vertically averaged over the -60cm y 60cm interval (beam axis at y=0) ... Expected high energy hadron fluence in UJ56 (triplet electronics) is worrying ...
Title: PowerPoint Presentation Last modified by: Paolo Mereghetti Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Title: PowerPoint Presentation Last modified by: Paolo Mereghetti Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Title: PowerPoint Presentation Last modified by: Paolo Mereghetti Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Title: PowerPoint Presentation Last modified by: Paolo Mereghetti Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Title: PowerPoint Presentation Last modified by: Paolo Mereghetti Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
S.Mereghetti - Participation to SVOM ASI ... Swift UVOT is sensible only in the blue / UV) ... Thales Alenia Space Italia (ex Laben) Media Lario. BCV Progetti ...
Magnetars: SGRs and AXPs Magnetars in the Galaxy ~7 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv: 1010.4592)
Title: Neutron star masses: dwarfs, giants and neighbors Author: PKSternberg Last modified by: sternberg pk Created Date: 11/26/2005 8:18:07 AM Document presentation ...
Lecture 4. Magnetars: SGRs and AXPs Sergei Popov (SAI MSU) Magnetars on the Galaxy 5 SGRs, 10 AXPs, plus candidates, plus radio pulsars with high magnetic fields
Title: Close-by young isolated neutron stars (and black holes) Author: polar Last modified by: sergepolar Created Date: 4/1/2005 6:24:30 AM Document presentation format
Sgr A* 30th Fest -- 2004 March. 1. Interstellar Scattering of Sgr A* D. C. Backer ... An Early View on Scatter Broadening. Backer 1978 ApJ, 222, L9. b. zb/Z ...
typical rotation periods: 1.5 ms 5 s ... I O2 = 3 1052 P-2(ms) erg ... Anti Coincidence Shield (ACS) (512 kg, 91 BGO blocks) The ACS is also used as an ...
Yosi Gelfand, Greg Taylor, Chryssa Kouveliotou, David Eichler, Yoni Granot, Enrico Ramirez-Ruiz, ... Swift out to 70 Mpc, tail to 10 Mpc - 1% - 20% of short ...
Glitches; the Link Between the Typical Radio Pulsars and the Anomalous X-ray Pulsars ... Theoretical models for pulsar glitches; star quake and vortex creep ...
1997 Aug 12 discovery of a new transient, active only 1 day ! ... day at the beginning (starting on 4th February) - then exposure up to 10 ks / day during ...
spiskycnv no essential changes (formally part of OSIM. spiskymax added input/output source ... Need to convert the DE200 ephemeris file to the ISDC standard ...