Crowded-Field Astrometry with SIM PlanetQuest. II. An Improved Instrument Model
R. Sridharan, Ronald J. Allen

TL;DR
This paper enhances an astrometric instrument model for SIM PlanetQuest by including spectral dispersion, multi-pixel detectors, and fringe binning, leading to more accurate bias estimates and improved understanding of instrumental effects.
Contribution
It introduces a more comprehensive instrument model that accounts for spectral dispersion, pixelation, and fringe binning, refining previous bias estimations in crowded-field astrometry.
Findings
Pixellation of dispersed fringes causes systematic differences from earlier models.
The improved model helps identify ways to reduce measurement confusion.
Provides a better basis for evaluating instrumental effects in future astrometric observations.
Abstract
In a previous paper we described a method of estimating the single-measurement bias to be expected in astrometric observations of targets in crowded fields with the future Space Interferometry Mission (SIM). That study was based on a simplified model of the instrument and the measurement process involving a single-pixel focal plane detector, an idealized spectrometer, and continuous sampling of the fringes during the delay scanning. In this paper we elaborate on this ``instrument model'' to include the following additional complications: spectral dispersion of the light with a thin prism, which turns the instrument camera into an objective prism spectrograph; a multiple-pixel detector in the camera focal plane; and, binning of the fringe signal during scanning of the delay. The results obtained with this improved model differ in small but systematic ways from those obtained with the…
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