Improved COMPTEL maps of the milky way

Details Improved COMPTEL maps of the milky way Improved COMPTEL maps of the milky way

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..586b&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 586-590 (2000).

Computer Science

Databases

5

Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Characteristics And Properties Of The Milky Way Galaxy, Gamma-Ray, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

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. .

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