352 citations · 2.8k across the 65 of their papers we have counts for
7 papers · 2 filters
The 3rd IBIS/ISGRI soft gamma-ray survey catalog
A. J. Bird, A. Malizia, A. Bazzano +20
In this paper we report on the third soft gamma-ray source catalog obtained with the IBIS/ISGRI gamma-ray imager on board the INTEGRAL satellite. The scientific dataset is based on…
INTEGRAL and Swift observations of the supergiant fast X-ray transient AXJ1845.0-0433=IGRJ18450-0435
V. Sguera, A. J. Bird, A. J. Dean +8
Context: AXJ1845.0-0433 was discovered by ASCA in 1993 during fast outburst activity characterized by several flares on short timescales. Up to now, the source was not detected aga…
SWIFT/XRT follow-up observations of INTEGRAL AGNs
R. Landi, A. Malizia, L. Bassani +9
In five years of operation, data from INTEGRAL has been used to discover a large number of gamma-ray sources, a substantial fraction of which have turned out to be active galactic…
20-100 keV properties of cataclysmic variables detected in the INTEGRAL/IBIS survey
E. J. Barlow, C. Knigge, A. J. Bird +5
Analysis of INTEGRAL/IBIS survey observations has revealed that the rare intermediate polar and asynchronous polar cataclysmic variables are consistently found to emit in the 20-10…
Swift/XRT follow-up observations of TeV sources of the HESS Inner Galaxy survey
R. Landi, L. Bassani, A. Malizia +6
In order to provide a firm identification of the newly discovered Galactic TeV sources, a search for counterparts in a broad band from soft X-ray to soft gamma-rays is crucial as d…
INTEGRAL observations of AGN obscured by the Galactic Plane
M. Molina, A. Malizia, L. Bassani +9
In this paper we present INTEGRAL observations of 7 AGNs: two newly discovered type 1 Seyferts, IGR J18027-1455 and IGR J21247+5058, and five well known Seyferts, NGC 6814 (type 1.…
Spectral states of the X-ray binary IGR J17091--3624 observed by INTEGRAL and RXTE
F. Capitanio, A. Bazzano, P. Ubertini +6
IGR J17091-3624 was discovered in 2003 April by INTEGRAL/IBIS during its Galactic Centre Deep Exposure programme. The source was initially detectable only in the 40--100 keV range,…