Improved COMPTEL maps of the milky way

Авторы: Bloemen H., Bennett K., Collmar W., Diehl R., Hermsen W., Iyudin A., Knödlseder J., McConnell M., Ryan J., Schönfelder V., Strong A.
Сборник: THE FIFTH COMPTON SYMPOSIUM
Серия: AIP Conference Proceedings
Том: 510
Год издания: 2000
Издательство: AIP Publishing
Местоположение издательства: United States
Первая страница: 586
Последняя страница: 590
DOI: 10.1063/1.1303270
Аннотация: 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.
Добавил в систему: Июдин Анатолий Федорович

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