TL;DR
This paper introduces a novel simulation-based inference framework using 3D convolutional neural networks to estimate galaxy cluster masses from their phase-space distribution, effectively handling uncertainties and interlopers.
Contribution
It is the first to apply machine learning with simulation-based inference to utilize full 3D phase-space data for dynamical mass estimation of galaxy clusters.
Findings
Achieved consistent mass estimates for ~800 SDSS galaxy clusters.
Demonstrated robustness of the method against interloper contamination.
Quantified uncertainties in mass estimates effectively.
Abstract
We present a simulation-based inference framework using a convolutional neural network to infer dynamical masses of galaxy clusters from their observed 3D projected phase-space distribution, which consists of the projected galaxy positions in the sky and their line-of-sight velocities. By formulating the mass estimation problem within this simulation-based inference framework, we are able to quantify the uncertainties on the inferred masses in a straightforward and robust way. We generate a realistic mock catalogue emulating the Sloan Digital Sky Survey (SDSS) Legacy spectroscopic observations (the main galaxy sample) for redshifts and explicitly illustrate the challenges posed by interloper (non-member) galaxies for cluster mass estimation from actual observations. Our approach constitutes the first optimal machine learning-based exploitation of the information…
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