Photometric Redshift Estimation of BASS DR3 Quasars by Machine Learning
Changhua Li, Yanxia Zhang, Chenzhou Cui, Dongwei Fan, Yongheng Zhao,, Xue-Bing Wu, Jing-Yi Zhang, Jun Han, Yunfei Xu, Yihan Tao, Shanshan Li,, Boliang He

TL;DR
This paper develops machine learning models, especially a two-step approach using CatBoost, to accurately estimate photometric redshifts of quasars from BASS DR3, aiding high-redshift quasar identification.
Contribution
It introduces a two-step redshift estimation model with CatBoost, outperforming one-step models for quasars, especially at high redshifts.
Findings
Two-step model with CatBoost yields best performance.
The model predicts 3938 high-redshift quasar candidates.
Two-step approach improves redshift estimation accuracy.
Abstract
Correlating BASS DR3 catalogue with ALLWISE database, the data from optical and infrared information are obtained. The quasars from SDSS are taken as training and test samples while those from LAMOST are considered as external test sample. We propose two schemes to construct the redshift estimation models with XGBoost, CatBoost and Random forest. One scheme (namely one-step model) is to predict photometric redshifts directly based on the optimal models created by these three algorithms; the other scheme (namely two-step model) is to firstly classify the data into low- and high- redshift datasets, and then predict photometric redshifts of these two datasets separately. For one-step model, the performance of these three algorithms on photometric redshift estimation is compared with different training samples, and CatBoost is superior to XGBoost and Random forest. For two-step model, the…
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