Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey
arXiv:0804.4483 · doi:10.1111/j.1365-2966.2008.13689.x
Abstract
In order to understand the formation and subsequent evolution of galaxies one must first distinguish between the two main morphological classes of massive systems: spirals and early-type systems. This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS). This achievement was made possible by inviting the general public to visually inspect and classify these galaxies via the internet. The project has obtained more than 40,000,000 individual classifications made by ~100,000 participants. We discuss the motivation and strategy for this project, and detail how the classifications were performed and processed. We find that Galaxy Zoo results are consistent with those for subsets of SDSS galaxies classified by professional astronomers, thus demonstrating that our data provides a robust morphological catalogue. Obtaining morphologies by direct visual inspection avoids introducing biases associated with proxies for morphology such as colour, concentration or structual parameters. In addition, this catalogue can be used to directly compare SDSS morphologies with older data sets. The colour--magnitude diagrams for each morphological class are shown, and we illustrate how these distributions differ from those inferred using colour alone as a proxy for morphology.
Submitted to MNRAS
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- Galaxy classification: a deep learning approach for classifying Sloan Digital Sky Survey images
- Recent Star-Forming Activity in Local Elliptical Galaxies
- Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array
- Towards an Understanding of the Massive Red Spiral Galaxy Formation
- Twelve Years of Galaxy Zoo
- NoSOCS in SDSS. V. Red Disc and Blue Bulge Galaxies Across Different Environments
- Gradient Pattern Analysis Applied to Galaxy Morphology
- The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1
- Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?
- WALLABY Pilot Survey: the Potential Polar Ring Galaxies NGC~4632 and NGC~6156
- Why do many early-type galaxies lack emission lines? I. Fossil clues
- A declining major merger fraction with redshift in the local Universe from the largest-yet catalog of major and minor mergers in SDSS
- Considering Human Aspects on Strategies for Designing and Managing Distributed Human Computation
- First results from the LUCID-Timepix spacecraft payload onboard the TechDemoSat-1 satellite in Low Earth Orbit
- A preliminary reconstruction of the orbit of the Chelyabinsk Meteoroid
- A SLUGGS and Gemini/GMOS combined study of the elliptical galaxy M60: wide-field photometry and kinematics of the globular cluster system
- The Evolutionary Sequence of Post-Starburst Galaxies
- Planet Hunters TESS IV: A massive, compact hierarchical triple star system TIC 470710327
- Unsupervised Galaxy Morphological Visual Representation with Deep Contrastive Learning
- The Importance Of Star Formation Intensity In LYα Escape From Green Pea Galaxies And Lyman Break Galaxy Analogs
- SDSS-IV MaNGA: Signatures of halo assembly in kinematically misaligned galaxies
- Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
- The impact from survey depth and resolution on the morphological classification of galaxies
- Polar Ring Galaxies in the Galaxy Zoo
- Radio Detection of Green Peas: Implications for Magnetic Fields in Young Galaxies
- Quantified HI Morphology IV: The Merger Fraction and Rate in WHISP
- HI Content and Optical Properties of Field Galaxies from the ALFALFA Survey. I.Selection of a Control Sample
- Planet Four: Probing Springtime Winds on Mars by Mapping the Southern Polar CO Jet Deposits
- Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
- Optical, near-IR and sub-mm IFU Observations of the nearby dual AGN Mrk 463
- Morphology and the Color-Mass Diagram as Clues to Galaxy Evolution at z~1
