2 citations · 7 across the 8 of their papers we have counts for
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The Vela pulsar proper motion revisited with HST astrometry
A. De Luca, R. P. Mignani, P. A. Caraveo
Using all the HST WFC/WFPC2 images of the field collected so far, we have performed an accurate relative astrometry analysis to re-assess the value of the Vela pulsar proper motion…
Search for the optical counterpart of the 16ms X-ray pulsar in the LMC
R. P. Mignani, L. Pulone, G. Marconi +2
The 16ms X-ray pulsar PSR J0537-6910 in SNR N157B is the fastest known isolated (non-recycled) pulsar and, with a rotational energy loss dE/dt ~ 4.8 10^38 erg/s, is the most energe…
An Atmospheric Model for the Ion Cyclotron Line of Geminga
A. Jacchia, F. De Luca, E. Lazzaro +3
Recent optical/UV data of Geminga (Mignani et al. 1998) have strengthen the significance of the emission feature present over the thermal continuum best fitting the EUV/soft X-ray…
The AGILE gamma-ray detector
A. Morselli, A. Perrino, P. Picozza +6
The gamma-ray detector AGILE, operating in the energy range from 30 MeV to 50 GeV, is composed by a tracking part, a light calorimeter and an anticoincidence system. Here we descri…
A New HST Measurement of the Crab Pulsar Proper Motion
Patrizia A. Caraveo, Roberto P. Mignani
We have used a set of archived HST/WFPC2 exposures of the inner regions of the Crab Nebula to obtain a new measurement of the pulsar proper motion, the first after the original wor…