activity
19962009
most citedAn alternative hypothesis for the outburst mechanism in Supergiant Fast X-ray Transients: the case of IGR J11215-5952

121 citations · 723 across the 29 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph2006

INTEGRAL observations of the X-ray burster 4U1850-087: first detection of hard X-ray emission extending above 50keV

Lara Sidoli, Ada Paizis, Angela Bazzano +1

The X-ray burster 4U1850-087, located in the globular cluster NGC6712, is an ultracompact binary likely harbouring a degenerate companion.The source has been observed with INTEGRAL…

astro-ph20061 cited

INTEGRAL observations of IGRJ11215-5952: the first Supergiant Fast X-ray Transient displaying periodic outbursts

Lara Sidoli, Ada Paizis, Sandro Mereghetti

The hard X-ray source IGRJ11215-5952, discovered with INTEGRAL during a brief outburst in 2005, has been proposed as a new member of the class of Supergiant Fast X-ray Transients.…

astro-ph200611 cited

The ultra-compact binary 4U1850-087 observed with INTEGRAL: hard X-ray emission from an X-ray burster

L. Sidoli, A. Paizis, A. Bazzano +1

The X-ray burster 4U1850-087, located in the Galactic globular cluster NGC6712, is an ultracompact binary (orbital period~21 min),likely harbouring a degenerate companion.The sourc…

astro-ph200624 cited

Five years of SGR 1900+14 observations with BeppoSAX

P. Esposito, S. Mereghetti, A. Tiengo +3

We present a systematic analysis of all the BeppoSAX data of the soft gamma-ray repeater SGR 1900+14: these observations allowed us to study the long term properties of the source…

astro-ph200610 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-ph200613 cited

Unveiling the nature of the highly absorbed X-ray source SAXJ1748.2-2808 with XMM-Newton

L. Sidoli, S. Mereghetti, F. Favata +2

We report on the results of an EPIC XMM-Newton observation of the faint source SAXJ1748.2-2808 and the surrounding field. This source was discovered during the BeppoSAX Galactic ce…