francisco Virgili, Ying Qin, Bing Zhang +1

Using the gamma-ray bursts simultaneously detected by Swift/BAT and Fermi/GBM we performed a joint spectral and temporal analysis of the prompt emission data and confirm the rough…

astro-ph.HE2011★ 99 cited

Fermi and Swift Gamma-Ray Burst Afterglow Population Studies

J. L. Racusin, S. R. Oates, P. Schady +15

The new and extreme population of GRBs detected by Fermi-LAT shows several new features in high energy gamma-rays that are providing interesting and unexpected clues into GRB promp…

astro-ph.HE2011★ 69 cited

Gamma-ray burst rate: high-redshift excess and its possible origins

Francisco J. Virgili, Bing Zhang, Kentaro Nagamine +1

Prompted by various analyses of long (Type II) GRB rates and their relationship to the cosmic star-formation history, metallicity and luminosity function evolution, we systematical…

astro-ph.HE2009★ 80 cited

Are all short-hard gamma-ray bursts produced from mergers of compact stellar objects?

Francisco J. Virgili, Bing Zhang, Paul O'Brien +1

The origin and progenitors of short-hard gamma-ray bursts remain a puzzle and a highly debated topic. Recent Swift observations suggest that these GRBs may be related to catastroph…

astro-ph.HE2009★ 440 cited

Discerning the physical origins of cosmological Gamma-ray bursts based on multiple observational criteria: the cases of z=6.7 GRB 080913, z=8.3 GRB 090423, and some short/hard GRBs

Bing Zhang, Bin-Bin Zhang, Francisco J. Virgili +10

(Abridged) The two high-redshift gamma-ray bursts, GRB 080913 at z=6.7 and GRB 090423 at z=8.3, recently detected by Swift appear as intrinsically short, hard GRBs. They could have…

astro-ph2008★ 131 cited

Low-Luminosity Gamma-Ray Bursts as a Distinct GRB Population:A Firmer Case from Multiple Criteria Constraints

Francisco Virgili, Enwei Liang, Bing Zhang

The intriguing observations of Swift/BAT X-ray flash XRF 060218 and the BATSE-BeppoSAX gamma-ray burst GRB 980425, both with much lower luminosity and redshift compared to other ob…

astro-ph2006★ 314 cited

Low Luminosity Gamma-Ray Bursts as a Unique Population: Luminosity Function, Local Rate, and Beaming Factor

Enwei Liang, Bing Zhang, Francisco Virgili +1

Swift/BAT has detected ~ 200 long-duration GRBs, with redshift measurements for ~50 of them. We derive the luminosity function (Phi^{HL}) and the local event rate (rho_0^{HL}) of t…