GeneticKNN: A Weighted KNN Approach Supported by Genetic Algorithm for Photometric Redshift Estimation of Quasars
arXiv:2009.08608 · doi:10.1088/1674-4527/21/1/17
Abstract
We combine K-Nearest Neighbors (KNN) with genetic algorithm (GA) for photometric redshift estimation of quasars, short for GeneticKNN, which is a weighted KNN approach supported by GA. This approach has two improvements compared to KNN: one is the feature weighted by GA; another is that the predicted redshift is not the redshift average of K neighbors but the weighted average of median and mean of redshifts for K neighbors, i.e. . Based on the SDSS and SDSS-WISE quasar samples, we explore the performance of GeneticKNN for photometric redshift estimation, comparing with the other six traditional machine learning methods, i.e. Least absolute shrinkage and selection operator (LASSO), support vector regression (SVR), Multi Layer Perceptrons (MLP), XGBoost, KNN and random forest. KNN and random forest show their superiority. Considering the easy implementation of KNN, we make improvement on KNN as GeneticKNN and apply GeneticKNN on photometric redshift estimation of quasars. Finally the performance of GeneticKNN is better than that of LASSO, SVR, MLP, XGBoost, KNN and random forest for all cases. Moreover the accuracy is better with the additional WISE magnitudes for the same method.
arXiv comment17 pages, 4 tables, 6 figures
References in corpus (22)
- The Sloan Digital Sky Survey: Technical Summary
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science
- The Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release
- TPZ : Photometric redshift PDFs and ancillary information by using prediction trees and random forests
- Photometric redshifts in the SWIRE Survey
- Photometric redshift estimation via deep learning
- Photometric redshifts and quasar probabilities from a single, data-driven generative model
- ArborZ: Photometric Redshifts Using Boosted Decision Trees
- Photo-z for weak lensing tomography from space: the role of optical and near-IR photometry
- Robust Machine Learning Applied to Astronomical Datasets III: Probabilistic Photometric Redshifts for Galaxies and Quasars in the SDSS and GALEX
- Photometric redshifts for Quasars in multi band Surveys
- Probabilistic selection of high-redshift quasars
- Astroinformatics of galaxies and quasars: a new general method for photometric redshifts estimation
- Bayesian photometric redshifts with empirical training sets
- The Extremely Luminous Quasar Survey (ELQS) in the SDSS footprint I.: Infrared Based Candidate Selection
- Photometric Redshift Estimation Using Spectral Connectivity Analysis
- Can Self-Organizing Maps accurately predict photometric redshifts?
- Data-driven, interpretable photometric redshifts trained on heterogeneous and unrepresentative data
- A new method to improve photometric redshift reconstruction. Applications to the Large Synoptic Survey Telescope
- Color-redshift Relations and Photometric Redshift Estimations of Quasars in Large Sky Surveys
- The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample to r<19.5