A small satellite version of a soft x-ray polarimeter

Marshall HL, Heine S, Garner A, Gullikson E, Guenther M, Leitz C, Masterson R, Miller E, Zhang W, Boissay Malaquin R, Caiazzo I, Chakrabarty D, Davidson R, Gallo L, Heilmann RK, Heyl J, Kara E, Marscher A, Schulz N. 2020. A small satellite version of a soft x-ray polarimeter. Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. Astronomical Telescopes + Instrumentation vol. 11444, 114442Y.


Conference Paper | Published | English

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Author
Marshall, Herman L.; Heine, Sarah; Garner, Alan; Gullikson, Eric; Guenther, Moritz; Leitz, Christopher; Masterson, Rebecca; Miller, Eric; Zhang, William; Boissay Malaquin, Rozenn; Caiazzo, IlariaISTA ; Chakrabarty, Deepto
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Abstract
We describe a new implementation of a broad-band soft X-ray polarimeter, substantially based on a previous design. This implementation, the Pioneer Soft X-ray Polarimeter (PiSoX) is a SmallSat, designed for NASA’s call for Astrophysics Pioneers, small missions that could be CubeSats, balloon experiments, or SmallSats. As in REDSoX, the grating arrangement is designed optimally for the purpose of polarimetry with broad-band focussing optics by matching the dispersion of the spectrometer channels to laterally graded multilayers (LGMLs). The system can achieve polarization modulation factors over 90%. For PiSoX, the optics are lightweight Si mirrors in a one-bounce parabolic configuration. High efficiency, blazed gratings from opposite sectors are oriented to disperse to a LGML forming a channel covering the wavelength range from 35 Å to 75 Å (165 - 350 eV). Upon satellite rotation, the intensities of the dispersed spectra, after reflection and polarizing by the LGMLs, give the three Stokes parameters needed to determine a source’s linear polarization fraction and orientation. The design can be extended to higher energies as LGMLs are developed further. We describe examples of the potential scientific return from instruments based on this design.
Publishing Year
Date Published
2020-12-13
Proceedings Title
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Volume
11444
Article Number
114442Y
Conference
Astronomical Telescopes + Instrumentation
Conference Location
Virtual
Conference Date
2020-12-14 – 2020-12-18
eISSN
IST-REx-ID

Cite this

Marshall HL, Heine S, Garner A, et al. A small satellite version of a soft x-ray polarimeter. In: Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. Vol 11444. SPIE; 2020. doi:10.1117/12.2562811
Marshall, H. L., Heine, S., Garner, A., Gullikson, E., Guenther, M., Leitz, C., … Schulz, N. (2020). A small satellite version of a soft x-ray polarimeter. In Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray (Vol. 11444). Virtual: SPIE. https://doi.org/10.1117/12.2562811
Marshall, Herman L., Sarah Heine, Alan Garner, Eric Gullikson, Moritz Guenther, Christopher Leitz, Rebecca Masterson, et al. “A Small Satellite Version of a Soft X-Ray Polarimeter.” In Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, Vol. 11444. SPIE, 2020. https://doi.org/10.1117/12.2562811.
H. L. Marshall et al., “A small satellite version of a soft x-ray polarimeter,” in Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, Virtual, 2020, vol. 11444.
Marshall HL, Heine S, Garner A, Gullikson E, Guenther M, Leitz C, Masterson R, Miller E, Zhang W, Boissay Malaquin R, Caiazzo I, Chakrabarty D, Davidson R, Gallo L, Heilmann RK, Heyl J, Kara E, Marscher A, Schulz N. 2020. A small satellite version of a soft x-ray polarimeter. Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. Astronomical Telescopes + Instrumentation vol. 11444, 114442Y.
Marshall, Herman L., et al. “A Small Satellite Version of a Soft X-Ray Polarimeter.” Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, vol. 11444, 114442Y, SPIE, 2020, doi:10.1117/12.2562811.
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arXiv 2012.02829

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