Masanori Ohno (ISAS/JAXA). HXD: 10-600 keV WAM: 50keV-5MeV XIS: 0.2-12keV X-ray Afterglow (XIS + HXD withToO) Wide energy band (0.2-600 keV) Ultra-low.
X-ray polarisation: Science Accretion powered pulsars / high magnetic field neutron stars: X-ray beaming pattern (fan/pencil) is not known and will.
Study on polarization of high- energy photons from the Crab pulsar 〇 J. Takata (TIARA-NTHU/ASIAA,Taiwan) H.-K. Chang (NTH Univ., Taiwan) K.S. Cheng (HK.
Field Trials of an RFI Adaptive Filter for Pulsar Observations M. Kesteven, R.N. Manchester, G. Hampson & A. Brown Australia Telescope National Facility.
Abstract The Gamma-ray Large Area Space Telescope (GLAST) will be launched less than a year from now, and its Large Area Telescope (LAT) is expected to.
Scuola nazionale de Astrofisica Radio Pulsars 2: Timing and ISM Outline Timing methods Glitches and timing noise Binary pulsar timing Post-Keplerian effects,
Abstract
RXTE Studies of Accreting X-ray Pulsars via Cyclotron Lines
