Toward large-area sub-arcsecond x-ray telescopes II

Stephen L. O'Dell; Ryan Allured; Andrew O. Ames; Michael P. Biskach; David M. Broadway; Ricardo J. Bruni; David N. Burrows; Jian Cao; Brandon D. Chalifoux; Kai Wing Chan; Yip Wah Chung; Vincenzo Cotroneo; Ronald F. Elsner; Jessica A. Gaskin; Mikhail V. Gubarev; Ralf K. Heilmann; Edward Hertz; Thomas N. Jackson; Kiranmayee Kilaru; Jeffrey J. Kolodziejczak; Ryan S. McClelland; Brian D. Ramsey; Paul B. Reid; Raul E. Riveros; Jacqueline M. Roche; Suzanne E. Romaine; Timo T. Saha; Mark L. Schattenburg; Daniel A. Schwartz; Eric D. Schwartz; Peter M. Solly; Susan Trolier-Mckinstry; Melville P. Ulmer; Alexey Vikhlinin; Margeaux L. Wallace; Xiaoli Wang; David L. Windt; Youwei Yao; Shi Ye; William W. Zhang; Heng Zuo

doi:10.1117/12.2238247

Toward large-area sub-arcsecond x-ray telescopes II

Stephen L. O'Dell, Ryan Allured, Andrew O. Ames, Michael P. Biskach, David M. Broadway, Ricardo J. Bruni, David N. Burrows, Jian Cao, Brandon D. Chalifoux, Kai Wing Chan, Yip Wah Chung, Vincenzo Cotroneo, Ronald F. Elsner, Jessica A. Gaskin, Mikhail V. Gubarev, Ralf K. Heilmann, Edward Hertz, Thomas N. Jackson, Kiranmayee Kilaru, Jeffrey J. KolodziejczakRyan S. McClelland, Brian D. Ramsey, Paul B. Reid, Raul E. Riveros, Jacqueline M. Roche, Suzanne E. Romaine, Timo T. Saha, Mark L. Schattenburg, Daniel A. Schwartz, Eric D. Schwartz, Peter M. Solly, Susan Trolier-Mckinstry, Melville P. Ulmer, Alexey Vikhlinin, Margeaux L. Wallace, Xiaoli Wang, David L. Windt, Youwei Yao, Shi Ye, William W. Zhang, Heng Zuo

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

16 Scopus citations

Abstract

In order to advance significantly scientific objectives, future x-ray astronomy missions will likely call for x-ray telescopes with large aperture areas (3 m²) and fine angular resolution ( 1²). Achieving such performance is programmatically and technologically challenging due to the mass and envelope constraints of space-borne telescopes and to the need for densely nested grazing-incidence optics. Such an x-ray telescope will require precision fabrication, alignment, mounting, and assembly of large areas (600 m2) of lightweight (2 kg/m² areal density) high-quality mirrors, at an acceptable cost (1 M$/m² of mirror surface area). This paper reviews relevant programmatic and technological issues, as well as possible approaches for addressing these issues-including direct fabrication of monocrystalline silicon mirrors, active (in-space adjustable) figure correction of replicated mirrors, static post-fabrication correction using ion implantation, differential erosion or deposition, and coating-stress manipulation of thin substrates.

Original language	English (US)
Title of host publication	Adaptive X-Ray Optics IV
Editors	Stephen L. O'Dell, Ali M. Khounsary
Publisher	SPIE
ISBN (Electronic)	9781510603219
DOIs	https://doi.org/10.1117/12.2238247
State	Published - 2016
Event	Adaptive X-Ray Optics IV - San Diego, United States Duration: Aug 28 2016 → Aug 29 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9965
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Adaptive X-Ray Optics IV
Country/Territory	United States
City	San Diego
Period	8/28/16 → 8/29/16

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2238247

Cite this

O'Dell, S. L., Allured, R., Ames, A. O., Biskach, M. P., Broadway, D. M., Bruni, R. J., Burrows, D. N., Cao, J., Chalifoux, B. D., Chan, K. W., Chung, Y. W., Cotroneo, V., Elsner, R. F., Gaskin, J. A., Gubarev, M. V., Heilmann, R. K., Hertz, E., Jackson, T. N., Kilaru, K., ... Zuo, H. (2016). Toward large-area sub-arcsecond x-ray telescopes II. In S. L. O'Dell, & A. M. Khounsary (Eds.), Adaptive X-Ray Optics IV Article 996507 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9965). SPIE. https://doi.org/10.1117/12.2238247

