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20002026
most citedBAT AGN Spectroscopic Survey - V. X-ray properties of the Swift/BAT 70-month AGN catalog

555 citations · 2.5k across the 30 of their papers we have counts for

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astro-ph2008★ 37 cited

An X-ray and optical study of the ultracompact X-ray binary A1246-58

J. J. M. in 't Zand, C. G. Bassa, P. G. Jonker +4

Results are discussed of an X-ray and optical observation campaign of the low-mass X-ray binary A1246-58 performed with instruments on Satellite per Astronomia X ('BeppoSAX'), the…

astro-ph2007★ 64 cited

A Comparison of the Variability of the Symbiotic X-ray Binaries GX 1+4, 4U 1954+31, and 4U 1700+24 from Swift/BAT and RXTE/ASM Observations

R. H. D. Corbet, J. L. Sokoloski, K. Mukai +2

We present an analysis of the X-ray variability of three symbiotic X-ray binaries, GX 1+4, 4U 1700+24, and 4U 1954+31, using observations made with the Swift Burst Alert Telescope…

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★ 200 cited

The long-term evolution of the spin, pulse shape, and orbit of the accretion-powered millisecond pulsar SAX J1808.4-3658

Jacob M. Hartman, Alessandro Patruno, Deepto Chakrabarty +6

We present a 7 yr timing study of the 2.5 ms X-ray pulsar SAX J1808.4-3658, an X-ray transient with a recurrence time of ~2 yr, using data from the Rossi X-ray Timing Explorer cove…

astro-ph2007★ 87 cited

The INTEGRAL Galactic bulge monitoring program: the first 1.5 years

E. Kuulkers, S. E. Shaw, A. Paizis +13

The Galactic bulge region is a rich host of variable high-energy point sources. Since 2005, February 17 we are monitoring the source activity in this region about every three days…

astro-ph2006★ 53 cited

Extreme Properties Of GRB061007: A Highly Energetic OR Highly Collimated Burst?

P. Schady, M. De Pasquale, J. Cummings +20

%auto-ignore This paper has been withdrawn by the authors due to dublicate submission. To download the paper please go to astro-ph/0611081