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20012024
most citedObservational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

88 citations · 257 across the 22 of their papers we have counts for

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13 papers · 1 filter

astro-ph2007★ 9 cited

SAXJ1712.6-3739: a persistent hard X-ray source as monitored with INTEGRAL

Mariateresa Fiocchi, Angela Bazzano, Pietro Ubertini +1

The X-ray source SAXJ1712.6-3739 is a very weak Low Mass X-ray Binary discovered in 1999 with BeppoSAX and located in the Galactic Center. This region has been deeply investigated…

astro-ph2007★ 1 cited

Long term monitoring of the BHC 1E 1740.7-2942

M. Del Santo, A. Bazzano, N. Bezayiff +4

The microquasar 1E 1740.7-2942 is one of the most appealing source of the Galactic Centre region. The high energy feature detected once by SIGMA has been searched in the last years…

astro-ph2007★ 8 cited

Cygnus X-3 transition from the ultrasoft to the hard state

V. Beckmann, S. Soldi, G. Belanger +8

Aims: The nature of Cygnus X-3 is still not understood well. This binary system might host a black hole or a neutron star. Recent observations by INTEGRAL have shown that Cygnus X-…

astro-ph2007★ 11 cited

INTEGRAL high energy monitoring of the X-ray burster KS 1741-293

G. De Cesare, A. Bazzano, S. Martinez Nunez +4

KS 1741-293, discovered in 1989 by the X-ray camera TTM in the Kvant module of the Mir space station and identified as an X-ray burster, has not been detected in the hard X band un…

astro-ph2006★ 10 cited

First broad band study of the mysterious source 1E 1743.1-2843

M. Del Santo, L. Sidoli, A. Bazzano +4

In the last years, the persistent source 1E 1743.1-2843 has been observed in the X-rays, but never above 20 keV. In previous works, it was stressed that a possible high energy emis…

astro-ph2005

INTEGRAL observation of the X-ray burster KS 1741-293

G. De Cesare, A. Bazzano, G. Stratta +3

KS 1741-293 was firstly detected in 1989 with the X-ray wide field camera TTM (3-10 keV) on board of the Rontgen-Kvant-Mir observatory. During these observations this source exhibi…