arXiv · 2608.03356
Pixel-Level Calibration for Space-Based High Precision Astrometry Using Young's Fringes
Abstract
The detection of Earth-like exoplanets via astrometry necessitates centroiding precision at the 0.3 microarcsec level, thereby imposing stringent constraints on the focal plane geometry of space telescopes. The AGATE focal plane instrument, a proposed component of the NASA Habitable Worlds Observatory (HWO), aims to achieve this objective through the calibration of the intra-pixel response function of CMOS detectors to an accuracy of 50 micropixel (220 nm The present paper proposes a Young's fringes-based calibration method, derived from those employed by JPL and IPAG, for the purpose of mapping the pixel response barycenter offsets across the detector. Using a Pyxalis GIGAPYX-4600 CMOS sensor, we demonstrate via simulations and laboratory measurements that (1) a precision of 500 micropixel is achievable with 10,000 frames (current setup); (2) inter-pixel capacitance crosstalk and fringe hyperbolicity are dominating the errors at small and large scales, respectively; and, (3) an iterative inverse problem approach with a hyperbolic fringe model is proposed to overcome paraxial approximation limits for 1 Gpix focal planes. These results pave the way for on-board calibration of HWO's astrometric instrument, ensuring the sub-microarcsec precision required for exo-Earth detection.
Explore related subjects
Keep this discovery
Hugo Rousset, Eric Thiébaut, Chloé Rey, Manon Lizzana, Sébastien Soler, Fabrice Pancher, Julien Michelot, Logi Olgeirsson, Jean Baptiste Le Bouquin, Alain Léger, Fabien Malbet. 2026-08-04. Pixel-Level Calibration for Space-Based High Precision Astrometry Using Young's Fringes. https://arxiv.org/abs/2608.03356
Cite the original work for its findings. Save a collection to share your selection of sources.