Fermi/GBM monitoring of Accreting pulsars

Abstract:

For a given source we combine the rate residuals over detectors and obtain an estimate of the variable part of the source flux. Using a model of the source spectrum and the time dependent detector responses we compute the source induced rate expected in detector i at time tk if the source has unit flux in the channel’s energy range. The variable part of the flux is then estimate by minimizing

Año de publicación:

2010

Keywords:

Fuente:

google