Timing Analysis of the Isolated Neutron Star RXJ0720.4–3125 Silvia Zane, Frank Haberl, Mark Cropper, Vyacheslav Zavlin, David Lumb, Steve Sembay & Christian.
AGILE M. Tavani INAF, Roma, 15 dic. 2003. EGRET 30 MeV-30 GeV (1.8 tons) Spark chamber TOF Calorimeter (NaI)
XMM EPIC MOS Steve Sembay ([email protected]) EPIC Calibration Meeting Tuebingen 03/02/03-06/02/03 MOS Cooling Results and Current Response Both MOS Cameras.
Chapter 10 – part 3 - Neutron stars and Black Holes Neutron stars.
The Multiwavelength Approach to Unidentified Gamma-Ray Sources MOTIVATION: Gamma-ray sources should be multiwavelength objects. X-RAYS:Counterpart searches.
The Magnetic Field of an Isolated Neutron Star from X-ray Cyclotron Absorption Lines
Mass & Radius of Compact Objects F astest pulsar and its stellar EOS
Identification of high energy gamma-ray sources and source populations
XMM-Newton contribution
Chapter 13 Neutron Stars and Black Holes