@inproceedings{0fe0796eea0945d7b53f34b512e3d56a,

title = "Toward large-area sub-arcsecond x-ray telescopes II",

abstract = "In order to advance significantly scientific objectives, future x-ray astronomy missions will likely call for x-ray telescopes with large aperture areas (3 m2) and fine angular resolution ( 12). Achieving such performance is programmatically and technologically challenging due to the mass and envelope constraints of space-borne telescopes and to the need for densely nested grazing-incidence optics. Such an x-ray telescope will require precision fabrication, alignment, mounting, and assembly of large areas (600 m2) of lightweight (2 kg/m2 areal density) high-quality mirrors, at an acceptable cost (1 M$/m2 of mirror surface area). This paper reviews relevant programmatic and technological issues, as well as possible approaches for addressing these issues-including direct fabrication of monocrystalline silicon mirrors, active (in-space adjustable) figure correction of replicated mirrors, static post-fabrication correction using ion implantation, differential erosion or deposition, and coating-stress manipulation of thin substrates.",

author = "O'Dell, {Stephen L.} and Ryan Allured and Ames, {Andrew O.} and Biskach, {Michael P.} and Broadway, {David M.} and Bruni, {Ricardo J.} and Burrows, {David N.} and Jian Cao and Chalifoux, {Brandon D.} and Chan, {Kai Wing} and Chung, {Yip Wah} and Vincenzo Cotroneo and Elsner, {Ronald F.} and Gaskin, {Jessica A.} and Gubarev, {Mikhail V.} and Heilmann, {Ralf K.} and Edward Hertz and Jackson, {Thomas N.} and Kiranmayee Kilaru and Kolodziejczak, {Jeffrey J.} and McClelland, {Ryan S.} and Ramsey, {Brian D.} and Reid, {Paul B.} and Riveros, {Raul E.} and Roche, {Jacqueline M.} and Romaine, {Suzanne E.} and Saha, {Timo T.} and Schattenburg, {Mark L.} and Schwartz, {Daniel A.} and Schwartz, {Eric D.} and Solly, {Peter M.} and Susan Trolier-Mckinstry and Ulmer, {Melville P.} and Alexey Vikhlinin and Wallace, {Margeaux L.} and Xiaoli Wang and Windt, {David L.} and Youwei Yao and Shi Ye and Zhang, {William W.} and Heng Zuo",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Adaptive X-Ray Optics IV ; Conference date: 28-08-2016 Through 29-08-2016",

year = "2016",

doi = "10.1117/12.2238247",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "O'Dell, {Stephen L.} and Khounsary, {Ali M.}",

booktitle = "Adaptive X-Ray Optics IV",

address = "United States",

}

O'Dell, SL, Allured, R, Ames, AO, Biskach, MP, Broadway, DM, Bruni, RJ, Burrows, DN, Cao, J, Chalifoux, BD, Chan, KW, Chung, YW, Cotroneo, V, Elsner, RF, Gaskin, JA, Gubarev, MV, Heilmann, RK, Hertz, E, Jackson, TN, Kilaru, K, Kolodziejczak, JJ, McClelland, RS, Ramsey, BD, Reid, PB, Riveros, RE, Roche, JM, Romaine, SE, Saha, TT, Schattenburg, ML, Schwartz, DA, Schwartz, ED, Solly, PM, Trolier-Mckinstry, S, Ulmer, MP, Vikhlinin, A, Wallace, ML, Wang, X, Windt, DL, Yao, Y, Ye, S, Zhang, WW & Zuo, H 2016, Toward large-area sub-arcsecond x-ray telescopes II. in SL O'Dell & AM Khounsary (eds), Adaptive X-Ray Optics IV., 996507, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9965, SPIE, Adaptive X-Ray Optics IV, San Diego, United States, 8/28/16. https://doi.org/10.1117/12.2238247

Toward large-area sub-arcsecond x-ray telescopes II. / O'Dell, Stephen L.; Allured, Ryan; Ames, Andrew O. et al.
Adaptive X-Ray Optics IV. ed. / Stephen L. O'Dell; Ali M. Khounsary. SPIE, 2016. 996507 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9965).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Toward large-area sub-arcsecond x-ray telescopes II

AU - O'Dell, Stephen L.

