Toward active x-ray telescopes II

Stephen L. O'Dell; Thomas L. Aldcroft; Carolyn Atkins; Timothy W. Button; Vincenzo Cotroneo; William N. Davis; Peter Doel; Charlotte H. Feldman; Mark D. Freeman; Mikhail V. Gubarev; Raegan L. Johnson-Wilke; Jeffery J. Kolodziejczak; Charles F. Lillie; Alan G. Michette; Brian D. Ramsey; Paul B. Reid; Daniel Rodriguez Sanmartin; Timo T. Saha; Daniel A. Schwartz; Susan E. Trolier-McKinstry; Melville P. Ulmer; Rudeger H.T. Wilke; Richard Willingale; William W. Zhang

doi:10.1117/12.930090

Toward active x-ray telescopes II

Stephen L. O'Dell, Thomas L. Aldcroft, Carolyn Atkins, Timothy W. Button, Vincenzo Cotroneo, William N. Davis, Peter Doel, Charlotte H. Feldman, Mark D. Freeman, Mikhail V. Gubarev, Raegan L. Johnson-Wilke, Jeffery J. Kolodziejczak, Charles F. Lillie, Alan G. Michette, Brian D. Ramsey, Paul B. Reid, Daniel Rodriguez Sanmartin, Timo T. Saha, Daniel A. Schwartz, Susan E. Trolier-McKinstryMelville P. Ulmer, Rudeger H.T. Wilke, Richard Willingale, William W. Zhang

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

10 Scopus citations

Abstract

In the half century since the initial discovery of an astronomical (non-solar) x-ray source, the observation time required to achieve a given sensitivity has decreased by eight orders of magnitude. Largely responsible for this dramatic progress has been the refinement of the (grazing-incidence) focusing x-ray telescope, culminating with the exquisite subarcsecond imaging performance of the Chandra X-ray Observatory. The future of x-ray astronomy relies upon the development of x-ray telescopes with larger aperture areas (> 1 m²) and comparable or finer angular resolution (< 1″). Combined with the special requirements of grazing-incidence optics, the mass and envelope constraints of space-borne telescopes render such advances technologically challenging-requiring precision fabrication, alignment, and assembly of large areas (> 200 m²) of lightweight (≈ 1 kg m^-2 areal density) mirrors. Achieving precise and stable alignment and figure control may entail active (in-space adjustable) x-ray optics. This paper discusses relevant programmatic and technological issues and summarizes current progress toward active x-ray telescopes.

Original language	English (US)
Title of host publication	Adaptive X-Ray Optics II
DOIs	https://doi.org/10.1117/12.930090
State	Published - 2012
Event	Adaptive X-Ray Optics II - San Diego, CA, United States Duration: Aug 14 2012 → Aug 14 2012

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8503
ISSN (Print)	0277-786X

Other

Other	Adaptive X-Ray Optics II
Country/Territory	United States
City	San Diego, CA
Period	8/14/12 → 8/14/12

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

10.1117/12.930090

Cite this

O'Dell, S. L., Aldcroft, T. L., Atkins, C., Button, T. W., Cotroneo, V., Davis, W. N., Doel, P., Feldman, C. H., Freeman, M. D., Gubarev, M. V., Johnson-Wilke, R. L., Kolodziejczak, J. J., Lillie, C. F., Michette, A. G., Ramsey, B. D., Reid, P. B., Sanmartin, D. R., Saha, T. T., Schwartz, D. A., ... Zhang, W. W. (2012). Toward active x-ray telescopes II. In Adaptive X-Ray Optics II Article 850307 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8503). https://doi.org/10.1117/12.930090

@inproceedings{5d9d09d5d371418ea0851e92f2e20abd,

title = "Toward active x-ray telescopes II",

abstract = "In the half century since the initial discovery of an astronomical (non-solar) x-ray source, the observation time required to achieve a given sensitivity has decreased by eight orders of magnitude. Largely responsible for this dramatic progress has been the refinement of the (grazing-incidence) focusing x-ray telescope, culminating with the exquisite subarcsecond imaging performance of the Chandra X-ray Observatory. The future of x-ray astronomy relies upon the development of x-ray telescopes with larger aperture areas (> 1 m2) and comparable or finer angular resolution (< 1″). Combined with the special requirements of grazing-incidence optics, the mass and envelope constraints of space-borne telescopes render such advances technologically challenging-requiring precision fabrication, alignment, and assembly of large areas (> 200 m2) of lightweight (≈ 1 kg m-2 areal density) mirrors. Achieving precise and stable alignment and figure control may entail active (in-space adjustable) x-ray optics. This paper discusses relevant programmatic and technological issues and summarizes current progress toward active x-ray telescopes.",

