Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
Irene Moskowitz, Eric Gawiser, Abby Bault, Adam Broussard, Jeffrey A., Newman, Joe Zuntz, the LSST Dark Energy Science Collaboration

TL;DR
This paper introduces a neural network-based method to optimize tomographic binning in galaxy surveys, improving dark energy constraints by selectively removing galaxies with unreliable redshift estimates.
Contribution
It proposes a neural network classifier to enhance tomographic binning and optimize redshift bin edges, leading to improved dark energy figure of merit in galaxy survey analyses.
Findings
Neural network classifier improves figure of merit by ~13%.
Selective removal of poor redshift estimates recovers ~25% of the loss.
Optimal binning by comoving distance yields the highest dark energy constraints.
Abstract
Large imaging surveys, such as the Legacy Survey of Space and Time, rely on photometric redshifts and tomographic binning for 3x2pt analyses that combine galaxy clustering and weak lensing. In this paper, we propose a method for optimizing the tomographic binning choice for the lens sample of galaxies. We divide the CosmoDC2 and Buzzard simulated galaxy catalogs into a training set and an application set, where the training set is nonrepresentative in a realistic way, and then estimate photometric redshifts for the application sets. The galaxies are sorted into redshift bins covering equal intervals of redshift or comoving distance, or with an equal number of galaxies in each bin, and we consider a generalized extension of these approaches. We find that bins of equal comoving distance produce the highest dark energy figure of merit of the initial binning choices, but that the choice of…
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Taxonomy
TopicsAdvanced Vision and Imaging · Galaxies: Formation, Evolution, Phenomena · CCD and CMOS Imaging Sensors
