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.
@article{arxiv.2408.15929,
title = {Challenges in focal plane and telescope calibration for High-Precision Space Astrometry},
author = {F. Malbet and M. Lizzana and F. Pancher and S. Soler and A. Léger and T. Lépine and G. A. Mamon and A. Sozzetti and A. Riva and D. Busonero and L. Labadie and P. -O. Lagage and R. Goullioud},
journal= {arXiv preprint arXiv:2408.15929},
year = {2024}
}
Comments
SPIE Conference "Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave", Yokohama, Japan. arXiv admin note: text overlap with arXiv:2207.12540