Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.4305w&link_type=abstract
American Astronomical Society Meeting 210, #43.05; Bulletin of the American Astronomical Society, Vol. 39, p.157
Astronomy and Astrophysics
Astronomy
Scientific paper
Gamma-Ray line studies are one of the prime scientific goals of ESA's INTEGRAL mission. The INTEGRAL Spectrometer (SPI) is designed to detect and measure lines in the 20-8000 keV range with energy resolution of 2-8 keV. We made a comprehensive search for Gamma-ray lines using the first year (AO-1) of the SPI public data. We found no evidence for any previously unpredicted lines (Teegarden & Watanabe 2006). We continue the search with the second year (AO-2) of the public data as well as recently observed the AO-4 Key Program (KP) data. We will show our preliminary results and discuss our findings.
Teegarden Bonnard J.
Watanabe Ken
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