activity
19972025
most citedMethods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

1.8k citations · 14.4k across the 145 of their papers we have counts for

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Showing 2009 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2009★ 5 cited

X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst

K. L. Page, J. P. Osborne, A. M. Read +6

Aims: The launch of Swift has allowed many more novae to be observed regularly over the X-ray band. Such X-ray observations of novae can reveal ejecta shocks and the nuclear burnin…

astro-ph.HE2009★ 62 cited

Swift observations of the X-ray and UV evolution of V2491 Cyg (Nova Cyg 2008 No. 2)

K. L. Page, J. P. Osborne, P. A. Evans +8

We present extensive, high-density Swift observations of V2491 Cyg (Nova Cyg 2008 No. 2). Observing the X-ray emission from only one day after the nova discovery, the source is fol…

astro-ph.HE2009

The phases of X-ray emission of RS Oph

J. -U. Ness, S. Starrfield, K. L. Page +3

The recurrent symbiotic nova RS Oph reoccurred after 21 years on 12 February 2006. In contrast to the 1985 outburst, much denser coverage with X-ray observations was achieved. Swif…

astro-ph.HE2009★ 56 cited

Multi-wavelength observations of the energetic GRB 080810: detailed mapping of the broadband spectral evolution

K. L. Page, R. Willingale, E. Bissaldi +31

GRB 080810 was one of the first bursts to trigger both Swift and the Fermi Gamma-ray Space Telescope. It was subsequently monitored over the X-ray and UV/optical bands by Swift, in…

astro-ph.HE2009★ 246 cited

The 22-Month Swift-BAT All-Sky Hard X-ray Survey

J. Tueller, W. H. Baumgartner, C. B. Markwardt +36

We present the catalog of sources detected in the first 22 months of data from the hard X-ray survey (14--195 keV) conducted with the BAT coded mask imager on the \swift satellite.…

astro-ph.HE2009★ 37 cited

Swift X-ray and UV monitoring of the Classical Nova V458 Vul (Nova Vul 2007)

J. -U. Ness, J. J. Drake, A. P. Beardmore +18

We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vu…