activity
20032007
most citedTiming an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

50 citations · 427 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph2007★ 8 cited

Spectral analysis of LMC X-2 with XMM/Newton: unveiling the emission process in the extragalactic Z-source

G. Lavagetto, R. Iaria, A. D'Ai' +2

We present the results of the analysis of an archival observation of LMC X-2 performed with XMM/Newton. The spectra taken by high-precision instruments have never been analyzed bef…

astro-ph2007★ 45 cited

Spin up and phase fluctuations in the timing of the accreting millisecond pulsar XTE J1807-294

A. Riggio, T. Di Salvo, L. Burderi +4

We performed a timing analysis of the 2003 outburst of the accreting X-ray millisecond pulsar XTE J1807-294 observed by RXTE. Using recently refined orbital parameters we report fo…

astro-ph2007

A complex environment around Cir X-1

A. D'Ai, R. Iaria, T. Di Salvo +2

We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X--1 during the phase passage 0.223-0.261. A comparative analysis of X-ray spectra,…

astro-ph2007★ 10 cited

Precise determination of orbital parameters in system with slowly drifting phases: application to the case of XTE J1807-294

A. Riggio, T. Di Salvo, L. Burderi +4

We describe a timing technique that allows to obtain precise orbital parameters of an accreting millisecond pulsar in those cases in which intrinsic variations of the phase delays…

astro-ph2007★ 49 cited

Broad-band Spectral Evolution of Scorpius X-1 along its Color-Color Diagram

A. D'Aí, P. Zycki, T. Di Salvo +3

We analyze a large collection of RXTE archive data from April 1997 to August 2003 of the bright X-ray source Scorpius X-1 in order to study the broadband spectral evolution of the…

astro-ph2007★ 27 cited

Chandra Observation of the Big Dipper X 1624-490

R. Iaria, G. Lavagetto, A. D'Ai' +2

We present the results of a 73 ks long Chandra observation of the dipping source X 1624-490. During the observation a complex dip lasting 4 hours is observed. We analyse the persis…