14 July 2008 XPOL: a photoelectric polarimeter onboard XEUS
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The XEUS mission incorporates two satellites: the Mirror Spacecraft with 5 m2 of collecting area at 1 keV and 2 m2 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.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Enrico Costa, Enrico Costa, Ronaldo Bellazzini, Ronaldo Bellazzini, Jean Bregeon, Jean Bregeon, Alessandro Brez, Alessandro Brez, Massimo Frutti, Massimo Frutti, Sergio Di Cosimo, Sergio Di Cosimo, Luca Latronicio, Luca Latronicio, Francesco Lazzarotto, Francesco Lazzarotto, Giorgio Matt, Giorgio Matt, Massimo Minuti, Massimo Minuti, Ennio Morelli, Ennio Morelli, Fabio Muleri, Fabio Muleri, Michele Pinchera, Michele Pinchera, Massimiliano Razzano, Massimiliano Razzano, Alda Rubini, Alda Rubini, Paolo Soffitta, Paolo Soffitta, Gloria Spandre, Gloria Spandre, } "XPOL: a photoelectric polarimeter onboard XEUS", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 70110F (14 July 2008); doi: 10.1117/12.789545; https://doi.org/10.1117/12.789545

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