Calibration for the X-ray Polarimetry Mission GEMS

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The Gravity and Extreme Magnetism SMEX (GEMS) mission was selected by NASA for flight in 2014. GEMS will make the first sensitive survey of X-ray polarization across a wide set of source classes including stellar black holes, Seyfert galaxies and quasars, blazars, rotation and accretion-powered pulsars, magnetars, shell supernova remnants and pulsar wind nebulae. GEMS employs grazing-incidence foil mirrors and novel time-projection chamber (TPC) polarimeters leveraging the photoelectric effect to image the charge tracks of photoelectrons produced by 2 - 10 keV X-rays. We present an overview of the methods that will be used for ground calibration of the TPC polarimeters and the development of polarized and unpolarized X-ray sources for this purpose.

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