activity
20042009
most citedSpin-down rate and inferred dipole magnetic field of the soft gamma-ray repeater SGR 1627-41

32 citations · 103 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.HE200932 cited

Spin-down rate and inferred dipole magnetic field of the soft gamma-ray repeater SGR 1627-41

P. Esposito, M. Burgay, A. Possenti +11

Using Chandra data taken on 2008 June, we detected pulsations at 2.59439(4) s in the soft gamma-ray repeater SGR 1627-41. This is the second measurement of the source spin period a…

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-ph200713 cited

Discovery of X-ray emission from the young radio pulsar PSR J1357-6429

P. Esposito, A. Tiengo, A. De Luca +1

We present the first X-ray detection of the very young pulsar PSR J1357-6429 (characteristic age of 7.3 kyr) using data from the XMM-Newton and Chandra satellites. We find that the…

astro-ph200628 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…

astro-ph2006

DEMON: a Proposal for a Satellite-Borne Experiment to study Dark Matter and Dark Energy

Alicia Berciano Alba, Pedro Borges da Silva, Hans Eichelberger +12

We outline a novel satellite mission concept, DEMON, aimed at advancing our comprehension of both dark matter and dark energy, taking full advantage of two complementary methods: w…

astro-ph2005

On the complex X-ray structure tracing the motion of Geminga

A. De Luca, P. A. Caraveo, F. Mattana +2

A deep (100 ks) XMM-Newton observation of Geminga has shown two faint tails of diffuse X-ray emission, extending for ~2' behind the pulsar, well aligned with the proper motion (PM)…