Optical instrument design of the high-energy x-ray probe (HEX-P)

Kristin K. Madsen; Fiona Harrison; D. Broadway; F. E. Christensen; M. Descalle; D. Ferreira; B. Grefenstette; D. Gurgew; A. Hornschemeier; H. Miyasaka; T. Okajima; S. Pike; M. Pivovaroff; T. Saha; D. Stern; J. Vogel; D. Windt; W. Zhang

doi:10.1117/12.2314117

Optical instrument design of the high-energy x-ray probe (HEX-P)

Kristin K. Madsen^*, Fiona Harrison, D. Broadway, F. E. Christensen, M. Descalle, D. Ferreira, B. Grefenstette, D. Gurgew, A. Hornschemeier, H. Miyasaka, T. Okajima, S. Pike, M. Pivovaroff, T. Saha, D. Stern, J. Vogel, D. Windt, W. Zhang

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

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Abstract

The High-Energy X-ray Probe (HEX-P) is a probe-class next-generation high-energy X-ray mission concept that will vastly extend the reach of broadband X-ray observations. Studying the 2-200 keV energy range, HEXP has 40 times the sensitivity of any previous mission in the 10-80 keV band, and will be the first focusing instrument in the 80-200 keV band. A successor to the Nuclear Spectroscopic Telescope Array (NuSTAR), a NASA Small Explorer launched in 2012, HEX-P addresses key NASA science objectives, and will serve as an important complement to ESA's L-class Athena mission. HEX-P will utilize multilayer coated X-ray optics, and in this paper we present the details of the optical design, and discuss the multilayer prescriptions necessary for the reflection of hard X-ray photons. We consider multiple module designs with the aim of investigating the tradeoff between high- and low-energy effective area, and review the technology development necessary to reach that goal within the next decade.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
Editors	Jan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
Number of pages	10
Volume	10699
Publisher	SPIE - International Society for Optical Engineering
Publication date	2018
Article number	106996M
ISBN (Print)	9781510619517
DOIs	https://doi.org/10.1117/12.2314117
Publication status	Published - 2018
Event	SPIE Astronomical Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray - Austin, United States Duration: 10 Jun 2018 → 15 Jun 2018

Conference

Conference	SPIE Astronomical Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
Country	United States
City	Austin
Period	10/06/2018 → 15/06/2018
Sponsor	4D Technology Corporation, Andor Technology, Ltd., Astronomical Consultants and Equipment, Inc., Giant Magellan Telescope, SPIE

Keywords

HEX-P
Satellite
X-ray

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Madsen, K. K., Harrison, F., Broadway, D., Christensen, F. E., Descalle, M., Ferreira, D., Grefenstette, B., Gurgew, D., Hornschemeier, A., Miyasaka, H., Okajima, T., Pike, S., Pivovaroff, M., Saha, T., Stern, D., Vogel, J., Windt, D., & Zhang, W. (2018). Optical instrument design of the high-energy x-ray probe (HEX-P). In J-W. A. den Herder, S. Nikzad, & K. Nakazawa (Eds.), Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray (Vol. 10699). [106996M] SPIE - International Society for Optical Engineering. https://doi.org/10.1117/12.2314117

Madsen, Kristin K. ; Harrison, Fiona ; Broadway, D. ; Christensen, F. E. ; Descalle, M. ; Ferreira, D. ; Grefenstette, B. ; Gurgew, D. ; Hornschemeier, A. ; Miyasaka, H. ; Okajima, T. ; Pike, S. ; Pivovaroff, M. ; Saha, T. ; Stern, D. ; Vogel, J. ; Windt, D. ; Zhang, W. / Optical instrument design of the high-energy x-ray probe (HEX-P). Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray. editor / Jan-Willem A. den Herder ; Shouleh Nikzad ; Kazuhiro Nakazawa. Vol. 10699 SPIE - International Society for Optical Engineering, 2018.

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title = "Optical instrument design of the high-energy x-ray probe (HEX-P)",

abstract = "The High-Energy X-ray Probe (HEX-P) is a probe-class next-generation high-energy X-ray mission concept that will vastly extend the reach of broadband X-ray observations. Studying the 2-200 keV energy range, HEXP has 40 times the sensitivity of any previous mission in the 10-80 keV band, and will be the first focusing instrument in the 80-200 keV band. A successor to the Nuclear Spectroscopic Telescope Array (NuSTAR), a NASA Small Explorer launched in 2012, HEX-P addresses key NASA science objectives, and will serve as an important complement to ESA's L-class Athena mission. HEX-P will utilize multilayer coated X-ray optics, and in this paper we present the details of the optical design, and discuss the multilayer prescriptions necessary for the reflection of hard X-ray photons. We consider multiple module designs with the aim of investigating the tradeoff between high- and low-energy effective area, and review the technology development necessary to reach that goal within the next decade.",

keywords = "HEX-P, Satellite, X-ray",

author = "Madsen, {Kristin K.} and Fiona Harrison and D. Broadway and Christensen, {F. E.} and M. Descalle and D. Ferreira and B. Grefenstette and D. Gurgew and A. Hornschemeier and H. Miyasaka and T. Okajima and S. Pike and M. Pivovaroff and T. Saha and D. Stern and J. Vogel and D. Windt and W. Zhang",

year = "2018",

doi = "10.1117/12.2314117",

language = "English",

isbn = "9781510619517",

volume = "10699",

editor = "{den Herder}, {Jan-Willem A. } and Nikzad, {Shouleh } and Nakazawa, {Kazuhiro }",

booktitle = "Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray",

publisher = "SPIE - International Society for Optical Engineering",

note = "SPIE Astronomical Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray ; Conference date: 10-06-2018 Through 15-06-2018",