author = "O'Dell, {Stephen L.} and Aldcroft, {Thomas L.} and Carolyn Atkins and Button, {Timothy W.} and Vincenzo Cotroneo and Davis, {William N.} and Peter Doel and Feldman, {Charlotte H.} and Freeman, {Mark D.} and Gubarev, {Mikhail V.} and Johnson-Wilke, {Raegan L.} and Kolodziejczak, {Jeffery J.} and Lillie, {Charles F.} and Michette, {Alan G.} and Ramsey, {Brian D.} and Reid, {Paul B.} and Sanmartin, {Daniel Rodriguez} and Saha, {Timo T.} and Schwartz, {Daniel A.} and Trolier-McKinstry, {Susan E.} and Ulmer, {Melville P.} and Wilke, {Rudeger H.T.} and Richard Willingale and Zhang, {William W.}",

year = "2012",

doi = "10.1117/12.930090",

language = "English (US)",

isbn = "9780819492203",

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

booktitle = "Adaptive X-Ray Optics II",

note = "Adaptive X-Ray Optics II ; Conference date: 14-08-2012 Through 14-08-2012",

}

O'Dell, SL, Aldcroft, TL, Atkins, C, Button, TW, Cotroneo, V, Davis, WN, Doel, P, Feldman, CH, Freeman, MD, Gubarev, MV, Johnson-Wilke, RL, Kolodziejczak, JJ, Lillie, CF, Michette, AG, Ramsey, BD, Reid, PB, Sanmartin, DR, Saha, TT, Schwartz, DA, Trolier-McKinstry, SE, Ulmer, MP, Wilke, RHT, Willingale, R & Zhang, WW 2012, Toward active x-ray telescopes II. in Adaptive X-Ray Optics II., 850307, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8503, Adaptive X-Ray Optics II, San Diego, CA, United States, 8/14/12. https://doi.org/10.1117/12.930090

TY - GEN

T1 - Toward active x-ray telescopes II

AU - O'Dell, Stephen L.

AU - Aldcroft, Thomas L.

AU - Atkins, Carolyn

AU - Button, Timothy W.

AU - Cotroneo, Vincenzo

AU - Davis, William N.

AU - Doel, Peter

AU - Feldman, Charlotte H.

AU - Freeman, Mark D.

AU - Gubarev, Mikhail V.

AU - Johnson-Wilke, Raegan L.

AU - Kolodziejczak, Jeffery J.

AU - Lillie, Charles F.

AU - Michette, Alan G.

AU - Ramsey, Brian D.

AU - Reid, Paul B.

AU - Sanmartin, Daniel Rodriguez

AU - Saha, Timo T.

AU - Schwartz, Daniel A.

AU - Trolier-McKinstry, Susan E.

AU - Ulmer, Melville P.

AU - Wilke, Rudeger H.T.

AU - Willingale, Richard

AU - Zhang, William W.

PY - 2012

Y1 - 2012

N2 - In the half century since the initial discovery of an astronomical (non-solar) x-ray source, the observation time required to achieve a given sensitivity has decreased by eight orders of magnitude. Largely responsible for this dramatic progress has been the refinement of the (grazing-incidence) focusing x-ray telescope, culminating with the exquisite subarcsecond imaging performance of the Chandra X-ray Observatory. The future of x-ray astronomy relies upon the development of x-ray telescopes with larger aperture areas (> 1 m2) and comparable or finer angular resolution (< 1″). Combined with the special requirements of grazing-incidence optics, the mass and envelope constraints of space-borne telescopes render such advances technologically challenging-requiring precision fabrication, alignment, and assembly of large areas (> 200 m2) of lightweight (≈ 1 kg m-2 areal density) mirrors. Achieving precise and stable alignment and figure control may entail active (in-space adjustable) x-ray optics. This paper discusses relevant programmatic and technological issues and summarizes current progress toward active x-ray telescopes.

AB - In the half century since the initial discovery of an astronomical (non-solar) x-ray source, the observation time required to achieve a given sensitivity has decreased by eight orders of magnitude. Largely responsible for this dramatic progress has been the refinement of the (grazing-incidence) focusing x-ray telescope, culminating with the exquisite subarcsecond imaging performance of the Chandra X-ray Observatory. The future of x-ray astronomy relies upon the development of x-ray telescopes with larger aperture areas (> 1 m2) and comparable or finer angular resolution (< 1″). Combined with the special requirements of grazing-incidence optics, the mass and envelope constraints of space-borne telescopes render such advances technologically challenging-requiring precision fabrication, alignment, and assembly of large areas (> 200 m2) of lightweight (≈ 1 kg m-2 areal density) mirrors. Achieving precise and stable alignment and figure control may entail active (in-space adjustable) x-ray optics. This paper discusses relevant programmatic and technological issues and summarizes current progress toward active x-ray telescopes.

UR - http://www.scopus.com/inward/record.url?scp=84872541046&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84872541046&partnerID=8YFLogxK

U2 - 10.1117/12.930090

DO - 10.1117/12.930090

M3 - Conference contribution

AN - SCOPUS:84872541046

SN - 9780819492203

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

BT - Adaptive X-Ray Optics II

T2 - Adaptive X-Ray Optics II

Y2 - 14 August 2012 through 14 August 2012

ER -

Toward active x-ray telescopes II

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