Deep learning predictions of galaxy merger stage and the importance of observational realism
arXiv:1910.07031 · doi:10.1093/mnras/stz2934
Abstract
Machine learning is becoming a popular tool to quantify galaxy morphologies and identify mergers. However, this technique relies on using an appropriate set of training data to be successful. By combining hydrodynamical simulations, synthetic observations and convolutional neural networks (CNNs), we quantitatively assess how realistic simulated galaxy images must be in order to reliably classify mergers. Specifically, we compare the performance of CNNs trained with two types of galaxy images, stellar maps and dust-inclusive radiatively transferred images, each with three levels of observational realism: (1) no observational effects (idealized images), (2) realistic sky and point spread function (semi-realistic images), (3) insertion into a real sky image (fully realistic images). We find that networks trained on either idealized or semi-real images have poor performance when applied to survey-realistic images. In contrast, networks trained on fully realistic images achieve 87.1% classification performance. Importantly, the level of realism in the training images is much more important than whether the images included radiative transfer, or simply used the stellar maps (87.1% compared to 79.6% accuracy, respectively). Therefore, one can avoid the large computational and storage cost of running radiative transfer with a relatively modest compromise in classification performance. Making photometry-based networks insensitive to colour incurs a very mild penalty to performance with survey-realistic data (86.0% with r-only compared to 87.1% with gri). This result demonstrates that while colour can be exploited by colour-sensitive networks, it is not necessary to achieve high accuracy and so can be avoided if desired. We provide the public release of our statistical observational realism suite, RealSim, as a companion to this paper.
MNRAS accepted. 25 pages, 15 figures, 4 tables. RealSim: https://github.com/cbottrell/RealSim
References in corpus (40)
- Multi-messenger Observations of a Binary Neutron Star Merger
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
- Rotation-invariant convolutional neural networks for galaxy morphology prediction
- A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
- Galaxy Pairs in the Sloan Digital Sky Survey I: Star Formation, AGN Fraction, and the Luminosity/Mass-Metallicity Relation
- The effect of galaxy mass ratio on merger--driven starbursts
- Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
- SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly Architecture
- Sunrise: Polychromatic Dust Radiative Transfer in Arbitrary Geometries
- Fast Automated Analysis of Strong Gravitational Lenses with Convolutional Neural Networks
- Molecular and atomic gas along and across the main sequence of star-forming galaxies
- Galaxy pairs in the Sloan Digital Sky Survey - IX: Merger-induced AGN activity as traced by the Wide-field Infrared Survey Explorer
- Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: IV The Controlling Parameters of the Starburst SED
- Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey
- A definitive merger-AGN connection at z~0 with CFIS: mergers have an excess of AGN and AGN hosts are more frequently disturbed
- Merging and Clustering of the Swift BAT AGN Sample
- Galaxy And Mass Assembly (GAMA): Galaxy close-pairs, mergers, and the future fate of stellar mass
- On the possible environmental effect in distributing heavy elements beyond individual gaseous halos
- Mapping galaxy encounters in numerical simulations: The spatial extent of induced star formation
- Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
- The Luminosity Dependence of the Galaxy Merger Rate
- Interacting galaxies on FIRE-2: The connection between enhanced star formation and interstellar gas content
- The Spitzer Spirals, Bridges, and Tails Interacting Galaxy Survey: Interaction-Induced Star Formation in the Mid-Infrared
- AEGIS: Enhancement of Dust-enshrouded Star Formation in Close Galaxy Pairs and Merging Galaxies up to z ~ 1
- Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELS
- Galaxy And Mass Assembly (GAMA): Refining the Local Galaxy Merger Rate using Morphological Information
- Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
- Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
- On the lifetime of merger features of equal-mass disk mergers
- The VIMOS VLT Deep Survey: the contribution of minor mergers to the growth of L_B >= L*_B galaxies since z ~ 1 from spectroscopically identified pairs
- Galaxy pairs in the Sloan Digital Sky Survey - XII: The fuelling mechanism of low excitation radio-loud AGN
- What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
- Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
- Bulge plus disc and Sérsic decomposition catalogues for 16,908 galaxies in the SDSS Stripe 82 co-adds: A detailed study of the structural measurements
- Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
- The Molecular Wind in the Nearest Seyfert Galaxy Circinus Revealed by ALMA
- A New Public Release of the GIZMO Code
Cited by in corpus (68)
