Review of detector requirements: some challenges for the present
arXiv:2405.14955 · doi:10.1117/1.JATIS.11.1.011207
Abstract
Astrophysics demands higher precision in measurements across photometry, spectroscopy, and astrometry. Several science cases necessitate not only precision but also a high level of accuracy. We highlight the challenges involved, particularly in achieving spectral fidelity, which refers to our ability to accurately replicate the input spectrum of an astrophysical source. Beyond wavelength calibration, this encompasses correcting observed spectra for atmospheric, telescope, and instrumental signatures. Elevating spectral fidelity opens avenues for addressing fundamental questions in physics and astrophysics. We delve into specific science cases, critically analyzing the prerequisites for conducting crucial observations. Special attention is given to the requirements for spectrograph detectors, their calibrations and data reduction. Importantly, these considerations align closely with the needs of photometry and astrometry.
Published in Journal of Astronomical Telescopes, Instruments, and Systems (JATIS). Based on the contribution to the conference Image Sensors for Precision Astronomy 2024
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