Full-sky Astrometric Mapping Explorer (FAME) CCD centroiding experiment

Kenneth J. Triebes; Larry Gilliam; Timothy Hilby; Scott D. Horner; Patrick Perkins; Richard H. Vassar; Frederick H. Harris; David G. Monet

doi:10.1117/12.394031

28 July 2000 Full-sky Astrometric Mapping Explorer (FAME) CCD centroiding experiment

Kenneth J. Triebes, Larry Gilliam, Timothy Hilby, Scott D. Horner, Patrick Perkins, Richard H. Vassar, Frederick H. Harris, David G. Monet

Author Affiliations +

Proceedings Volume 4013, UV, Optical, and IR Space Telescopes and Instruments; (2000) https://doi.org/10.1117/12.394031
Event: Astronomical Telescopes and Instrumentation, 2000, Munich, Germany

Abstract

FAME is a MIDEX astrometry mission designed to map the position of 40,000,000 stars to an accuracy of 50 micro-arc seconds. Optimized between mission requirements, size, weight, and cost, the FAME instrument consists of a 0.6 X 0.5 m² aperture whose point spread function central peak is linearly sampled by two pixels. To achieve its astrometric mapping mission requirements, this instrument must achieve a single look centroiding accuracy on a visual magnitude 9.0 (or brighter) star of < 0.003 pixels while operating the focal plane in a time domain integration, TDI, mode. As this performance requirement represents a significant improvement over the current state of the art of 0.02 to 0.01 pixel resolution, a risk reduction experiment was conducted to determine our centroiding ability using a flight traceable CCD operated in TDI mode.

Citation Download Citation

Kenneth J. Triebes, Larry Gilliam, Timothy Hilby, Scott D. Horner, Patrick Perkins, Richard H. Vassar, Frederick H. Harris, and David G. Monet "Full-sky Astrometric Mapping Explorer (FAME) CCD centroiding experiment", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); https://doi.org/10.1117/12.394031

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