AU - Allured, Ryan

AU - Ames, Andrew O.

AU - Biskach, Michael P.

AU - Broadway, David M.

AU - Bruni, Ricardo J.

AU - Burrows, David N.

AU - Cao, Jian

AU - Chalifoux, Brandon D.

AU - Chan, Kai Wing

AU - Chung, Yip Wah

AU - Cotroneo, Vincenzo

AU - Elsner, Ronald F.

AU - Gaskin, Jessica A.

AU - Gubarev, Mikhail V.

AU - Heilmann, Ralf K.

AU - Hertz, Edward

AU - Jackson, Thomas N.

AU - Kilaru, Kiranmayee

AU - Kolodziejczak, Jeffrey J.

AU - McClelland, Ryan S.

AU - Ramsey, Brian D.

AU - Reid, Paul B.

AU - Riveros, Raul E.

AU - Roche, Jacqueline M.

AU - Romaine, Suzanne E.

AU - Saha, Timo T.

AU - Schattenburg, Mark L.

AU - Schwartz, Daniel A.

AU - Schwartz, Eric D.

AU - Solly, Peter M.

AU - Trolier-Mckinstry, Susan

AU - Ulmer, Melville P.

AU - Vikhlinin, Alexey

AU - Wallace, Margeaux L.

AU - Wang, Xiaoli

AU - Windt, David L.

AU - Yao, Youwei

AU - Ye, Shi

AU - Zhang, William W.

AU - Zuo, Heng

PY - 2016

Y1 - 2016

N2 - In order to advance significantly scientific objectives, future x-ray astronomy missions will likely call for x-ray telescopes with large aperture areas (3 m2) and fine angular resolution ( 12). Achieving such performance is programmatically and technologically challenging due to the mass and envelope constraints of space-borne telescopes and to the need for densely nested grazing-incidence optics. Such an x-ray telescope will require precision fabrication, alignment, mounting, and assembly of large areas (600 m2) of lightweight (2 kg/m2 areal density) high-quality mirrors, at an acceptable cost (1 M$/m2 of mirror surface area). This paper reviews relevant programmatic and technological issues, as well as possible approaches for addressing these issues-including direct fabrication of monocrystalline silicon mirrors, active (in-space adjustable) figure correction of replicated mirrors, static post-fabrication correction using ion implantation, differential erosion or deposition, and coating-stress manipulation of thin substrates.

AB - In order to advance significantly scientific objectives, future x-ray astronomy missions will likely call for x-ray telescopes with large aperture areas (3 m2) and fine angular resolution ( 12). Achieving such performance is programmatically and technologically challenging due to the mass and envelope constraints of space-borne telescopes and to the need for densely nested grazing-incidence optics. Such an x-ray telescope will require precision fabrication, alignment, mounting, and assembly of large areas (600 m2) of lightweight (2 kg/m2 areal density) high-quality mirrors, at an acceptable cost (1 M$/m2 of mirror surface area). This paper reviews relevant programmatic and technological issues, as well as possible approaches for addressing these issues-including direct fabrication of monocrystalline silicon mirrors, active (in-space adjustable) figure correction of replicated mirrors, static post-fabrication correction using ion implantation, differential erosion or deposition, and coating-stress manipulation of thin substrates.

UR - http://www.scopus.com/inward/record.url?scp=85015168718&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85015168718&partnerID=8YFLogxK

U2 - 10.1117/12.2238247

DO - 10.1117/12.2238247

M3 - Conference contribution

AN - SCOPUS:85015168718

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Adaptive X-Ray Optics IV

A2 - O'Dell, Stephen L.

A2 - Khounsary, Ali M.

PB - SPIE

T2 - Adaptive X-Ray Optics IV

Y2 - 28 August 2016 through 29 August 2016

ER -

Toward large-area sub-arcsecond x-ray telescopes II

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