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Paper Citation Record · LEDGER

A relation between characteristic stellar age of galaxies and their intrinsic shape

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1804.07769.

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

pith.paper-citation-record.v1
1804.07769 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T01:00:36.789637Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 fc74bf68-4936-4a32-ab02-9ee8e454e7f4 · inbound

Fuelling the central region of galaxies with misaligned gas accretion cites this paper.

Fuelling the central region of galaxies with misaligned gas accretion A relation between characteristic stellar age of galaxies and their intrinsic shape

Reference 138

Resolution
unresolved
no resolver link, observed 2026-08-02T01:00:36.789637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:00:36.789637Z digest=sha256:bdacfca449d0d26d1b46034a32acd5f93a23c45d384db71c27283dce0ead93f2

Observation 7b626efa-67c9-4f77-9b9b-51bd34b179ab · inbound

Morphology-spin connection in the SAMI Galaxy Survey cites this paper.

Morphology-spin connection in the SAMI Galaxy Survey A relation between characteristic stellar age of galaxies and their intrinsic shape

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-01T14:46:54.223898Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:46:54.223898Z digest=sha256:9d3f2b83a1f11a993e2a3eb7ab289ae6dfca1f64d3c9796ba683e411e787d76d

Observation cb6a3e1e-c6f9-451c-ae45-9036959de9c4 · inbound

Too many quiescent late-type galaxies or a matter of misclassification? cites this paper.

Too many quiescent late-type galaxies or a matter of misclassification? A relation between characteristic stellar age of galaxies and their intrinsic shape

Reference 138

Resolution
unresolved
no resolver link, observed 2026-07-31T08:31:41.696715Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T08:31:41.696715Z digest=sha256:8c6866fdf1c7a4ce9aaf64b823032ecbe41b3d8339c3322c2eb5ff0130cef1e6