- The DAWES review 10: The impact of deep learning for the analysis of galaxy surveys
- Galaxy Merger Rates up to z 3 using a Bayesian Deep Learning Model A Major-Merger classifier using IllustrisTNG Simulation data
- Convolutional neural network identification of galaxy post-mergers in UNIONS using IllustrisTNG
- Galaxy mergers can rapidly shut down star formation
- Galaxy Morphological Classification Catalogue of the Dark Energy Survey Year 3 data with Convolutional Neural Networks
- IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
- The merger fraction of post-starburst galaxies in UNIONS
- Characterization of Low Surface Brightness structures in annotated deep images
- DeepMerge II: Building Robust Deep Learning Algorithms for Merging Galaxy Identification Across Domains
- ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
- Galaxy pairs in the Sloan Digital Sky Survey -- XIV. Galaxy mergers do not lie on the Fundamental Metallicity Relation
- Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
- Star formation characteristics of CNN-identified post-mergers in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
- Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
- Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
- North Ecliptic Pole merging galaxy catalogue
- The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
- Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
- Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks
- AGN in post-mergers from the Ultraviolet Near Infrared Optical Northern Survey
- Stellar Populations With Optical Spectra: Deep Learning vs. Popular Spectrum Fitting Codes
- An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs
- Accurate Identification of Galaxy Mergers with Stellar Kinematics
- Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
- A re-assessment of strong line metallicity conversions in the machine learning era
- The observability of galaxy merger signatures in nearby gas-rich spirals
- A complete catalogue of merger fractions in AGN hosts: No evidence for an increase in detected merger fraction with AGN luminosity
- The galaxy morphology-density relation in the EAGLE simulation
- Mapping the Diversity of Galaxy Spectra with Deep Unsupervised Machine Learning
- Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
- Realistic synthetic integral field spectroscopy with RealSim-IFS
- Galaxy merger challenge: A comparison study between machine learning-based detection methods
- Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples
- Molecular gas and star formation in nearby starburst galaxy mergers
- ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
- ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
- A 3.8yr optical quasi-periodic oscillations in blue quasar SDSS J132144+033055 through combined light curves from CSS and ZTF
- Gaussian Process Classification for Galaxy Blend Identification in LSST
- Identification of Grand-design and Flocculent Spirals from SDSS using Convolutional Neural network
- Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks
- Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
- Machine learning the gap between real and simulated nebulae: A domain-adaptation approach to classify ionised nebulae in nearby galaxies
- Cosmology with Galaxy Cluster Properties using Machine Learning
- An astronomical image content-based recommendation system using combined deep learning models in a fully unsupervised mode
- Machine learning technique for morphological classification of galaxies from the SDSS. III. Image-based inference of detailed features
- Merger identification through photometric bands, colours, and their errors
- A candidate of binary black hole system in AGN with broad Balmer emission lines having quite different line widths
- Machine learning technique for morphological classification of galaxies from SDSS. II. The image-based morphological catalogs of galaxies at 0.02<z<0.1
- SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
- Halo Growth and Merger Rates as a Cosmological Test
- Harnessing the Hubble Space Telescope Archives: A Catalogue of 21,926 Interacting Galaxies
- Determining the time before or after a galaxy merger event
- A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
- Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
- Total and dark mass from observations of galaxy centers with Machine Learning
- IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
- GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
- Harvesting the Lyα forest with convolutional neural networks
- AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
- Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
- A machine learning approach to assessing the presence of substructure in quasar host galaxies using the Hyper Suprime-Cam Subaru Strategic Program
- Quantitatively rating galaxy simulations against real observations with anomaly detection
- The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
- DeepMerge: Classifying High-redshift Merging Galaxies with Deep Neural Networks
- Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
- The major merger-active galactic nucleus connection up to the cosmic noon
- A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
- Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam