TL;DR
This paper introduces a machine learning approach to derive spectral templates from a large galaxy dataset, significantly improving photometric redshift accuracy by reducing outliers, bias, and scatter compared to traditional templates.
Contribution
We develop a novel training algorithm that learns spectral energy distributions directly from galaxy data, surpassing limitations of existing spectrophotometric and spectral synthesis methods.
Findings
Reduced outlier fraction in redshift estimates by up to 28%
Bias in redshift estimation decreased by up to 91%
Scatter in redshift estimates reduced by up to 25%
Abstract
Estimating redshifts from broadband photometry is often limited by how accurately we can map the colors of galaxies to an underlying spectral template. Current techniques utilize spectrophotometric samples of galaxies or spectra derived from spectral synthesis models. Both of these approaches have their limitations, either the sample sizes are small and often not representative of the diversity of galaxy colors or the model colors can be biased (often as a function of wavelength) which introduces systematics in the derived redshifts. In this paper we learn the underlying spectral energy distributions from an ensemble of 100K galaxies with measured redshifts and colors. We show that we are able to reconstruct emission and absorption lines at a significantly higher resolution than the broadband filters used to measure the photometry for a sample of 20 spectral templates. We find…
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