Challenges in focal plane and telescope calibration for High-Precision Space Astrometry

Abstract

With sub-microarcsecond angular accuracy, the \theia telescope will be capable of revealing the architectures of nearby exoplanetary systems down to the mass of Earth. This research addresses the challenges inherent in space astrometry missions, focusing on focal plane calibration and telescope optical distortion. We propose to assess the future feasibility of large-format detectors (50 to 200 megapixels) in a controlled laboratory environment. The aim is to improve the architecture of the focal plane while ensuring that specifications are met. The use of field stars as metrological sources for calibrating the optical distortion of the field may help to constrain telescope stability. The paper concludes with an attempt to confirm in the laboratory the performance predicted by simulations. We will also address the possibility of using such techniques with a dedicated instrument for the Habitable World Observatory.

SPIE Conference "Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave", Yokohama, Japan. arXiv admin note: text overlap with arXiv:2207.12540

References in corpus (6)

• The Gaia mission
• Improved GRAVITY astrometric accuracy from modeling of optical aberrations
• The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data
• Theia: Faint objects in motion or the new astrometry frontier
• A detector interferometric calibration experiment for high precision astrometry
• A new estimation of astrometric exoplanet detection limits in the habitable zone around nearby stars