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Paper Citation Record · LEDGER

Time-dependent secular evolution in galaxies

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0404169.

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

pith.paper-citation-record.v1
astro-ph/0404169 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 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:44:09.131405Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

2
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7413a277-4f4c-4e25-b573-6705d650d975 · inbound

The Dipole Instability in Gravitational $N$-body Systems: A Natural Explanation for Lopsidedness and Off-Centered Nuclei in Galaxies cites this paper.

The Dipole Instability in Gravitational $N$-body Systems: A Natural Explanation for Lopsidedness and Off-Centered Nuclei in Galaxies Time-dependent secular evolution in galaxies

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-07T12:44:09.131405Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T12:44:09.131405Z digest=sha256:351ff3b5cbcdf75fb2e823fcde80f5e5b245f78e4f40047a4690a70c2e7ddc86

Observation ba6abf00-f608-4bd4-8537-9a7a694d65f2 · inbound

Self-interacting dark matter promotes bar formation in disk galaxies cites this paper.

Self-interacting dark matter promotes bar formation in disk galaxies Time-dependent secular evolution in galaxies

Reference 79

Resolution
metadata mismatch
local_arxiv, observed 2026-06-29T01:32:58.784298Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-06-29T01:30:28.489024Z digest=sha256:bc1c6adb04d66eb356c282cbb1c1c8fdf7f9907597dc955ce60b8a7fdab903a9

Observation 9a0c9677-f316-4554-a5a4-9502b68e3a15 · inbound

Wrinkles in Time. II. Stellar Age Trends in Kinematic Signatures from Transient Spiral Structure cites this paper.

Wrinkles in Time. II. Stellar Age Trends in Kinematic Signatures from Transient Spiral Structure Time-dependent secular evolution in galaxies

Reference 62

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T01:35:12.799983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-01T01:33:50.343703Z digest=sha256:d57b227675ee2f84c004e3bbad5a407263273c958052a3f53030ba3dbd5694ac