- The evolution of pitch angles of spiral arms
- PSFGAN: a generative adversarial network system for separating quasar point sources and host galaxy light
- New candidates to polar-ring galaxies from the Sloan Digital Sky Survey
- A study on the statistical significance of mutual information between morphology of a galaxy and its large-scale environment
- Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
- Quantitative analysis of spirality in elliptical galaxies
- The frequency of dust lanes in edge-on spiral galaxies identified by Galaxy Zoo in KiDS imaging of GAMA targets
- The observability of galaxy merger signatures in nearby gas-rich spirals
- A Robust Study of High-Redshift Galaxies: Unsupervised Machine Learning for Characterising morphology with JWST up to z ~ 8
- Observational Tracking of the 2D Structure of Coronal Mass Ejections Between the Sun and 1 AU
- The Moon Zoo citizen science project: Preliminary results for the Apollo 17 landing site
- The AGN contribution to the UV-FIR luminosities of interacting galaxies and its role in identifying the Main Sequence
- Morphological Segregation in the Surroundings of Cosmic Voids
- Galaxy And Mass Assembly (GAMA) Blended Spectra Catalog: Strong Galaxy-Galaxy Lens and Occulting Galaxy Pair Candidates
- Automated Lensing Learner: Automated Strong Lensing Identification with a Computer Vision Technique
- Galaxy Zoo Builder: Morphological Dependence of Spiral Galaxy Pitch Angle
- Galaxy morphology prediction using capsule networks
- Identifying the progenitor set of present-day early-type galaxies: a view from the standard model
- K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists
- Two Candidates for Dual AGN in Dwarf-Dwarf Galaxy Mergers
- Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
- Measuring the X-shaped structures in edge-on galaxies
- VLT/VIMOS Observations of an Occulting Galaxy Pair: Redshifts and Effective Extinction Curve
- Induced nuclear activity in galaxy pairs with different morphologies (E+E), (E+S) and (S+S)
- On the HI Content of MaNGA Major Merger Pairs
- Machine Learning for Galaxy Morphology Classification
- The Edge-on Galaxies in the Pan-STARRS survey (EGIPS)
- Multiband galaxy morphologies for CLASH: a convolutional neural network transferred from CANDELS
- Deciphering the Large-Scale Environment of Radio Galaxies in the Local Universe II. A Statistical Analysis of Environmental Properties
- IRAC Near-Infrared Features in the Outer Parts of S4G Galaxies
- GWitchHunters: Machine Learning and citizen science to improve the performance of Gravitational Wave detector
- Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
- Joint NuSTAR and Chandra analysis of the obscured quasar in IC 2497 - Hanny's Voorwerp system
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- The Revolution in Astronomy Education: Data Science for the Masses
- Clues on the history of early-type galaxies from SDSS spectra and GALEX photometry
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- AGN luminosity and stellar age -- two missing ingredients for AGN unification as seen with iPTF supernovae
- The Effect of Minor and Major Mergers on the Evolution of Low Excitation Radio Galaxies
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- A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local Universe
- Galaxy morphologies at cosmic noon with JWST: A foundation for exploring gas transport with bars and spiral arms
- Automatic detection of peculiar galaxy pairs in Sloan Digital Sky Survey
- The Impact of Redshift on Galaxy Morphometric Classification: case studies for SDSS, DES, LSST and HST with Morfometryka
- Observational search for primordial chirality violations using galaxy angular momenta
- AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: mid-infrared view of transition galaxies
- Astronomaly at scale: searching for anomalies amongst 4 million galaxies
- The Milky Way Project: What are Yellowballs?
