Estimate for GLAST LAT milky way Dark Matter WIMP line sensitivity

AIP Conference Proceedings

Volumn 921, Issue , 2007, Pages 514-515

  Edmonds, Y ^a,b   Baltz, E ^a,b   Bloom, E ^a,b   Cohen Tanugi, J ^a,b   Godfrey, G ^a,b   Wai, L ^a,b   Wang, P ^a,b   Scargle, J ^c   Conrad, J ^d  

^a SLAC NATIONAL ACCELERATOR LABORATORY   (United States)

^b STANFORD UNIVERSITY   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d ALBANOVA UNIVERSITY CENTER   (Sweden)

Author keywords

Dark Matter; Gamma rays; GLAST; WIMP

Indexed keywords

EID: 78649795215     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.2757428     Document Type: Conference Paper

References (4)

1. Galprop, http://galprop.stanford.edu/web-galprop/galprop-home.html
2. Stoehr et al., Mon. Not. R. Astron. Soc. 345, 1313-1322(2003)
3. ObsSim, http://glast-ground.slac.stanford.edu/workbook/pages/sciTools- observationSimTutorial/obsSimTutorial.htm.
4. DC-2, http://glast-ground.slac.stanford.edu/workbook/dc2-home.htm IRFs version 3 see http://www-glast.slac.stanford.edu/software/IS/glast-lat- performance.htm as of February 2007.