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19962014
most citedCosmological Results from High-z Supernovae

1.7k citations · 6.6k across the 51 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.CO2009★ 120 cited

Dust and Metal Column Densities in Gamma-Ray Burst Host Galaxies

P. Schady, M. J. Page, S. R. Oates +7

In this paper we present the results from the analysis of a sample of 28 gamma-ray burst (GRB) afterglow spectral energy distributions, spanning the X-ray through to near-infrared…

astro-ph.SR2009★ 53 cited

Spectra and Light Curves of Failed Supernovae

Chris L. Fryer, Peter J. Brown, Filomena Bufano +11

Astronomers have proposed a number of mechanisms to produce supernova explosions. Although many of these mechanisms are now not considered primary engines behind supernovae, they d…

astro-ph.CO2009★ 625 cited

A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3

N. R. Tanvir, D. B. Fox, A. J. Levan +59

It is thought that the first generations of massive stars in the Universe were an important, and quite possibly dominant, source of the ultra-violet radiation that reionized the hy…

astro-ph.CO2009★ 94 cited

Ultraviolet Spectroscopy of Supernovae: The First Two Years of Swift Observations

F. Bufano, S. Immler, M. Turatto +13

We present the entire sample of ultraviolet (UV) spectra of supernovae (SNe) obtained with the Ultraviolet/Optical Telescope (UVOT) on board the Swift satellite during the first 2…

astro-ph2009★ 44 cited

Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst

N. P. M. Kuin, W. B. Landsman, M. J. Page +22

We present the earliest ever ultraviolet spectrum of a gamma-ray burst (GRB) as observed with the Swift-UVOT. The GRB 081203A spectrum was observed for 50 seconds with the UV grism…

astro-ph.HE2009★ 8 cited

The unusual X-ray light-curve of GRB 080307: the onset of the afterglow?

K. L. Page, R. Willingale, P. T. O'Brien +11

Swift-detected GRB 080307 showed an unusual smooth rise in its X-ray light-curve around 100 seconds after the burst, at the start of which the emission briefly softened. This `hump…