activity
20052009
most citedNonthermal Hard X-ray Emission and Iron Kalpha Emission from a Superflare on II Pegasi

105 citations · 283 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph.HE200950 cited

Monitoring Supergiant Fast X-ray Transients with Swift. Results from the first year

P. Romano, L. Sidoli, G. Cusumano +12

Swift has allowed the possibility to give Supergiant Fast X-ray Transients (SFXTs), the new class of High Mass X-ray Binaries discovered by INTEGRAL, non serendipitous attention th…

astro-ph200729 cited

GRB 060607A: A GRB with Bright Asynchronous Early -ray and Optical Emissions

Houri Ziaeepour, Stephen T. Holland, Patricia T. Boyd +8

The early optical emission of the moderately high redshift () GRB 060607A shows a remarkable broad and strong peak with a rapid rise and a relatively slow power-law decay.…

astro-ph20073 cited

Discovery of the accretion-powered millisecond pulsar SWIFT J1756.9-2508 with a low-mass companion

H. A. Krimm, C. B. Markwardt, C. J. Deloye +10

We report on the discovery by the Swift Gamma-Ray Burst Explorer of the eighth known transient accretion-powered millisecond pulsar, SWIFT J1756.9-2508, as part of routine observat…

astro-ph2006105 cited

Nonthermal Hard X-ray Emission and Iron Kalpha Emission from a Superflare on II Pegasi

R. A. Osten, S. Drake, J. Tueller +4

We report on an X-ray flare detected on the active binary system II~Pegasi with the Swift telescope. The trigger had a 10-200 keV luminosity of 2.2 erg s-- a…

astro-ph200696 cited

The X-ray afterglow of the short gamma ray burst 050724

S. Campana, G. Tagliaferri, D. Lazzati +23

Short duration (<2 s) Gamma-ray bursts (GRBs) have been a mystery since their discovery. Until May 2005 very little was known about short GRBs, but this situation has changed rapid…

astro-ph2005

Confirmation of the $\eps$ -- $\eiso$ (Amati) relation from the X-ray flash XRF 050416A observed by Swift/BAT

T. Sakamoto, L. Barbier, S. D. Barthelmy +10

We report Swift Burst Alert Telescope (BAT) observations of the X-ray Flash (XRF) XRF 050416A. The fluence ratio between the 15-25 keV and 25-50 keV energy bands of this event is 1…