Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-19T12:25:38.470Z Has data issue: false hasContentIssue false

ELM-KNN for photometric redshift estimation of quasars

Published online by Cambridge University Press:  30 May 2017

Yanxia Zhang
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, P.R.China email: [email protected]
Yang Tu
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, P.R.China email: [email protected] College of Science, China Three Gorges University, Yichang, Hubei, P.R.China
Yongheng Zhao
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, P.R.China email: [email protected]
Haijun Tian
Affiliation:
College of Science, China Three Gorges University, Yichang, Hubei, P.R.China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We explore photometric redshift estimation of quasars with the SDSS DR12 quasar sample. Firstly the quasar sample is separated into three parts according to different redshift ranges. Then three classifiers based on Extreme Learning Machine (ELM) are created in the three redshift ranges. Finally k-Nearest Neighbor (kNN) approach is applied on the three samples to predict photometric redshifts of quasars with multiwavelength photometric data. We compare the performance with different input patterns by ELM-KNN with that only by kNN. The experimental results show that ELM-KNN is feasible and superior to kNN (e.g. rms is 0.0751 vs. 0.2626 for SDSS sample), in other words, the ensemble method has the potential to increase regressor performance beyond the level reached by an individual regressor alone and will be a good choice when facing much more complex data.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Brescia, M., Cavuoti, S., D’Abrusco, R., Longo, G., & Mercurio, A. 2013, ApJ, 772 (2), 140 Google Scholar
Han, B., Ding, H.-P., Zhang, Y.-X., & Zhao, Y.-H. 2016, RAA, 16 (5), 74 Google Scholar
Huang, G.-B., 2015, Cogn Comput, 7, 263 Google Scholar
Huang, G.-B., Zhu, Q.-Y., & Siew, C.-K. 2006, Neurocomputing, 70, 489 Google Scholar
Paris, I., Petitjean, P., Ross, N. P., et al. 2016, arXiv e-print, arXiv:1608.06483Google Scholar
Wu, X.-B. & Jia, Z.-D., 2010, MNRAS, 406, 1583 Google Scholar
Zhang, Y., Ma, H., Peng, N., Zhao, Y., & Wu, X. 2013, AJ, 146, 22 Google Scholar