7/26/12W. Majid1 Crab Giant Pulses W. Majid *, S. Ellingson (PI), C. Garcia-Miro, T. Kuiper, J. Lazio, S. Lowe, C. Naudet, D. Thompson, K. Wagstaff * Jet.
Software Correlation at JIVE & Real-time e-VLBI in the EVN Operations and PI Interaction Astronomy Gains from SFXC Real-time e-EVN status Proposal.
Status of LCLS A. Brachmann, SLAC National Accelerator Laboratory.
RXJ0146.9 +6121 a soft X-ray excess in a low luminosity accreting pulsar La Palombara & Mereghetti astro-ph/0604193.
Scuola nazionale de Astrofisica Radio Pulsars 3: Searches and Population Studies Outline Methods and early searches Globular Cluster searches Parkes Multibeam.
1. Introduction Her X-1 is an eclipsing binary system, with a neutron star (NS) primary and an A/F secondary star. The spin period is ~1.24 s and the orbital.
Anti-glitch induced by collision of a solid body with the magnetar 1E 2259+586
Aristeidis Noutsos University of Manchester. Pulsar Polarization Pulsar radiation is elliptically polarised with a high degree of linear polarization.
Pulsar Data Analysis Team Lyne
(a) The magneto quantum oscillation shows unprecedented detail, analyzed in (b).
1. Introduction
Scuola nazionale de Astrofisica Radio Pulsars 3: Searches and Population Studies