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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 2006Show all

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astro-ph2006★ 50 cited

Early Ultraviolet, Optical and X-Ray Observations of the Type IIP SN 2005cs in M51 with Swift

Peter J. Brown, Luc Dessart, Stephen T. Holland +14

We report early photospheric-phase observations of the Type IIP Supernova (SN) 2005cs obtained by Swift's Ultraviolet-Optical and X-Ray Telescopes. Observations started within two…

astro-ph2006★ 380 cited

The gamma-ray burst GRB060614 requires a novel explosive process

A. Gal-Yam, D. Fox, P. Price +26

Over the past decade our physical understanding of gamma-ray bursts (GRBs) has progressed rapidly thanks to the discovery and observation of their long-lived afterglow emission. Lo…

astro-ph2006★ 82 cited

X-Ray Observations of Type Ia Supernovae with Swift: Evidence for Circumstellar Interaction for SN 2005ke

S. Immler, P. J. Brown, P. Milne +15

We present a study of the early (days to weeks) X-ray and UV properties of eight Type Ia supernovae (SNe Ia) which have been extensively observed with the X-Ray Telescope (XRT) and…

astro-ph2006★ 74 cited

GRB 060313: A New Paradigm for Short-Hard Bursts?

Peter W. A. Roming, Daniel Vanden Berk, Valentin Palshin +22

We report the simultaneous observations of the prompt emission in the gamma-ray and hard X-ray bands by the Swift-BAT and the KONUS-Wind instruments of the short-hard burst, GRB 06…

astro-ph2006★ 32 cited

Optical, Infrared, and Ultraviolet Observations of the X-Ray Flash GRB 050416A

S. T. Holland, P. T. Boyd, J. Gorosabel +25

We present ultraviolet, optical, and infrared photometry of the afterglow of the X-ray flash XRF 050416A taken between approximately 100 seconds and 36 days after the burst. We fin…

astro-ph2006★ 22 cited

Swift Observations of GRB 050603: An afterglow with a steep late time decay slope

Dirk Grupe, Peter Brown, Jay Cummings +16

We report the results of Swift observations of the Gamma Ray Burst GRB 050603. With a V magnitude V=18.2 about 10 hours after the burst the optical afterglow was the brightest so f…