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Madsen, KK, Harrison, F, Broadway, D, Christensen, FE, Descalle, M, Ferreira, D, Grefenstette, B, Gurgew, D, Hornschemeier, A, Miyasaka, H, Okajima, T, Pike, S, Pivovaroff, M, Saha, T, Stern, D, Vogel, J, Windt, D & Zhang, W 2018, Optical instrument design of the high-energy x-ray probe (HEX-P). in J-WA den Herder, S Nikzad & K Nakazawa (eds), Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray. vol. 10699, 106996M, SPIE - International Society for Optical Engineering, SPIE Astronomical Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, Austin, United States, 10/06/2018. https://doi.org/10.1117/12.2314117

Optical instrument design of the high-energy x-ray probe (HEX-P). / Madsen, Kristin K.; Harrison, Fiona; Broadway, D.; Christensen, F. E.; Descalle, M.; Ferreira, D.; Grefenstette, B.; Gurgew, D.; Hornschemeier, A.; Miyasaka, H.; Okajima, T.; Pike, S.; Pivovaroff, M.; Saha, T.; Stern, D.; Vogel, J.; Windt, D.; Zhang, W.

Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray. ed. / Jan-Willem A. den Herder; Shouleh Nikzad; Kazuhiro Nakazawa. Vol. 10699 SPIE - International Society for Optical Engineering, 2018. 106996M.

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - Optical instrument design of the high-energy x-ray probe (HEX-P)

AU - Madsen, Kristin K.

AU - Harrison, Fiona

AU - Broadway, D.

AU - Christensen, F. E.

AU - Descalle, M.

AU - Ferreira, D.

AU - Grefenstette, B.

AU - Gurgew, D.

AU - Hornschemeier, A.

AU - Miyasaka, H.

AU - Okajima, T.

AU - Pike, S.

AU - Pivovaroff, M.

AU - Saha, T.

AU - Stern, D.

AU - Vogel, J.

AU - Windt, D.

AU - Zhang, W.

PY - 2018

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N2 - The High-Energy X-ray Probe (HEX-P) is a probe-class next-generation high-energy X-ray mission concept that will vastly extend the reach of broadband X-ray observations. Studying the 2-200 keV energy range, HEXP has 40 times the sensitivity of any previous mission in the 10-80 keV band, and will be the first focusing instrument in the 80-200 keV band. A successor to the Nuclear Spectroscopic Telescope Array (NuSTAR), a NASA Small Explorer launched in 2012, HEX-P addresses key NASA science objectives, and will serve as an important complement to ESA's L-class Athena mission. HEX-P will utilize multilayer coated X-ray optics, and in this paper we present the details of the optical design, and discuss the multilayer prescriptions necessary for the reflection of hard X-ray photons. We consider multiple module designs with the aim of investigating the tradeoff between high- and low-energy effective area, and review the technology development necessary to reach that goal within the next decade.

AB - The High-Energy X-ray Probe (HEX-P) is a probe-class next-generation high-energy X-ray mission concept that will vastly extend the reach of broadband X-ray observations. Studying the 2-200 keV energy range, HEXP has 40 times the sensitivity of any previous mission in the 10-80 keV band, and will be the first focusing instrument in the 80-200 keV band. A successor to the Nuclear Spectroscopic Telescope Array (NuSTAR), a NASA Small Explorer launched in 2012, HEX-P addresses key NASA science objectives, and will serve as an important complement to ESA's L-class Athena mission. HEX-P will utilize multilayer coated X-ray optics, and in this paper we present the details of the optical design, and discuss the multilayer prescriptions necessary for the reflection of hard X-ray photons. We consider multiple module designs with the aim of investigating the tradeoff between high- and low-energy effective area, and review the technology development necessary to reach that goal within the next decade.

KW - HEX-P

KW - Satellite

KW - X-ray

U2 - 10.1117/12.2314117

DO - 10.1117/12.2314117

M3 - Article in proceedings

AN - SCOPUS:85051871664

SN - 9781510619517

VL - 10699

BT - Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray

A2 - den Herder, Jan-Willem A.

A2 - Nikzad, Shouleh

A2 - Nakazawa, Kazuhiro

PB - SPIE - International Society for Optical Engineering

T2 - SPIE Astronomical Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray

Y2 - 10 June 2018 through 15 June 2018

ER -

Madsen KK, Harrison F, Broadway D, Christensen FE, Descalle M, Ferreira D et al. Optical instrument design of the high-energy x-ray probe (HEX-P). In den Herder J-WA, Nikzad S, Nakazawa K, editors, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray. Vol. 10699. SPIE - International Society for Optical Engineering. 2018. 106996M https://doi.org/10.1117/12.2314117