TL;DR
This paper introduces a multimodal machine learning approach that significantly improves the accuracy of photometric redshift estimation for quasars by leveraging spectral features learned from photometric data, outperforming single-modal methods.
Contribution
The paper presents a novel multimodal learning framework combining feature transformation and transfer learning to enhance quasar redshift predictions from photometric data.
Findings
Achieved a 4.04% increase in prediction accuracy.
84.45% of test samples had |Δz|<0.1 with the proposed method.
Reduced RMS of |Δz| from 0.1332 to 0.1235.
Abstract
We propose a Multimodal Machine Learning method for estimating the Photometric Redshifts of quasars (PhotoRedshift-MML for short), which has long been the subject of many investigations. Our method includes two main models, i.e. the feature transformation model by multimodal representation learning, and the photometric redshift estimation model by multimodal transfer learning. The prediction accuracy of the photometric redshift was significantly improved owing to the large amount of information offered by the generated spectral features learned from photometric data via the MML. A total of 415,930 quasars from Sloan Digital Sky Survey (SDSS) Data Release 17, with redshifts between 1 and 5, were screened for our experiments. We used |{\Delta}z| = |(z_phot-z_spec)/(1+z_spec)| to evaluate the redshift prediction and demonstrated a 4.04% increase in accuracy. With the help of the generated…
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