Share Email Print
cover

Proceedings Paper

A set of x-ray polarimeters for the New Hard X-ray Imaging and Polarimetric Mission
Author(s): Paolo Soffitta; Enrico Costa; Fabio Muleri; Riccardo Campana; Ettore Del Monte; Sergio Di Cosimo; Yuri Evangelista; Sergio Fabiani; Marco Feroci; Francesco Lazzarotto; Alda Rubini; Ronaldo Bellazzini; Alessandro Brez; Massimo Minuti; Nicola Omodei; Michele Pinchera; Massimiliano Razzano; Carmelo Sgrò; Gloria Spandre; Andrea Argan; Giorgio Matt
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The New Hard X-Ray Imaging and Polarimetric Mission makes a synergic use of Hard X-Ray Imaging, Spectroscopy and Polarimetry, as independent diagnostic of the same physical systems. It exploits the technology of multi-layer optics that, with a focal length of 10 m, allow for spectroscopic and imaging, with a resolution from 15 to 20 arcseconds, on the band 0.2 - 80 keV. One of the four telescopes is devoted to polarimetry. Since the band of a photoelectric polarimeter is not that wide, we foresee two of them, one tuned on the lower energy band (2-10 keV) and another one tuned on higher energies (6 - 35 keV). The blurring due to the inclined penetration of photons in the gas , thanks to the long focal length is practically negligible. In practice the polarimeters fully exploit the resolution the telescope and NHXM can perform angular resolved simultaneous spectroscopy and polarimetry on the band 2 - 35 keV. We are also studying the possibility to extend the band up to 80 keV by means of a focal plane scattering polarimeter.

Paper Details

Date Published: 29 July 2010
PDF: 13 pages
Proc. SPIE 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 77321A (29 July 2010); doi: 10.1117/12.856434
Show Author Affiliations
Paolo Soffitta, INAF - IASF Roma (Italy)
Enrico Costa, INAF - IASF Roma (Italy)
Fabio Muleri, INAF - IASF Roma (Italy)
Riccardo Campana, INAF - IASF Roma (Italy)
Ettore Del Monte, INAF - IASF Roma (Italy)
Sergio Di Cosimo, INAF - IASF Roma (Italy)
Yuri Evangelista, INAF - IASF Roma (Italy)
Sergio Fabiani, INAF - IASF Roma (Italy)
Marco Feroci, INAF - IASF Roma (Italy)
Francesco Lazzarotto, INAF - IASF Roma (Italy)
Alda Rubini, INAF - IASF Roma (Italy)
Ronaldo Bellazzini, Istituto Nazionale di Fisica Nucleare (Italy)
Alessandro Brez, Istituto Nazionale di Fisica Nucleare (Italy)
Massimo Minuti, Istituto Nazionale di Fisica Nucleare (Italy)
Nicola Omodei, Istituto Nazionale di Fisica Nucleare (Italy)
Michele Pinchera, Istituto Nazionale di Fisica Nucleare (Italy)
Massimiliano Razzano, Istituto Nazionale di Fisica Nucleare (Italy)
Carmelo Sgrò, Istituto Nazionale di Fisica Nucleare (Italy)
Gloria Spandre, Istituto Nazionale di Fisica Nucleare (Italy)
Andrea Argan, Istituto Nazionale di Astrofisica (Italy)
Giorgio Matt, Univ. degli Studi di Roma Tre (Italy)


Published in SPIE Proceedings Vol. 7732:
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
Monique Arnaud; Stephen S. Murray; Tadayuki Takahashi, Editor(s)

© SPIE. Terms of Use
Back to Top