S. Piraino
INAF
9 Papers
13 Citations
S. Piraino is an academic researcher from INAF. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 5, co-authored 9 publications.
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Papers
Testing reflection features in 4U 1705−44 with XMM-Newton, BeppoSAX, and RXTE in the hard and soft states
Elise Egron,T. Di Salvo,Sara Motta,Luciano Burderi,Alessandro Papitto,Refiz Duro,Antonino D'Ai,Alessandro Riggio,Alessandro Riggio,T. M. Belloni,R. Iaria,N. R. Robba,S. Piraino,Andrea Santangelo +13 more
TL;DR: In this article, the spectral decomposition of a bright atoll source 4U 1705−44 has been studied in a broad-band (0.1−200 keV) energy range, with good energy resolution, using self-consistent reflection models.
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A relativistic iron emission line from the neutron star low-mass X-ray binary GX 3+1
S. Piraino,Andrea Santangelo,P. Kaaret,B. Mück,Antonino D'Ai,T. Di Salvo,R. Iaria,N. R. Robba,Luciano Burderi,Elise Egron +9 more
TL;DR: In this paper, the authors present the results of a spectroscopic study of the Fe-Kα emission of the persistent neutron-star atoll low-mass X-ray binary and type ǫ 3+1 with the EPIC-PN on board XMM-Newton.
BeppoSAX observations of XTE J1946+274
TL;DR: In this paper, the authors report on the Beppo SAX monitoring of a giant outburst of the transient X-ray pulsar XTE J1946+274 in 1998.
The reflection component in NS LMXBs
Antonino D'Ai,Alessandro Papitto,T. Di Salvo,R. Iaria,N. R. Robba,E. Egron,S. Piraino +6 more
- 01 Jan 2014
TL;DR: In this article, a comparative analysis of the reflection component from a series of spectroscopic studies on selected sources: 4U 1705-44, observed both in the soft and hard state, the pulsating ms pulsars SAX J1808.4- 3658 and IGR J17511-3057, and the intermittent pulsar HETE J1900-2455.
A relativistic iron emission line from the neutron star low-mass X-ray binary GX 3+1
S. Piraino,Andrea Santangelo,P. Kaaret,B. Mück,Antonino D'Ai,T. Di Salvo,R. Iaria,N. R. Robba,Luciano Burderi,Elise Egron +9 more
TL;DR: In this article, the authors present the results of a spectroscopic study of the Fe K-alpha emission of the persistent neutron-star atoll low-mass X-ray binary with the EPIC-PN on board XMM-Newton.