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Fermi GBM Science. Valerie Connaughton of the ... - Fermi - NASA

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Earth Occultation Step Fitting<br />

• Predict occultation times<br />

• Determine detectors viewing<br />

source <strong>of</strong> interest<br />

• Fit to each detector and energy<br />

channel<br />

– Background model<br />

– Model count rates for each<br />

source<br />

• Detector responses<br />

• Assumed energy spectrum<br />

• Atmospheric transmission<br />

• Compute best scale factor for<br />

all detectors to estimate fluxes.<br />

COSPAR Workshop Bangalore 2010 <strong>Valerie</strong> <strong>Connaughton</strong><br />

Monday, February 8, 2010 DOY 39

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