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Astrometry exoplanet detection using the Habex Workhorse camera

Paper Abstract

Accurate measurement of exoplanetary masses is a critical step in addressing key aspects of NASA’s science vision. Astrometry can detect and measure masses of planets orbiting the target star. However, the signal for earth-analogs is in the sub-microarcsecond regime, well beyond our instrumentation. In this paper, we study part of an astrometry error budget for the HabEx Workhorse Camera and we propose a calibration approach to reach earth-analog sensitivity.

Paper Details

Date Published: 1 August 2021
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Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 1182317 (1 August 2021); doi: 10.1117/12.2594996
Show Author Affiliations
Eduardo A. Bendek, Jet Propulsion Lab. (United States)
Stefan Martin, Jet Propulsion Lab. (United States)
Olivier Guyon, The Univ. of Arizona (United States)


Published in SPIE Proceedings Vol. 11823:
Techniques and Instrumentation for Detection of Exoplanets X
Stuart B. Shaklan; Garreth J. Ruane, Editor(s)

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