Paper Citation Record · LEDGER

A New Non-Parametric Approach to Galaxy Morphological Classification

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:astro-ph/0311352.

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pith.paper-citation-record.v1
astro-ph/0311352 v2

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measured 21 of 21 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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736
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Pith citing papers

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Predicting Potential Host Galaxies of Supermassive Black Hole Binaries Based on Stellar Kinematics in Archival IFU Surveys cites this paper.

Predicting Potential Host Galaxies of Supermassive Black Hole Binaries Based on Stellar Kinematics in Archival IFU Surveys A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 67

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Observation cab199d2-0d0e-44a0-b6ab-1ae333c84925 · inbound

statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys cites this paper.

statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 67

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Morphological complexity of NGC 628 - a multiwavelength multiscale analysis using the ordinal pattern framework cites this paper.

Morphological complexity of NGC 628 - a multiwavelength multiscale analysis using the ordinal pattern framework A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 42

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The Hubble sequence in JWST CEERS from unbiased galaxy morphologies cites this paper.

The Hubble sequence in JWST CEERS from unbiased galaxy morphologies A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 65

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ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in $z\sim3$ Sub-millimeter Galaxies cites this paper.

ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in $z\sim3$ Sub-millimeter Galaxies A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 67

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Extending the ALMA survey of the SCUBA-2 CLS UDS field: Tracing the obscured formation of spheroids across z~1-4 cites this paper.

Extending the ALMA survey of the SCUBA-2 CLS UDS field: Tracing the obscured formation of spheroids across z~1-4 A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 75

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A Rare Eddington-Limited, Heavily Obscured Low-Mass Active Galactic Nucleus Likely Triggered by a Galaxy Merger cites this paper.

A Rare Eddington-Limited, Heavily Obscured Low-Mass Active Galactic Nucleus Likely Triggered by a Galaxy Merger A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 71

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Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1 cites this paper.

Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1 A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 73

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Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies cites this paper.

Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 61

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Observation 24e84bf4-5e48-4d17-9aae-2925c01894cc · inbound

Robustness Analysis of USmorph: II. Optimizing Feature Extraction, Dimensionality Reduction, and Clustering for Unsupervised Galaxy Morphology Classification cites this paper.

Robustness Analysis of USmorph: II. Optimizing Feature Extraction, Dimensionality Reduction, and Clustering for Unsupervised Galaxy Morphology Classification A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 113

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Morphology of Optical Changing-Look AGN-host Galaxies: Evidence for an Important Role of Mergers cites this paper.

Morphology of Optical Changing-Look AGN-host Galaxies: Evidence for an Important Role of Mergers A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 34

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Metal-Poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.6 cites this paper.

Metal-Poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.6 A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 44

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Observation b0985f91-0726-4eab-8733-083a39622cd2 · inbound

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ cites this paper.

Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 246

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Observation 1969429a-284d-49e7-98b9-f4d2f301bba9 · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 165

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Cluster vs Field: Clear Evidence for a Morphology-Density Relation in All Environments at $z\sim1.6$ cites this paper.

Cluster vs Field: Clear Evidence for a Morphology-Density Relation in All Environments at $z\sim1.6$ A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 43

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MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec cites this paper.

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 290

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Observation a01d4042-a5b4-46e7-81f0-e98d5db7be36 · inbound

Global trends in morphology from massive to dwarf galaxies cites this paper.

Global trends in morphology from massive to dwarf galaxies A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 30

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Observation 99d4d569-b5a4-4dc4-af61-54f6976c92a3 · inbound

Deep Extragalactic VIsible Legacy Survey (DEVILS): Morphologically-selected galaxy merger fractions and their direct comparison to close-pair samples cites this paper.

Deep Extragalactic VIsible Legacy Survey (DEVILS): Morphologically-selected galaxy merger fractions and their direct comparison to close-pair samples A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 3

Resolution: verified exact; doi, observed 2026-07-01T05:15:24.411929Z

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Observation be868ea8-5aee-4d55-877d-da06aef4dabe · inbound

Source Finding and Characterisation for SKAO Science cites this paper.

Source Finding and Characterisation for SKAO Science A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 88

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Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 93

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Morphologies of SAGAbg low-mass galaxies in Legacy Survey multi-band imaging: dependence on stellar masses, star-formation rates and low-redshift evolution cites this paper.

Morphologies of SAGAbg low-mass galaxies in Legacy Survey multi-band imaging: dependence on stellar masses, star-formation rates and low-redshift evolution A New Non-Parametric Approach to Galaxy Morphological Classification

Reference 78

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