Paper
1 June 1994 Astrometric calibration of array detectors
Stuart B. Shaklan, Steven H. Pravdo
Author Affiliations +
Abstract
The high level of spatial uniformity in modern CCDs and other array detectors make them excellent devices for astrometric and navigational systems. However, at the level of accuracy envisioned by the more ambitious projects, current technology produces devices with significant pixel registration errors. This paper describes a technique for measuring relative pixel positions to an accuracy approaching 0.001 pixel. The technique has been applied to WF/PC II CCDs which are shown to have 500 nm step-and-repeat errors.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stuart B. Shaklan and Steven H. Pravdo "Astrometric calibration of array detectors", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); https://doi.org/10.1117/12.176810
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Charge-coupled devices

Quantum efficiency

Stars

Calibration

Spatial frequencies

Sensors

Space telescopes

RELATED CONTENT

CCD detectors for the advanced camera for surveys
Proceedings of SPIE (August 16 2000)
The STELLA robotic observatory on Tenerife
Proceedings of SPIE (September 24 2012)
XMM-Newton satellite MOS CCD detectors calibration results
Proceedings of SPIE (November 28 2000)
CUBIC: preflight calibration results and initial operations
Proceedings of SPIE (October 31 1996)
CUBIC: preflight calibration status
Proceedings of SPIE (September 01 1995)

Back to Top