The SPI/INTEGRAL survey of the Galactic Plane
Abstract
We use SPI data obtained during the core program observation to present an analysis of the Galactic Plane source populations. We will discuss source properties. A Log N-Log S function is tentatively built with the goal of estimate the total source (ponctual) emission in Galactic Center emission.
- Publication:
-
35th COSPAR Scientific Assembly
- Pub Date:
- 2004
- Bibcode:
- 2004cosp...35.3909B