H.S. Krawczynski
X-ray polarimetry with the Polarization Spectroscopic Telescope Array (PolSTAR)
Krawczynski, H.S.; Stern, D.; Harrison, F.A.; Kislat, F.F.; Zajczyk, A.; Beilicke, M.; Hoormann, J.; Guo, Q.; Endsley, R.; Ingram, A.R.; Miyasaka, H.; Madsen, K.K.; Aaron, K.M.; Amini, R.; Baring, M.G.; Beheshtipour, B.; Bodaghee, A.; Booth, J.; Borden, C.; Böttcher, M.; Christensen, F.E.; Coppi, P.S.; Cowsik, R.; Davis, S.; Dexter, J.; Done, C.; Dominguez, L.A.; Ellison, D.; English, R.J.; Fabian, A.C.; Falcone, A.; Favretto, J.A.; Fernández, R.; Giommi, P.; Grefenstette, B.W.; Kara, E.; Lee, C.H.; Lyutikov, M.; Maccarone, T.; Matsumoto, H.; McKinney, J.; Mihara, T.; Miller, J.M.; Narayan, R.; Natalucci, L.; Özel, F.; Pivovaroff, M.J.; Pravdo, S.; Psaltis, D.; Okajima, T.; Toma, K.; Zhang, W.W.
Authors
D. Stern
F.A. Harrison
F.F. Kislat
A. Zajczyk
M. Beilicke
J. Hoormann
Q. Guo
R. Endsley
A.R. Ingram
H. Miyasaka
K.K. Madsen
K.M. Aaron
R. Amini
M.G. Baring
B. Beheshtipour
A. Bodaghee
J. Booth
C. Borden
M. Böttcher
F.E. Christensen
P.S. Coppi
R. Cowsik
S. Davis
J. Dexter
Professor Christine Done chris.done@durham.ac.uk
Professor
L.A. Dominguez
D. Ellison
R.J. English
A.C. Fabian
A. Falcone
J.A. Favretto
R. Fernández
P. Giommi
B.W. Grefenstette
E. Kara
C.H. Lee
M. Lyutikov
T. Maccarone
H. Matsumoto
J. McKinney
T. Mihara
J.M. Miller
R. Narayan
L. Natalucci
F. Özel
M.J. Pivovaroff
S. Pravdo
D. Psaltis
T. Okajima
K. Toma
W.W. Zhang
Abstract
This paper describes the Polarization Spectroscopic Telescope Array (PolSTAR), a mission proposed to NASA’s 2014 Small Explorer (SMEX) announcement of opportunity. PolSTAR measures the linear polarization of 3–50 keV (requirement; goal: 2.5–70 keV) X-rays probing the behavior of matter, radiation and the very fabric of spacetime under the extreme conditions close to the event horizons of black holes, as well as in and around magnetars and neutron stars. The PolSTAR design is based on the technology developed for the Nuclear Spectroscopic Telescope Array (NuSTAR) mission launched in June 2012. In particular, it uses the same X-ray optics, extendable telescope boom, optical bench, and CdZnTe detectors as NuSTAR. The mission has the sensitivity to measure ∼1% linear polarization fractions for X-ray sources with fluxes down to ∼5 mCrab. This paper describes the PolSTAR design as well as the science drivers and the potential science return.
Citation
Krawczynski, H., Stern, D., Harrison, F., Kislat, F., Zajczyk, A., Beilicke, M., …Zhang, W. (2016). X-ray polarimetry with the Polarization Spectroscopic Telescope Array (PolSTAR). Astroparticle Physics, 75, 8-28. https://doi.org/10.1016/j.astropartphys.2015.10.009
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 22, 2015 |
Online Publication Date | Oct 30, 2015 |
Publication Date | Feb 15, 2016 |
Deposit Date | Mar 16, 2016 |
Publicly Available Date | May 29, 2018 |
Journal | Astroparticle Physics |
Print ISSN | 0927-6505 |
Publisher | Elsevier |
Peer Reviewed | Peer Reviewed |
Volume | 75 |
Pages | 8-28 |
DOI | https://doi.org/10.1016/j.astropartphys.2015.10.009 |
Public URL | https://durham-repository.worktribe.com/output/1388777 |
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http://creativecommons.org/licenses/by-nc-nd/4.0/
Copyright Statement
© 2015 This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/
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