Flat-Fielding BATSE Occultation Data for use in a Hard X-Ray All Sky Survey
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.
Keywords
Cite
@article{arxiv.astro-ph/0101035,
title = {Flat-Fielding BATSE Occultation Data for use in a Hard X-Ray All Sky Survey},
author = {S. E. Shaw and A. J. Bird and A. J. Dean and N. Diallo and C. Ferguson and J. Knodlseder and J. J. Lockley and M. J. Westmore and D. R. Willis},
journal= {arXiv preprint arXiv:astro-ph/0101035},
year = {2007}
}
Comments
4 pages, 2 figures, for publication in Proceedings of the 4th Integral Workshop, Alicante, Spain. Replacement to add authors, problem with A4 paper in esapub.cls