activity
20032013
most citedINTEGRAL observations of the cosmic X-ray background in the 5-100 keV range via occultation by the Earth

196 citations · 646 across the 26 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2013

Soft X-ray follow-up of five hard X-ray emitters

L. Pavan, E. Bozzo, C. Ferrigno +5

We studied the soft-X-ray emission of five hard-X sources: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703 and IGR J17348-2045. These sources are: a confirmed s…

astro-ph.HE2013

Accreting millisecond X-ray pulsars: 10 years of INTEGRAL observations

M. Falanga, L. Kuiper, J. Poutanen +5

During the last 10 years, INTEGRAL made a unique contribution to the study of accreting millisecond X-ray pulsars (AMXPs), discovering three of the 14 sources now known of this cla…

astro-ph.HE201233 cited

Spectral and timing properties of the accreting X-ray millisecond pulsar IGR J17498-2921

M. Falanga, L. Kuiper, J. Poutanen +5

We analyze the spectral and timing properties of IGR J17498-2921 and the characteristics of X-ray bursts to constrain the physical processes responsible for the X-ray production in…

astro-ph.HE2011

XMM-Newton observations of the supergiant fast X-ray transients XTEJ1739-302, IGRJ08408-4503 and IGRJ18410-0535

E. Bozzo, C. Ferrigno, J. C. Leyder +5

We report here on the XMM-Newton observations of the three supergiant fast X-ray transients (SFXT) XTE J1739-302, IGRJ08408-4503, and IGRJ18410-0535. For the latter source we only…

astro-ph.HE20092 cited

The emerging population of pulsar wind nebulae in hard X-rays

Fabio Mattana, Diego Götz, Régis Terrier +2

The hard X-ray synchrotron emission from pulsar wind nebulae (PWNe) probes energetic particles, closely related to the pulsar injection power at the present time. INTEGRAL has disc…

astro-ph.HE20094 cited

The first X-ray eclipse of IGRJ16479-4514?

E. Bozzo, L. Stella, G. Israel +2

We report on the first long (~32 ks) pointed XMM-Newton observation of the supergiant fast X-ray transient IGRJ16479-4514. Results from the timing, spectral and spatial analysis of…