- The similar stellar populations of quiescent spiral and elliptical galaxies
- Crowdsourcing Predictors of Residential Electric Energy Usage
- A catalog of broad morphology of Pan-STARRS galaxies based on deep learning
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- A Study of Environmental Effects on Galaxy Spin Using MaNGA Data
- The Ultraviolet Attenuation Law in Backlit Spiral Galaxies
- Gas accretion as fuel for residual star formation in Galaxy Zoo elliptical galaxies
- Quenching depends on morphologies: implications from the ultraviolet-optical radial color distributions in Green Valley Galaxies
- Active galactic nuclei ghosts: A systematic search for faded nuclei
- The host galaxies of luminous type 2 AGN at 0.3-0.4
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- Euclid preparation. XLIII. Measuring detailed galaxy morphologies for Euclid with machine learning
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- DAWN JWST Archive: Morphology from profile fitting of over 340 000 galaxies in major fields
- Gems of the Galaxy Zoos -- a Wide-Ranging Hubble Space Telescope Gap-Filler Program
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- Data Challenges for Next-generation Radio Telescopes
- The Discovery of a Low-Luminosity SPIRAL DRAGN
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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
- The orientation of galaxy pairs with filamentary structures: dependence on morphology
- Merger Signatures are Common, but not Universal, In Massive, Recently-Quenched Galaxies at z~0.7
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- Star formation and morphological properties of galaxies in the Pan-STARRS survey- I. A machine learning approach to galaxy and supernova classification
- CANDELS Meets GSWLC: Evolution of the Relationship Between Morphology and Star Formation Since z = 2
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- Deep Learning Assessment of galaxy morphology in S-PLUS DataRelease 1
- Quantifying the fine structures of disk galaxies with deep learning:Segmentation of spiral arms in different Hubble types
- What distinguishes the host galaxies of radio-loud and radio-quiet AGNs?
- Spatially Resolved Galaxy Star Formation and its Environmental Dependence II. Effect of the Morphology-Density Relation
- Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo
- Morphological Classification of Radio Galaxies with wGAN-supported Augmentation
- SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sample
- The H Dots Survey. II. A Second List of Faint Emission-Line Objects
- Host galaxy and orientation differences between AGN different types
- The Systematics of Galaxy Morphology in the Comprehensive de Vaucouleurs revised Hubble-Sandage Classification System: Application to the EFIGI Sample
- Detection of Strongly Lensed Arcs in Galaxy Clusters with Transformers
- GaMPEN: A Machine Learning Framework for Estimating Bayesian Posteriors of Galaxy Morphological Parameters
- Relic jet activity in "Hanny's Voorwerp" revealed by the LOFAR Two metre Sky Survey
- Green valley galaxies in the cosmic web: internal versus environmental quenching
- A More Efficient Search for H2O Megamaser Galaxies : The Power of the X-ray and Mid-infrared Photometry
- Galaxy Pairs in the Sloan Digital Sky Survey XV: Properties of Ionised Outflows
- The incidence of AGN in galaxies with different stellar population ages
- Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
- Morphology of Seyfert Galaxies
- The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
- Bursts from Space: MeerKAT - The first citizen science project dedicated to commensal radio transients
- Diagnostic diagrams for ram-pressure stripped candidates
- The TESS Triple-9 Catalog II: a new set of 999 uniformly-vetted exoplanet candidates
- A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z 0.4
- Identification of Grand-design and Flocculent Spirals from SDSS using Convolutional Neural network
- The TELPERION Survey for Distant [O III] Clouds around Luminous and Hibernating AGN
- Classification and Evolution of Galaxies According to the Dynamical State of Host Clusters and Galaxy Luminosities
- AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
- SDSS-IV MaNGA: The [/Fe] of Early-Type Galaxies
- Misalignment between cold gas and stellar components in early-type galaxies
- On the triggering of extreme starburst events in low-metallicity galaxies: a deep search for companions of Green Peas
- A Bayesian Approach to Strong Lens Finding in the Era of Wide-area Surveys
- Lessons Learned from the Two Largest Galaxy Morphological Classification Catalogues built by Convolutional Neural Networks
- Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
- Do galactic bars depend on environment?: An information theoretic analysis of Galaxy Zoo 2
- Planet Hunters TESS III: two transiting planets around the bright G dwarf HD 152843
- Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies
- EXSdetect: an end-to-end software for extended source detection in X-ray images: application to Swift-XRT data
- Core-collapse Supernovae in the Dark Energy Survey: Luminosity Functions and Host Galaxy Demographics
- Shocked POststarburst Galaxy Survey. III. The Ultraviolet Properties of SPOGs
- Close Major Merger Pairs at : Bulge-to-Total Ratio and Star Formation Enhancement
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- Non-Parametric Cell-Based Photometric Proxies for Galaxy Morphology: Methodology and Application to the Morphologically-Defined Star Formation -- Stellar Mass Relation of Spiral Galaxies in the Local Universe
- Labeling Bias in Galaxy Morphologies
- Reanalysis of the spin direction distribution of Galaxy Zoo SDSS spiral galaxies
- An old stellar population or diffuse nebular continuum emission discovered in green pea galaxies
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- The effects of environment on the intrinsic shape of galaxies
- Chandra X-ray observations of the hyper-luminous infrared galaxy IRAS F15307+3252
- An empirical consistent redshift bias: A possible direct reproducible observation of Zwicky's TL theory
- Dissecting the morphological and spectroscopic properties of galaxies in the local Universe: I. Elliptical galaxies
- Distortion of Infall Regions in Redshift Space-I
- Can a conditioning on stellar mass explain the mutual information between morphology and environment?
