Paper
3 October 2007 Toward a complete metrologic solution for the mirrors for the Constellation-X Spectroscopy x-ray telescope
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Abstract
We present an overview update of the metrologic approach to be employed for the segmented mirror fabrication for Constellation-X spectroscopy x-ray telescope. We compare results achieved to date with mission requirements. This is discussed in terms of inherent capability versus in-practice capability. We find that all the needed metrics for the mirrors are in hand but that they are currently limited by the mounting of the mirrors themselves.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. P. Lehan, S. Owens, T. Hadjimichael, M. Hong, K.-W. Chan, T. T. Saha, P. Reid, and W. W. Zhang "Toward a complete metrologic solution for the mirrors for the Constellation-X Spectroscopy x-ray telescope", Proc. SPIE 6688, Optics for EUV, X-Ray, and Gamma-Ray Astronomy III, 668818 (3 October 2007); https://doi.org/10.1117/12.733080
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Cited by 5 scholarly publications.
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KEYWORDS
Mirrors

Metrology

Interferometry

X-ray telescopes

Spectroscopy

Interferometers

Calibration

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