Galaxy Distribution Incompleteness Testing Using Self-Organizing Maps
Isaac McMahon, Markus Michael Rau, Rachel Mandelbaum

TL;DR
This paper investigates how spectroscopic survey selection functions bias photometric redshift estimates, using self-organizing maps and simulations to evaluate calibration methods and their limitations.
Contribution
It introduces a local calibration testing approach with self-organizing maps to analyze the impact of selection functions on redshift inference and assesses bias mitigation techniques.
Findings
Removing underpopulated regions does not fully eliminate calibration biases.
Selection functions significantly affect redshift inference accuracy.
Bias correction methods need further development for effective mitigation.
Abstract
The calibration of redshift distributions for photometric samples using spectroscopic surveys is plagued by the difficulty in modelling the selection functions of spectroscopic surveys. In this work, we analyse how these selection functions impact redshift inference and quantify the induced biases using local calibration tests in photometry space. The study is carried out using simulations that mimic the radial selection function of a spectroscopic survey and an accompanying mock catalog of a photometric galaxy survey catalog. We use a self-organizing map to partition the photometry space and perform a local test to study the probability calibration of redshift inferences that use the spectroscopic data for calibration. The goal of this work is to investigate the effect of uncorrected selection functions in the calibration data on redshift prediction accuracy and critically…
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Taxonomy
TopicsImpact of Light on Environment and Health · Advanced Statistical Methods and Models · Spectroscopy and Chemometric Analyses
