activity
19962009
most citedThe strongest cosmic magnets: Soft Gamma-ray Repeaters and Anomalous X-ray Pulsars

676 citations · 2.5k across the 63 of their papers we have counts for

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Showing 2004 · astro-phShow all

17 papers · 2 filters

astro-ph2004

On the polar caps of the 3 Musketeers

A. De Luca, P. A. Caraveo, S. Mereghetti +2

XMM-Newton observations of PSR B0656+14, PSR B1055-52 and Geminga have substantially increased the statistics available for these three isolated neutron stars, so apparently simila…

astro-ph20045 cited

GRB 040403: a faint X-ray rich Gamma-ray Burst discovered by INTEGRAL

S. Mereghetti, D. Gotz, M. I. Andersen +13

GRB 040403 is one of the faintest gamma-ray bursts for which a rapid and accurate localization has been obtained. Here we report on the gamma-ray properties of this burst, based on…

astro-ph2004

The soft X-ray counterpart of the newly discovered INTEGRAL source IGRJ16195-4945

L. Sidoli, S. Vercellone, S. Mereghetti +1

The INTEGRAL satellite, during its regular scanning observations of the Galactic plane, has discovered several new X-ray sources emitting above 20 keV. The nature of the great majo…

astro-ph200423 cited

INTEGRAL observations of the PSR B1259-63 / SS2883 system after the 2004 periastron passage

S. E. Shaw, M. Chernyakova, J. Rodriguez +3

The millisecond pulsar PSR B1259-63 and the Be star SS2883 are situated in a highly eccentric binary system, with orbital period ~3.4 years. We report on hard X-ray observations ob…

astro-ph2004

Phase-resolved spectroscopy of Geminga shows rotating hot spot(s)

P. A. Caraveo, A. De Luca, S. Mereghetti +2

Isolated neutron stars are seen in x-rays through their nonthermal and/or surface thermal emissions. XMM-Newton observations of the Geminga pulsar show a 43 electron volt spectrum…

astro-ph2004

A first XMM-Newton look at the relativistic double pulsar PSR J0737-3039

A. Pellizzoni, A. De Luca, S. Mereghetti +5

We present the results of a 50 ks long X-ray observation of the relativistic double pulsar system PSR J0737-3039 obtained with the XMM-Newton satellite in March 2004. The source ha…