135 citations · 578 across the 18 of their papers we have counts for
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The dispersion in pulsar -ray efficiency
Daniel Íñiguez-Pascual, Daniele Viganò, Diego F. Torres
The observational efficiency of pulsars, defined as the ratio of the observationally derived isotropic-equivalent luminosity, , where is the average…
Magnetar Outburst Models with Cooling Simulations
D. De Grandis, N. Rea, K. Kovlakas +6
Magnetar outbursts are among the most noteworthy manifestations of magnetism in neutron stars. They are episodes in which the X-ray luminosity of a strongly magnetised neutron star…
Synchro-curvature description of γ-ray light curves and spectra of pulsars: concurrent fitting
Daniel Íñiguez-Pascual, Diego F. Torres, Daniele Viganò
We present a concurrent fitting of spectra and light curves of the whole population of detected gamma-ray pulsars. Using a synchro-curvature model we compare our theoretical output…
Synchro-curvature description of -ray light curves and spectra of pulsars: global properties
Daniel Íñiguez-Pascual, Diego F. Torres, Daniele Viganò
This work presents a methodological approach to generate realistic -ray light curves of pulsars, resembling reasonably well the observational ones observed by the Fermi-Large Ar…
3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves
Stefano Ascenzi, Daniele Viganò, Clara Dehman +3
The thermal evolution of isolated neutron stars is a key element in unraveling their internal structure and composition and establishing evolutionary connections among different ob…
A very young radio-loud magnetar
P. Esposito, N. Rea, A. Borghese +20
The magnetar Swift ,J1818.0-1607 was discovered in March 2020 when Swift detected a 9 ms hard X-ray burst and a long-lived outburst. Prompt X-ray observations revealed a spin perio…
The X-ray outburst of the Galactic Center magnetar over six years of Chandra observations
N. Rea, F. Coti Zelati, D. Vigano' +16
The magnetar SGR J1745-2900 discovered at parsecs distance from the Milky Way central black hole, Sagittarius A*, represents the closest pulsar to a supermassive black hole ever de…
Population Synthesis of Isolated Neutron Stars with magneto-rotational evolution II: from radio-pulsars to magnetars
M. Gullón, J. A. Pons, J. A. Miralles +3
Population synthesis studies constitute a powerful method to reconstruct the birth distribution of periods and magnetic fields of the pulsar population. When this method is applied…
The X-ray outburst of the Galactic Centre magnetar SGR J1745-2900 during the first 1.5 year
F. Coti Zelati, N. Rea, A. Papitto +17
In 2013 April a new magnetar, SGR 1745-2900, was discovered as it entered an outburst, at only 2.4 arcsec angular distance from the supermassive black hole at the Centre of the Mil…
Searching for small-scale diffuse emission around SGR 1806-20
D. Viganò, N. Rea, P. Esposito +6
Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20, after its 2004 powerful giant flare. We study the possible extended X-ray emission at small scal…