2008/07/12 by Enrico Costa, Ronaldo Bellazzini, Jean Bregeon +14 · 1 citation
Engineering · Physics and Astronomy · #Advanced Semiconductor Detectors and Materials #CCD and CMOS Imaging Sensors #Photocathodes and Microchannel Plates #astro-ph
paper · pdf · doi:10.1117/12.789545
published as Proceedings of SPIE Astronomical Instrumentation 2008 Conference, 23-28 June 2008 Marseille, France, vol. 7011-15 · 10 pages, 6 figures
openalex publication_date 2008/07/12 · arxiv created 2008/10/15 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30
The XEUS mission incorporates two satellites: the Mirror Spacecraft with 5 m<sup>2</sup> of collecting area at 1 keV and 2 m<sup>2</sup> at 7 keV, and an imaging resolution of 5" HEW and the Payload Spacecraft which carries the focal plane instrumentation. XEUS was submitted to ESA Cosmic Vision and was selected for an advanced study as a large mission. The baseline design includes XPOL, a polarimeter based on the photoelectric effect, that takes advantage of the large effective area which permits the study of the faint sources and of the long focal length, resulting in a very good spatial resolution, which allows the study of spatial features in extended sources. We show how, with XEUS, Polarimetry becomes an efficient tool at disposition of the Astronomical community.