Inverting Fisher biases for fast systematics exploration
Biancamaria Sersante, Christos Georgiou, Nora Elisa Chisari

TL;DR
This paper presents a novel application of the Fisher matrix formalism to quickly assess whether unmodelled systematic effects can explain discrepancies between different cosmological measurements.
Contribution
It introduces a method to invert the Fisher matrix process, enabling the investigation of systematic effects' potential to account for observed tensions in data.
Findings
The method accurately estimates small parameter biases caused by systematics.
It is applicable to various systematic effects, demonstrated with galaxy intrinsic alignments and baryonic feedback.
The approach provides a practical tool for bias assessment beyond the linear regime.
Abstract
Upcoming cosmological surveys will achieve increasingly precise constraints in cosmological parameter estimation. To guarantee the robustness of cosmological analyses, it is essential to account for and model systematic effects that can bias cosmological constraints, shifting the best fit parameters away from their fiducial values. It is possible to approximately infer the biases that un-modelled systematic effects might introduce in cosmological parameter estimation by means of the Fisher matrix formalism. In this paper, we introduce a new application of this formalism, where by inverting the process, we investigate whether a specific missing or mis-modelled systematic effect can explain away a given tension between two different probes or experiments. We showcase the proposed methodology by examining two representative systematics: galaxy intrinsic alignments and baryonic feedback. As…
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