10 August 2010 Achieving milli-arcsecond residual astrometric error for the JMAPS Mission
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The Joint Milliarcsecond Pathfinder Survey (JMAPS) is a small, space-based, all-sky, visible wavelength astrometric and photometric survey mission for 0th through 14th I-band magnitude stars with a planned 2013 launch. The primary objective of the JMAPS mission is the generation of an astrometric star catalog with 1 milliarcsecond (mas) positional accuracy or better, and photometry to the 1% accuracy level or better at 1st to 12th mag. Achieving this level of accuracy in the final catalog requires a demanding attention to reducing systematic effects. We present our findings on distortion, signal to noise, and the astrometric bandpass necessary to obtain the desired accuracy for JMAPS.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gregory S. Hennessy, Gregory S. Hennessy, Benjamin F. Lane, Benjamin F. Lane, Dan Veillette, Dan Veillette, Christopher Dieck, Christopher Dieck, } "Achieving milli-arcsecond residual astrometric error for the JMAPS Mission", Proc. SPIE 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave, 77314L (10 August 2010); doi: 10.1117/12.857476; https://doi.org/10.1117/12.857476

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