activity
19952005
most citedThe 1 - 50 keV spectral and timing analysis of IGR J18027-2016: an eclipsing, high mass X-ray binary

53 citations · 56 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph200553 cited

The 1 - 50 keV spectral and timing analysis of IGR J18027-2016: an eclipsing, high mass X-ray binary

A. B. Hill, R. Walter, C. Knigge +9

We report the association of the INTEGRAL source IGR J18027-2016 with the BeppoSAX source SAX J1802.7-2017. IGR J18027-2016 is seen to be a weak, persistent source by the IBIS/ISGR…

astro-ph2004

INTEGRAL monitoring of the Black Hole candidate 1E 1740.7-2942

M. Del Santo, A. Bazzano, D. M. Smith +24

The brightest persistent Galactic black hole candidate close to the Galactic Centre, 1E 1740.7-2942, has long been observed with INTEGRAL. In this paper, we report on the long-term…

astro-ph20043 cited

From BeppoSAX to INTEGRAL: PDS observations of hard X-ray sources detected in the IBIS survey

A. Malizia, L. Bassani, R. Landi +16

The first IBIS galactic plane survey has provided a list of high energy emitting objects above 20 keV; these sources have been detected mostly in the crowded region of the Galactic…

astro-ph2004

The sky behind our galaxy as seen by IBIS on INTEGRAL

L. Bassani, A. Malizia, J. B. Stephen +16

During the Core Programme, INTEGRAL has surveyed a large portion of the sky (around 9000 square degrees); although INTEGRAL is not optimized for extra-galactic studies its observat…

astro-ph2000

BeppoSAX discovery of a new Seyfert 2 galaxy: 1SAXJ2234.8-2541

A. Malizia, L. Bassani, I. Negueruela

In the present work we report the BeppoSAX serendipitous discovery of the type 2 AGN 1SAXJ2234.8-2541 in the MECS field of view when pointing at the Seyfert 2 galaxy NGC7314. The s…

astro-ph1995

A study of the core of the Shapley Concentration: II. ROSAT observation of A3558

S. Bardelli, E. Zucca, A. Malizia +3

We present the results of a pointed ROSAT PSPC observation of the cluster A3558 which is part of the core of the Shapley Concentration. The X-ray brightness distribution can be fit…