Crowded Field Astrometry with SIM

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The presence of faint background stars within the 3" field-of-view (FOV) of SIM confuses the measurements and introduces errors that can be significantly larger than the precision with which the measurements are expected to be made. Earlier studies on understanding the nature and magnitude of these errors have indicated that the errors depend upon the disposition of the sources within the FOV, baseline orientation, instrumental throughput, spectral energy distribution of the stars and the number of spectral channels used for recording the data. However, these earlier studies have not incorporated the actual measurement processthe measurement of intensity over the FOV as a function of path delay, in the case of confused fields. We report results of a detailed study undertaken in an effort to model the measurement process as accurately as possible and identify the approaches that can be used in order to obtain the best fit to the measured data. We plan to use this model to account for the error introduced by the confusing sources.

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