Fermi/GBM monitoring of Accreting pulsars

Details Fermi/GBM monitoring of Accreting pulsars Fermi/GBM monitoring of Accreting pulsars

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confe..22f&link_type=abstract

"The First Year of MAXI: Monitoring Variable X-ray Sources", 4th International MAXI Workshop held November 30 - December 2, 2010

Physics

Scientific paper

Since the Launch of Fermi we have been using the twelve NaI detectors of
the Gamma-ray Burst Monitor (GBM) to monitor the pulsations of bright
accreting pulsars in the 8-50 keV energy band. I will discuss our
measurement techniques, the science problems we are interested in
addressing, and some recent results.

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