Flat-Fielding BATSE Occultation Data for use in a Hard X-Ray All Sky Survey

S. E. Shaw; A. J. Bird; A. J. Dean; N. Diallo; C. Ferguson; J. Knodlseder; J. J. Lockley; M. J. Westmore; D. R. Willis

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arXiv · astro-ph/0101035

Flat-Fielding BATSE Occultation Data for use in a Hard X-Ray All Sky Survey

S. E. Shaw·A. J. Bird·A. J. Dean·N. Diallo·C. Ferguson·J. Knodlseder·J. J. Lockley·M. J. Westmore·D. R. Willis

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Abstract

The BATSE mission aboard CGRO can be used to observe hard X-ray sources by using the Earth occultation method. This method relies on measuring a step in the count rate profile in each BATSE detector as a source rises above or sets below the Earth's limb. A major problem in determining the step sizes (and hence the flux) is in extracting the steps from the varying background. A technique for flat-fielding the response of gamma ray detectors has been developed at Southampton. The technique uses a dynamic Monte-Carlo model to simulate the dominant components of the gamma-ray background encountered by the experiment at any point in its orbit. A maximum likelihood imaging method is also being developed that will be used to make a sky survey with all 9 years of the BATSE Continuous data set in the 20 - 500 keV range. An all sky map of 25 - 35 keV emission has been made using 60 days of data and has a 3 sigma flux sensitivity of 14 mCrab.

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BibTeX RIS

S. E. Shaw, A. J. Bird, A. J. Dean, N. Diallo, C. Ferguson, J. Knodlseder, J. J. Lockley, M. J. Westmore, D. R. Willis. 2001-01-03. Flat-Fielding BATSE Occultation Data for use in a Hard X-Ray All Sky Survey. https://arxiv.org/abs/astro-ph/0101035

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