activity
20042025
most citedThe Swift/BAT Hard X-ray Transient Monitor

582 citations · 5k across the 65 of their papers we have counts for

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astro-ph2008★ 1 cited

Swift monitoring of Supergiant Fast X-ray Transients: the out-of-outburst behaviour and the flares from IGRJ17544-2916 and XTEJ1739-302

L. Sidoli, P. Romano, G. Cusumano +10

Supergiant Fast X-ray Transients (SFXTs) are a sub-class of High Mass X-ray Binaries (HMXBs) associated with OB supergiant companions and displaying transient X-ray activity. This…

astro-ph2008★ 41 cited

Monitoring Supergiant Fast X-ray Transients with Swift. III. Outbursts of the prototypical SFXTs IGR J17544-2619 and XTE J1739-302

L. Sidoli, P. Romano, V. Mangano +7

IGR J17544-2619 and XTE J1739-302 are considered the prototypical sources of the new class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients (SFXTs).These sources w…

astro-ph2008★ 513 cited

An extremely luminous X-ray outburst at the birth of a supernova

A. M. Soderberg, E. Berger, K. L. Page +40

Massive stars end their short lives in spectacular explosions, supernovae, that synthesize new elements and drive galaxy evolution. Throughout history supernovae were discovered ch…

astro-ph2007★ 41 cited

GRB070610 : A Curious Galactic Transient

M. M. Kasliwal, S. B. Cenko, S. R. Kulkarni +23

GRB 070610 is a typical high-energy event with a duration of 5s.Yet within the burst localization we detect a highly unusual X-ray and optical transient, SwiftJ195509.6+261406. We…

astro-ph2007★ 68 cited

Evidence of Exponential Decay Emission in the Swift Gamma-ray Bursts

T. Sakamoto, J. E. Hill, R. Yamazaki +6

We present a systematic study of the steep decay emission from gamma-ray bursts (GRBs) observed by the Swift X-Ray Telescope (XRT). In contrast to the analysis described in recent…

astro-ph2007★ 14 cited

Periodicities in X-ray Binaries from Swift/BAT Observations

R. Corbet, C. Markwardt, L. Barbier +8

The Burst Alert Telescope (BAT) on board Swift has accumulated extensive light curves for 265 sources (not including GRBs) in the energy range 14 to 200 keV. We present here a summ…