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20012026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 28.7k across the 336 of their papers we have counts for

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Showing 2013 · astro-ph.HEShow all

16 papers · 2 filters

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★ 32 cited

Are gamma-ray bursts the same at high redshift and low redshift?

O. M. Littlejohns, N. R. Tanvir, R. Willingale +3

The majority of Swift gamma-ray bursts (GRBs) observed at z > 6 have prompt durations of T90 < 30s, which, at first sight, is surprising given that cosmological time-dilation means…

astro-ph.HE2013

Are GRBs the same at high and low redshift?

O. M. Littlejohns, N. R. Tanvir, R. Willingale +3

Due to their highly luminous nature, gamma-ray bursts (GRBs) are useful tools in studying the early Universe (up to z = 10). We consider whether the available subset of Swift high…

astro-ph.HE2013★ 1 cited

The low-extinction afterglow in the solar-metallicity host galaxy of GRB 110918A

J. Elliott, T. Krühler, J. Greiner +21

Galaxies selected through long gamma-ray bursts (GRBs) could be of fundamental importance when mapping the star formation history out to the highest redshifts. Before using them as…

astro-ph.HE2013★ 81 cited

GRB 120521C at z~6 and the Properties of High-redshift GRBs

T. Laskar, E. Berger, N. Tanvir +9

We present optical, near-infrared, and radio observations of the afterglow of GRB 120521C. By modeling the multi-wavelength dataset, we derive a photometric redshift of z~6.0, whic…

astro-ph.HE2013★ 34 cited

Hubble Space Telescope observations of the afterglow, supernova and host galaxy associated with the extremely bright GRB 130427A

A. J. Levan, N. R. Tanvir, A. S. Fruchter +13

We present Hubble Space Telescope (HST) observations of the exceptionally bright and luminous Swift gamma-ray burst, GRB 130427A. At z=0.34 this burst affords an excellent opportun…

astro-ph.HE2013★ 223 cited

The Afterglow of GRB 130427A from 1 to 10^16 GHz

D. A. Perley, S. B. Cenko, A. Corsi +31

We present multiwavelength observations of the afterglow of GRB 130427A, the brightest (in total fluence) gamma-ray burst of the past 29 years. Optical spectroscopy from Gemini-Nor…

astro-ph.HE2013★ 62 cited

The low-extinction afterglow in the solar-metallicity host galaxy of gamma-ray burst 110918A

J. Elliott, T. Krühler, J. Greiner +21

Metallicity is theoretically thought to be a fundamental driver in gamma-ray burst (GRB) explosions and energetics, but is still, even after more than a decade of extensive studies…

astro-ph.HE2013★ 746 cited

A "kilonova" associated with short-duration gamma-ray burst 130603B

N. R. Tanvir, A. J. Levan, A. S. Fruchter +4

Short-duration gamma-ray bursts (SGRBs) are intense flashes of cosmic gamma-rays, lasting less than ~2 s, whose origin is one of the great unsolved questions of astrophysics today.…

astro-ph.HE2013★ 71 cited

Superluminous X-rays from a superluminous supernova

A. J. Levan, A. M. Read, B. D. Metzger +2

The discovery of a population of superluminous supernovae (SLSNe), with peak luminosities a factor of ~100 brighter than normal SNe (typically SLSNe have M_V <-21), has shown an un…

astro-ph.HE2013★ 92 cited

Optical counterparts of the nearest ultraluminous X-ray sources

Jeanette C. Gladstone, Chris Copperwheat, Craig O. Heinke +5

We present a photometric survey of the optical counterparts of ultraluminous X-ray sources (ULXs) observed with the Hubble Space Telescope in nearby (< 5 Mpc) galaxies. Of the 33 U…

astro-ph.HE2013★ 79 cited

X-ray absorption evolution in Gamma-Ray Bursts: intergalactic medium or evolutionary signature of their host galaxies?

R. L. C. Starling, R. Willingale, N. R. Tanvir +5

The intrinsic X-ray emission of Gamma-Ray Bursts (GRBs) is often found to be absorbed over and above the column density through our own galaxy. The extra component is usually assum…

astro-ph.HE2013★ 206 cited

Demographics of the Galaxies Hosting Short-duration Gamma-Ray Bursts

Wen-fai Fong, Edo Berger, Ryan Chornock +17

We present observations of the afterglows and host galaxies of three short-duration gamma-ray bursts (GRBs): 100625A, 101219A and 110112A. We find that GRB 100625A occurred in a z=…

astro-ph.HE2013★ 293 cited

A new population of ultra-long duration gamma-ray bursts

A. J. Levan, N. R. Tanvir, R. L. C. Starling +38

We present comprehensive multiwavelength observations of three gamma-ray bursts (GRBs) with durations of several thousand seconds. We demonstrate that these events are extragalacti…

astro-ph.HE2013★ 499 cited

Signatures of magnetar central engines in short GRB lightcurves

A. Rowlinson, P. T. O'Brien, B. D. Metzger +2

A significant fraction of the Long Gamma-ray Bursts (LGRBs) in the Swift sample have a plateau phase showing evidence of ongoing energy injection. We suggest that many Short Gamma-…