In the course of the mission we have gradually developed an analysis method that separates in an iterative manner the celestial emission and the (a priori unknown) instrumental background. It has become our standard analysis tool for point sources. We illustrate here that this method is widely applicable now. It provides mutually consistent sets of model-fitting parameters (spectra) and sky maps, both for continuum and line studies. Because of the wide applicability, it has been possible to make various cross-checks while building up confidence in this procedure.
AIP Conference Proceedings
Digital Object Identifier (DOI)
Improved COMPTEL maps of the milky way Bloemen, H. and Bennett, K. and Collmar, W. and Diehl, R. and Hermsen, W. and Iyudin, A. and Knödlseder, J. and McConnell, M. and Ryan, J. and Schönfelder, V. and Strong, A., AIP Conference Proceedings, 510, 586-590 (2000), DOI:http://dx.doi.org/10.1063/1.1303270
© 2000 American Institute of Physics