Machine Learning Classification to Identify Catastrophic Outlier Photometric Redshift Estimates
arXiv:2112.07811 · doi:10.3847/1538-4357/ac53b5
Abstract
We present results of using a basic binary classification neural network model to identify likely catastrophic outlier photometric redshift estimates of individual galaxies, based only on the galaxies' measured photometric band magnitude values. We find that a simple implementation of this classification can identify a significant fraction of galaxies with catastrophic outlier photometric redshift estimates while falsely categorizing only a much smaller fraction of non-outliers. These methods have the potential to reduce the errors introduced into science analyses by catastrophic outlier photometric redshift estimates.
arXiv comment7 pages, 2 figure blocks. Updated to ApJ accepted version
References in corpus (16)
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
- PHAT: PHoto-z Accuracy Testing
- Catastrophic photometric redshift errors: weak lensing survey requirements
- A Sparse Gaussian Process Framework for Photometric Redshift Estimation
- Photometric Redshifts with the LSST: Evaluating Survey Observing Strategies
- A General Study of the Influence of Catastrophic Photometric Redshift Errors on Cosmology with Cosmic Shear Tomography
- Morpho-z: improving photometric redshifts with galaxy morphology
- Analysis of a Custom Support Vector Machine for Photometric Redshift Estimation and the Inclusion of Galaxy Shape Information
- Improved Photometric Redshifts via Enhanced Estimates of System Response, Galaxy Templates, and Magnitude Priors
- Augmenting machine learning photometric redshifts with Gaussian mixture models
- SuperNova Acceleration Probe (SNAP): Investigating Photometric Redshift Optimization
- Photometric Redshifts and Signal-to-Noise
- Cosmology Requirements on Supernova Photometric Redshift Systematics for Rubin LSST and Roman Space Telescope
- Improving Photometric Redshift Estimation for Cosmology with LSST using Bayesian Neural Networks