First Maps of the Soft X-Ray Diffuse Background from the ROSAT XRT/PSPC All-Sky Survey
Citations Over TimeTop 10% of 1995 papers
Abstract
This paper presents an initial version of the diffuse background results from the ROSA T soft X-ray all-sky survey. These maps cover ∼98% of the sky in the ¼ keV, ¾ keV, and 1.5 keV bands, with ∼2° angular resolution and high sensitivity for low surface brightness extended features. The effects of non-X-ray contamination and X-rays of solar system origin have been eliminated to the greatest possible extent, but discrete X-ray sources have not been removed. The much improved angular resolution, statistical precision, and completeness of coverage of these maps reveal considerable structure over the entire 0.1-2.0 keV energy range that was not observed previously. The data agree well with previous all-sky surveys in terms of absolute normalization and zero point.
Related Papers
- → Creation of 2-5 keV and 5-10 keV sky maps using XMM-Newton data(2014)2 cited
- → Candidate Isolated Neutron Stars and Other Optically Blank X-Ray Fields Identified from the ROSAT All-Sky and Sloan Digital Sky Surveys(2005)1 cited
- → Creation of 2-5 keV and 5-10 keV sky maps using XMM-Newton data(2014)
- A Large, Uniform Sample of X-ray Emitting AGN: the First 10 2.5 IDs from the ROSAT All Sky and Sloan Digital Sky Surveys(2000)