YOLO-CL: Galaxy cluster detection in the SDSS with deep machine learning
arXiv:2301.09657 · doi:10.1051/0004-6361/202345976
Abstract
(Abridged) Galaxy clusters are a powerful probe of cosmological models. Next generation large-scale optical and infrared surveys will reach unprecedented depths over large areas and require highly complete and pure cluster catalogs, with a well defined selection function. We have developed a new cluster detection algorithm YOLO-CL, which is a modified version of the state-of-the-art object detection deep convolutional network YOLO, optimized for the detection of galaxy clusters. We trained YOLO-CL on color images of the redMaPPer cluster detections in the SDSS. We find that YOLO-CL detects of the redMaPPer clusters, with a purity of calculated by applying the network to SDSS blank fields. When compared to the MCXC2021 X-ray catalog in the SDSS footprint,YOLO-CL is more complete then redMaPPer, which means that the neural network improved the cluster detection efficiency of its training sample. The YOLO-CL selection function is approximately constant with redshift, with respect to the MCXC2021 cluster mean X-ray surface brightness. YOLO-CL shows high performance when compared to traditional detection algorithms applied to SDSS. Deep learning networks benefit from a strong advantage over traditional galaxy cluster detection techniques because they do not need galaxy photometric and photometric redshift catalogs. This eliminates systematic uncertainties that can be introduced during source detection, and photometry and photometric redshift measurements. Our results show that YOLO-CL is an efficient alternative to traditional cluster detection methods. In general, this work shows that it is worth exploring the performance of deep convolution networks for future cosmological cluster surveys, such as the Rubin/LSST, Euclid or the Roman Space Telescope surveys.
14 pages, 12 fig Ilic co-conceived and developed YOLO-CL, applied it to SDSS images, and produced the plots for the completeness and purity analysis (2019-2021). Grishin reproduced Ilic's work and compared the final YOLO-CL cluster catalog to the other cluster finders (2021-2022). Mei co-conceived YOLO-CL, supervised the work and was the main writer of the paper text
References in corpus (51)
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- Overview of the DESI Legacy Imaging Surveys
- The Simons Observatory: Science goals and forecasts
- Cosmological Parameters from Observations of Galaxy Clusters
- The eROSITA X-ray telescope on SRG
- redMaPPer I: Algorithm and SDSS DR8 Catalog
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue
- A MaxBCG Catalog of 13,823 Galaxy Clusters from the Sloan Digital Sky Survey
- The MCXC: a Meta-Catalogue of X-ray detected Clusters of galaxies
- Cosmological Constraints from the SDSS maxBCG Cluster Catalog
- The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data
- Preparing Red-Green-Blue (RGB) Images from CCD Data
- A catalog of 132,684 clusters of galaxies identified from Sloan Digital Sky Survey III
- The Red-Sequence Cluster Survey I: The Survey and Cluster Catalogs for Patches RCS0926+37 and RCS1327+29
- Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
- The redMaPPer Galaxy Cluster Catalog From DES Science Verification Data
- The Gemini Cluster Astrophysics Spectroscopic Survey (GCLASS): The Role of Environment and Self-Regulation in Galaxy Evolution at z ~ 1
- A GMBCG Galaxy Cluster Catalog of 55,424 Rich Clusters from SDSS DR7
- The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
- A catalog of visual-like morphologies in the 5 CANDELS fields using deep-learning
- Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
- Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer
- Photometric redshifts from SDSS images using a Convolutional Neural Network
- Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
- Galaxy clusters identified from the SDSS DR6 and their properties
- redMaPPer II: X-ray and SZ Performance Benchmarks for the SDSS Catalog
- An Optical Catalog of Galaxy Clusters Obtained from an Adaptive Matched Filter Finder Applied to SDSS DR6
- An optical group catalogue to z = 1 from the zCOSMOS 10k sample
- Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies
- Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
- Measuring the dynamical state of Planck SZ-selected clusters: X-ray peak - BCG offset
- The DAWES review 10: The impact of deep learning for the analysis of galaxy surveys
- Deep Learning Identifies High-z Galaxies in a Central Blue Nugget Phase in a Characteristic Mass Range
- The Galaxy Cluster Mid-Infrared Luminosity Function at 1.3<z<3.2
- A catalog of polychromatic bulge-disk decompositions of ~ 17.600 galaxies in CANDELS
- The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
- Deep learning dark matter map reconstructions from DES SV weak lensing data
- Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
- Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope
- Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative Models
- COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
- Benchmarking and Scalability of Machine Learning Methods for Photometric Redshift Estimation
- Galaxy clusters and groups in the ALHAMBRA Survey
- Euclid preparation: XXII. Selection of Quiescent Galaxies from Mock Photometry using Machine Learning
- [OII] emitters in the GOODS field at z~1.85: a homogeneous measure of evolving star formation
- II. Apples to apples : cluster selection functions for next-generation surveys
- DeepSZ: Identification of Sunyaev-Zel'dovich Galaxy Clusters using Deep Learning
- Deep learning for Sunyaev-Zel'dovich detection in Planck
- Deep-CEE I: Fishing for Galaxy Clusters with Deep Neural Nets
- MILCANN : A neural network assessed tSZ map for galaxy cluster detection
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- YOLO-CIANNA: Galaxy detection with deep learning in radio data. I. A new YOLO-inspired source detection method applied to the SKAO SDC1
- YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
- Using Deep Learning Methods to Detect for Ultra-diffuse Galaxies in KiDS
- Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset