Building the analytical response in frequency domain of AC biased bolometers Application to Planck/HFI
Alexandre Sauv\'e, Ludovic Montier

TL;DR
This paper develops a physics-based analytical transfer function in frequency domain for AC biased bolometers, improving calibration and response modeling for astronomical instruments like Planck/HFI.
Contribution
It introduces a novel analytical model of bolometer response based on physical principles, replacing previous ad-hoc models, and validated through simulations.
Findings
Analytical transfer function suitable for calibration.
Model constrains optical transfer function fitting.
Improves ADC nonlinearity correction for varying signals.
Abstract
Context: Bolometers are high sensitivity detector commonly used in Infrared astronomy. The HFI instrument of the Planck satellite makes extensive use of them, but after the satellite launch two electronic related problems revealed critical. First an unexpected excess response of detectors at low optical excitation frequency for {\nu} < 1 Hz, and secondly the Analog To digital Converter (ADC) component had been insufficiently characterized on-ground. These two problems require an exquisite knowledge of detector response. However bolometers have highly nonlinear characteristics, coming from their electrical and thermal coupling making them very difficult to modelize. Goal: We present a method to build the analytical transfer function in frequency domain which describe the voltage response of an Alternative Current (AC) biased bolometer to optical excitation, based on the standard…
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