activity
20032025
most citedMagnetars as persistent hard X-ray sources: INTEGRAL discovery of a hard tail in SGR 1900+14

131 citations · 570 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2025★ 6 cited

The infrared counterpart and proper motion of magnetar SGR0501+4516

A. A. Chrimes, A. J. Levan, J. D. Lyman +19

Soft gamma repeaters (SGRs) are highly magnetised neutron stars (magnetars) notable for their gamma-ray and X-ray outbursts. In this paper, we use near-infrared (NIR) imaging of SG…

astro-ph2009★ 41 cited

The updated spectral catalogue of INTEGRAL Gamma-Ray Bursts

G. Vianello, D. Götz, S. Mereghetti

We present a catalogue with the properties of all the bursts detected and localized by the IBIS instrument onboard the INTEGRAL satellite from November 2002 to September 2008. The…

astro-ph2007★ 44 cited

SGR 1806-20 about two years after the giant flare: Suzaku, XMM-Newton and INTEGRAL observations

P. Esposito, S. Mereghetti, A. Tiengo +9

In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever observed. This probably involved a large-scale rearrangement of the magnetosphe…

astro-ph2007★ 121 cited

An alternative hypothesis for the outburst mechanism in Supergiant Fast X-ray Transients: the case of IGR J11215-5952

L. Sidoli, P. Romano, S. Mereghetti +4

(ABRIDGED)- The physical mechanism responsible for the short outbursts in a recently recognized class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients (SFXTs), is…

astro-ph2007★ 4 cited

Long term spectral variability in the soft gamma ray repeater SGR 1900+14

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

We present a systematic analysis of all the BeppoSAX data of SGR 1900+14. The observations spanning five years show that the source was brighter than usual on two occasions: ~20 da…

astro-ph2006★ 28 cited

A new symbiotic low mass X-ray binary system: 4U 1954+319

F. Mattana, D. Gotz, M. Falanga +4

4U 1954+319 was discovered 25 years ago, but only recently has a clear picture of its nature begun to emerge. We present for the first time a broad-band spectrum of the source and…