Methods for robustly measuring the minimum spanning tree and other field level statistics from galaxy surveys
Krishna Naidoo, Ofer Lahav

TL;DR
This paper introduces a novel Monte Carlo subsampling and jittering method to mitigate survey systematic effects in galaxy surveys, enabling more efficient and direct measurement of field level statistics like the MST for cosmological parameter inference.
Contribution
The authors propose a new inversion technique that reduces reliance on computationally intensive forward modelling by addressing survey systematics through Monte Carlo subsampling and jittering.
Findings
Jittering effectively masks small scale uncertainties and survey systematics.
Monte Carlo subsampling removes survey selection effects.
Method simplifies measurement of field level statistics from galaxy surveys.
Abstract
Field level statistics, such as the minimum spanning tree (MST), have been shown to be a promising tool for parameter inference in cosmology. However, applications to real galaxy surveys are challenging, due to the presence of small scale systematic effects and non-trivial survey selection functions. Since many field level statistics are 'hard-wired', the common practice is to forward model survey systematic effects to synthetic galaxy catalogues. However, this can be computationally demanding and produces results that are a product of cosmology and systematic effects, making it difficult to directly compare results from different experiments. We introduce a method for inverting survey systematic effects through a Monte Carlo subsampling technique where galaxies are assigned probabilities based on their galaxy weight and survey selection functions. Small scale systematic effects are…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