- On the origin of red spirals: Does assembly bias play a role?
- SDSS-IV MaNGA: When is morphology imprinted on galaxies?
- HI Imaging of a Blueberry Galaxy Suggests a Merger Origin
- Discovery of a near-infrared bar and a pseudobulge in the collisional ring galaxy Cartwheel
- A Comparison of Deep Learning Architectures for Optical Galaxy Morphology Classification
- How much dark matter is there inside early-type galaxies?
- Interface Design for Crowdsourcing Hierarchical Multi-Label Text Annotations
- Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence
- The impact of low luminosity AGN on their host galaxies: A radio and optical investigation of the kpc-scale outflow in MaNGA 1-166919
- Investigation of the parameters of spiral pattern in galaxies: the arm width
- Estimating densities with nonlinear support using Fisher-Gaussian kernels
- An [O III] search for extended emission around AGN with H I mapping: a distant cloud ionized by Mkn 1
- New constraints on red-spiral galaxies from their kinematics in clusters of galaxies
- A Morphological Study on Galaxies Hosting Optical Variability-Selected AGNs in the COSMOS Field
- Machine learning technique for morphological classification of galaxies from SDSS. II. The image-based morphological catalogs of galaxies at 0.02<z<0.1
- Firefly: a browser-based interactive 3D data visualization tool for millions of data points
- Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
- Merger identification through photometric bands, colours, and their errors
- Reconstructing Orbits of Galaxies in Extreme Regions (ROGER) III: galaxy evolution patterns in projected phase space around massive X-ray clusters
- Using Dark Energy Explorers and Machine Learning to Enhance the Hobby-Eberly Telescope Dark Energy Experiment
- Solar Jet Hunter: a citizen science initiative to identify coronal jets in EUV data sets
- Uncovering Tidal Treasures: Automated Classification of Faint Tidal Features in DECaLS Data
- The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities
- SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
- Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA
- Galaxy Zoo Morphology and Photometric Redshifts in the Sloan Digital Sky Survey
- Morphology, color-magnitude and scaling relations of galaxies in Abell 426
- A NuSTAR and XMM-Newton Study of the Two Most Actively Star-forming Green Pea Galaxies (SDSS J0749+3337 and SDSS J0822+2241)
- Hubble flow variations as a test for inhomogeneous cosmology
- Optimizing the Human-Machine Partnership with Zooniverse
- Bayesian bulge-disc decomposition of galaxy images
- Do minor interactions trigger star formation in galaxy pairs?
