Deep learning methods for obtaining photometric redshift estimations from images
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Open Access
- 25 February 2022
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 512 (2) , 1696-1709
Abstract
Knowing the redshift of galaxies is one of the first requirements of many cosmological experiments, and as it is impossible to perform spectroscopy for every galaxy being observed, photometric redshift (photo-z) estimations are still of particular interest. Here, we investigate different deep learning methods for obtaining photo-z estimates directly from images, comparing these with ‘traditional’ machine learning algorithms which make use of magnitudes retrieved through photometry. As well as testing a convolutional neural network (CNN) and inception-module CNN, we introduce a novel mixed-input model that allows for both images and magnitude data to be used in the same model as a way of further improving the estimated redshifts. We also perform benchmarking as a way of demonstrating the performance and scalability of the different algorithms. The data used in the study comes entirely from the Sloan Digital Sky Survey (SDSS) from which 1 million galaxies were used, each having 5-filtre (ugriz) images with complete photometry and a spectroscopic redshift which was taken as the ground truth. The mixed-input inception CNN achieved a mean squared error (MSE) =0.009, which was a significant improvement (|$30{{\ \rm per\ cent}}$|) over the traditional random forest (RF), and the model performed even better at lower redshifts achieving a MSE = 0.0007 (a |$50{{\ \rm per\ cent}}$| improvement over the RF) in the range of z < 0.3. This method could be hugely beneficial to upcoming surveys, such as Euclid and the Vera C. Rubin Observatory’s Legacy Survey of Space and Time (LSST), which will require vast numbers of photo-z estimates produced as quickly and accurately as possible.Keywords
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Funding Information
- STFC (ST/P006736/1, ST/M001334/1, ST/R000476/1)
- European Research Council (TESTDE FP7/291329)
- Alan Turing Institute
- EPSRC (EP/V001310/1)
- Alfred P. Sloan Foundation
- National Science Foundation
- U.S. Department of Energy
- Office of Science
- University of Arizona
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- Harvard University
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
This publication has 32 references indexed in Scilit:
- Comparison of statistical and machine learning methods in modelling of data with multicollinearityInternational Journal of Modelling, Identification and Control, 2013
- The Kilo-Degree SurveyExperimental Astronomy, 2012
- A comparison of six photometric redshift methods applied to 1.5 million luminous red galaxiesMonthly Notices of the Royal Astronomical Society, 2011
- Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep surveyAstronomy & Astrophysics, 2006
- Extremely randomized treesMachine Learning, 2006
- ANNz: Estimating Photometric Redshifts Using Artificial Neural NetworksPublications of the Astronomical Society of the Pacific, 2004
- LSST: a complementary probe of dark energyNuclear Physics B - Proceedings Supplements, 2003
- The Sloan Digital Sky Survey: Technical SummaryThe Astronomical Journal, 2000
- Bayesian Photometric Redshift EstimationThe Astrophysical Journal, 2000
- A logical calculus of the ideas immanent in nervous activityBulletin of Mathematical Biology, 1943