X-ray Polarimetry - INAF-IASF-Roma
X-ray Polarimetry - INAF-IASF-Roma
X-ray Polarimetry - INAF-IASF-Roma
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Implementation of X-<strong>ray</strong> polarimetry with GPD in proposed missions:<br />
- POLARIX<br />
(ASI small mission, fasa A completed)<br />
3 Jet-X optics (3,5 m FL, 20 ‘’ HED 500 cm 2 @ 2 keV, HEW=(20’’))<br />
3 GPD (1-cm, 1-Atm, He-DME 20-80)<br />
MDP 12 % in 10 5 s for 1 mCrab source (2-10 keV)<br />
3.8 % in 10 5 s for 10 mCrab source (2-10 keV)<br />
- NHXM<br />
(Proposed ESA M3 Mission not selected)<br />
1 of 4 Multi-layer optics (Pt-C) (10 m FL)<br />
2 GPD : 1-cm, 1-Atm, He-DME (LEP) (2-10 keV);<br />
3-cm 3-Atm Ar-DME (MEP) (6-35 keV)<br />
MDP:<br />
LEP 9.7 % in 10 5 s for 1 mCrab source (2-10 keV)<br />
3.1 % in 10 5 s for 10 mCrab source (2-10 keV)<br />
Costa, et al., Exp Ast 2010<br />
MEP 13 % in 10 5 s for 1 mCrab source (6-35 keV)<br />
4.1 % in 10 5 for 10 mCrab source (6-35 keV)<br />
In study (HEP, Compton scattering)<br />
MDP 7.2 % for 10 mCrab in 10 5 s (20-80 keV)<br />
Tagliaferri et al.i, Exp Ast 2010;<br />
- IXO<br />
Soffitta et al. SPIE 2010<br />
(ESA/NASA/JAXA Large Mission Evolved in Athena with no polarimeter on-board)<br />
Area= 2.5 m 2 FL = 20 m HEW= 5’’ XPOL: MDP 1 % 1 mCrab 10 5 s.<br />
Paolo Soffitta The Extreme and Variable High Energy Sky Chia Laguna 19-21/09/2011