- Strong [O III] λ5007 Compact Galaxies Identified from SDSS DR16 and Their Scaling Relations
- A MUSE/VLT spatially resolved study of the emission structure of Green Pea galaxies
- Usage Bibliometrics as a Tool to Measure Research Activity
- UM462, a local green pea galaxy analogue under the MUSE magnifying glass
- Search for the edge-on galaxies using an artificial neural network
- H-ATLAS: The Far-Infrared properties of galaxies in and around the Coma Cluster
- The Metallicity measurement of Early-type Galaxies
- Harnessing the Hubble Space Telescope Archives: A Catalogue of 21,926 Interacting Galaxies
- The Observable Supernova Rate in Galaxy-Galaxy Lensing Systems with the TESS Satellite
- CzSL: Learning from citizen science, experts and unlabelled data in astronomical image classification
- Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
- The impact of environmental effects on AGN: a decline in the incidence of ionized outflows
- Correlating galaxy shapes and initial conditions: an observational study
- Determining the time before or after a galaxy merger event
- Investigating the role of bars in quenching star formation using spatially resolved UV-optical colour maps
- The Bullseye: HST, Keck/KCWI, and Dragonfly Characterization of a Giant Nine-Ringed Galaxy
- The Classification of Optical Galaxy Morphology Using Unsupervised Learning Techniques
- Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks
- Computing Accurate Age and Distance Factors in Cosmology
- Galaxy Spin Classification I: Z-wise vs S-wise Spirals With Chirality Equivariant Residual Network
- The quantity of dark matter in early-type galaxies and its relation to the environment
- Galaxy Zoo JWST: Up to 75% of discs are featureless at
- The effects of UV photometry and binary interactions on photometric redshift and galaxy morphology
- Planet Hunters TESS V: a planetary system around a binary star, including a mini-Neptune in the habitable zone
- Learning with many experts: model selection and sparsity
- A post-merger enhancement only in star-forming Type 2 Seyfert galaxies: the deep learning view
- Galaxy Zoo: Clump Scout -- Design and first application of a two-dimensional aggregation tool for citizen science
- Reply & Supply: Efficient crowdsourcing when workers do more than answer questions
- Searching for Quasi-Periodic Eruptions using Machine Learning
- Does radiative feedback make faint z>6 galaxies look small?
- The First VLBI Detection of a Spiral DRAGN Core
- What determines the HI gas content in galaxies?: morphological dependence of the HI gas fraction across M*-SFR plane
- SpArcFiRe: morphological selection effects due to reduced visibility of tightly winding arms in distant spiral galaxies
- Estimating The Metallicity of Star-forming Early-type Galaxies
- Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
- Extreme gas kinematics in an off-nuclear HII region of SDSS J143245.98+404300.3
- The Galaxy Population of the Core of Coma Cluster
- Identification and analysis of galactic bars in DESI Legacy Imaging Surveys
- Spin alignment around TNG300-1 voids
- AstroInspect: a web-based system to organize, assess, and visually inspect astronomical objects
- The Ly and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
- Identification of ram pressure stripping features in galaxies using citizen science
- Three New Spiral Galaxies with Active Nuclei Producing Double Radio Lobes
- Image feature extraction and galaxy classification: a novel and efficient approach with automated machine learning
- A comparative study of source-finding techniques in HI emission line cubes using SoFiA, MTObjects, and supervised deep learning
- Sports stars: analyzing the performance of astronomers at visualization-based discovery
- Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation
- Observational evidence for the evolution of nuclear metallicity and star formation rate as the merger stage
- The Impact of Bars, Spirals and Bulge-Size on Gas-Phase Metallicity Gradients in MaNGA Galaxies
- Evaluating User Experience and Data Quality in Gamified Data Collection for Appearance-Based Gaze Estimation
- Aggregating predictions from experts: a scoping review of statistical methods, experiments, and applications
- VizNet: Towards A Large-Scale Visualization Learning and Benchmarking Repository
- Unveiling the nature of the "Green Pea" galaxies
- AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
- The Intrinsic Flattening of Galaxy Disks
- Black hole growth and host galaxy morphology
- Jovian Vortex Hunter: a citizen science project to study Jupiter's vortices
- Measuring the Metallicity of Early-type Galaxies. I. Composite Region
- The MOSDEF Survey: Probing Resolved Stellar Populations at Using a New Bayesian-defined Morphology Metric Called Patchiness
- A simple direct empirical observation of systematic bias of the redshift as a distance indicator
- Mock Observations: Morphological Analysis of Galaxies in TNG100 Simulations
- VeSPA: The SuperWASP Variable Star Photometry Archive
- Machine Learning and galaxy morphology: for what purpose?
