Separating Local and Cosmic Soft X-ray Emission in the Chandra Deep Field-South

Computer Science – Databases

Scientific paper

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X-Ray Sources, X-Ray Bursts, Particle Emission, Solar Wind, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Astrometric And Interferometric Instruments

Scientific paper

The Chandra Deep Field-South (CDF-S) observing program, comprising 2 Ms of data collected near Solar Maximum (1999 and 2000) and during Solar Minimum (2007), provides a uniquely rich and informative data set for investigation of solar wind charge exchange (SWCX) and the soft X-ray background (SXRB). When combined with data on solar wind composition from the ACE satellite, these observations permit studies of the effects of solar wind stratification (fast versus slow wind) and viewing geometry (through the heliosphere and geocorona) on SWCX emission. We discuss preliminary results from our analysis of these data, including an upper limit on the true cosmic (non-SWCX) SXRB in the 3/4-keV band in the direction of the CDF-S.

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