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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

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