- A Morphological Model to Separate Resolved-Unresolved Sources in the DESI Legacy Surveys: Application in the LS4 Alert Stream
- Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
- An analytical model to kinematically identify thin discs in MaNGA galaxies
- COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
- Late growth of early-type galaxies in low-z massive clusters
- The Challenge of Variable Effort Crowdsourcing and How Visible Gold Can Help
- Deep Learning Applications Based on WISE Infrared Data: Classification of Stars, Galaxies and Quasars
- Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
- Galactic Component Mapping of Galaxy UGC 2885 by Machine Learning Classification
- Tidally-induced radial migration waves in LMC-like galaxies
- Insights on Galaxy Evolution from Interpretable Sparse Feature Networks
- A machine learning approach to assessing the presence of substructure in quasar host galaxies using the Hyper Suprime-Cam Subaru Strategic Program
- Launching the VASCO citizen science project
- Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
- The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
- Using the XMM Optical Monitor to Study Cluster Galaxy Evolution
- Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch
- The luminosity history of fading local quasars over 10 years as observed by VLT/MUSE
- Linear response of rotating and flattened stellar clusters: the oblate Kuzmin-Kutuzov Stäckel family
- Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
- Semi-supervised Learning of Galaxy Morphology using Equivariant Transformer Variational Autoencoders
- Examining supernova events in Type 1 active galactic nuclei
- And the winner is: galaxy mass
- Search for Slow Bars in Two Barred Galaxies with Nuclear Structures: NGC 6951 and NGC 7716
- Blueberry and Green Pea galaxies live in low density environments
- Optical Follow-up of Planck Cluster Candidates with Small Instruments
- The Homogeneous Properties of Halpha-Selected Galaxies at (0.05<z<0.15)
- Galaxy Zoo: Morphologies based on UKIDSS NIR Imaging for 71,052 Galaxies
- The VIMOS Public Extragalactic Redshift Survey (VIPERS). The complexity of galaxy populations at 0.4< z<1.3 revealed with unsupervised machine-learning algorithms
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- Data-driven dissection of emission-line regions in Seyfert galaxies
- Pushing the Technical Frontier: From Overwhelmingly Large Data Sets to Machine Learning
- Modeling with the Crowd: Optimizing the Human-Machine Partnership with Zooniverse
- The Hubble Image Similarity Project
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- Applied Nanofabrication for X-ray Grating Spectroscopy
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- HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
- UV bright red-sequence galaxies: a comparative study between UV upturn and UV weak systems
- RGC-Bent: A Novel Dataset for Bent Radio Galaxy Classification
- Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA
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- Galaxy evolution on resolved scales: ageing and quenching in CALIFA
- Quantifying the Poor Purity and Completeness of Morphological Samples Selected by Galaxy Colour
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- Merger or Not: Accounting for Human Biases in Identifying Galactic Merger Signatures
- The Visual Survey Group: A Decade of Hunting Exoplanets and Unusual Stellar Events with Space-Based Telescopes
- Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges
- The SATCHEL pipeline: A general tool for data classified through citizen science
- Effect of AGN on the morphological properties of their host galaxies in the local Universe
- Radio Galaxy Zoo: Morphological classification by Fanaroff-Riley designation using self-supervised pre-training
- Fast rigid alignment of heterogeneous images in sliced Wasserstein distance
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- The effect of spiral arms on the Sérsic photometry of galaxies
- Unveiling an old disk around a massive young leaking blueberry in SDSS-IV MaNGA
- Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam
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- Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
- AnomalyMatch: Discovering Rare Objects of Interest with Semi-supervised and Active Learning
- Automated Quantitative Description of Spiral Galaxy Arm-Segment Structure
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- Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam
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