308 citations · 5.2k across the 160 of their papers we have counts for
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Be/X-ray binary SXP6.85 undergoes large Type II outburst in the Small Magellanic Cloud
L. J. Townsend, M. J. Coe, V. A. McBride +6
The Small Magellanic Cloud (SMC) Be/X-ray binary pulsar SXP6.85 = XTE J0103-728 underwent a large Type II outburst beginning on 2008 August 10. The source was consistently seen for…
Swift/XRT observations of unidentified INTEGRAL/IBIS sources
R. Landi, L. Bassani, A. Malizia +4
The 4th IBIS/ISGRI survey lists 723 hard X-ray sources many still unidentified. We cross-correlated the list of the sources included in the 4th IBIS catalogue with the Swift/XRT da…
The Fermi/LAT sky as seen by INTEGRAL/IBIS
P. Ubertini, V. Sguera, J. B. Stephen +3
In this letter we present the result of the cross correlation between the 4th INTEGRAL/IBIS soft gamma-ray catalog, in the range 20-100 keV, and the Fermi LAT bright source list of…
The 4th IBIS/ISGRI soft gamma-ray survey catalog
A. J. Bird, A. Bazzano, L. Bassani +19
In this paper we report on the fourth soft gamma-ray source catalog obtained with the IBIS gamma-ray imager on board the INTEGRAL satellite. The scientific dataset is based on more…
Discovery of the orbital period in the supergiant fast X-ray transient IGR J17544-2619
D. J. Clark, A. B. Hill, A. J. Bird +3
The supergiant fast X-ray transient (SFXT) system IGR J17544-2619 has displayed many large outbursts in the past and is considered an archetypal example of SFXTs. A search of the I…
The fraction of Compton-thick sources in an INTEGRAL complete AGN sample
A. Malizia, J. B. Stephen, L. Bassani +3
We study the NH distribution in a complete sample of 88 AGN selected in the 20-40 keV band from INTEGRAL/IBIS observations. We find that the fraction of absorbed (NH > 10^{22} cm^2…
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL
V. Sguera, G. E. Romero, A. Bazzano +3
3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is…