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Astrometric Interferometry in Space
Mike Shao (Jet Propulsion Laboratory)
Abstract:
This lecture will describe how space astrometry is conducted. Ground based
interferometric astrometry is tied to the rotation of the Earth. In space, the
platform (the spacecraft) is much less stable than the Earth, while at the
same time, we want to achieve much higher accuracy. The lecture will describe
how a space based astrometric interferometer would synthesize a microarcsec
stable platform using "guide" stars and optical metrology. The 2nd major topic
of the talk will be on systematic errors in space astrometric measurements.
What types of instrumental errors are expected, how large instrumental biases
can be corrected through calibration and "chopping".
Viewgraphs PDF 280k Bytes.
Viewgraphs PowerPoint 824k Bytes.
A note on the use of Summer School material.
Suggested Reading:
- Long-Baseline Optical and Near-Infrared Interferometry
M. Shao and M.M. Colavita,
Ann. Rev. Astron. Astrophys. 30, 457-498 (1992).
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2001 | CfA 2002
Course Notes from the 2002 Michelson Interferometry Summer School
Smithsonian Astrophysical Observatory, Cambridge Massachusetts, June 24-28, 2002
Edited by P.R. Lawson (JPL), MS 301-451 Jet Propulsion Laboratory
Pasadena, California, 91109
Last Updated 9 February 2004
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