Paper Citation Record · LEDGER

The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9907399.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/9907399 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-13T04:41:12.165957Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-02T18:27:16.646152Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9b2fa4bd-e353-4582-be53-44cd1fd0330c · 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 $z=5$ The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

Reference 261

Resolution: verified exact; local_arxiv, observed 2026-06-26T14:39:32.445031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 7f55e0a6-786d-41d0-a9c6-59245a40721a · inbound

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 The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-06-29T04:03:05.579182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 0db1bcb4-b1b3-48a5-b9f7-47741fa5aea7 · 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 The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-07-01T05:15:24.257646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 2e7f4d08-80fa-4c64-aefb-dd11df05c7bb · inbound

The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances cites this paper.

The multiwavelength structure of post-starburst galaxies at 0.5 < z < 3 with JWST PRIMER: compact morphologies and residual disturbances The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-07-02T18:27:16.647935Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation a48f5a07-a531-44e4-ae0c-bd5fc0638ae8 · inbound

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 The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies

Reference 39

Resolution: unresolved; no resolver link, observed 2026-07-13T04:41:12.165957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.