Characterization and prediction of the SPI background

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 552, 2004, Pages 819-822

  Teegarden, B J ^a   Jean, P ^b   Weidenspointner, G ^b   Knodlseder J ^b   Skinner, G K ^b   Von Ballmoos, P ^b   Shrader, C ^c   Sturner, S ^c   Watanabe, K ^d  

^a NASA HEADQUARTERS   (United States)

^b IRAP   (France)

^c GSFC   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC RAYS; DETECTORS; FLUXES; GAMMA RAYS; POSITRONS; SPACECRAFT; SPECTROMETERS; TELESCOPES;

COSMIC-RAY INTENSITY; ELECTRON-POSITRON ANNIHILATION RADIATION; INTEGRAL SPECTROMETER (SPI); SIGNAL-TO-BACKGROUND RATIO;

ASTRONOMY;

EID: 23844534062     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (9)

1. Jean, P. et al., A&A, 411, L107, 2003.
2. Jean, P. et al., these proceedings, 2004a.
3. Jean, P. et al., these proceedings, 2004b.
4. Knödlseder, J. et al., these proceedings, 2004.
5. Lonjou. V. et al., these proceedings, 2004.
6. Vedrenne, G. et al., A&A, 411, L63, 2003.
7. Weidenspointner, G. et al., A&A, 411, L113, 2003.
8. Weidenspointner, G. et al., New Astr. Reviews, 48, 227, 2004a.
9. Weidenspointner, G. et al., these proceedings, 2004b.