Paper Citation Record · LEDGER

Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:astro-ph/9707232.

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

pith.paper-citation-record.v1
astro-ph/9707232 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:24:50.154999Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T09:57:55.191647Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 5474e464-dd98-4fb2-b187-2e965a21e0c0 · inbound

A cosmology weakly dependent measurement of 2D Baryon Acoustic Oscillations scale from the Southern Photometric Local Universe Survey cites this paper.

A cosmology weakly dependent measurement of 2D Baryon Acoustic Oscillations scale from the Southern Photometric Local Universe Survey Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T05:24:50.154999Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed39250a-46e2-4460-bdf5-c9e5d7c9e381 · inbound

Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging cites this paper.

Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 144

Resolution: verified exact; local_arxiv, observed 2026-05-21T04:43:58.198092Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation d09a086d-0052-46a8-a729-776c32bb5280 · inbound

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-06-27T16:11:01.910799Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation af88addd-7b88-465e-b95b-13c69e601d67 · inbound

Galaxy clusters in the VIDEO fields: detection and characterisation in the context of MOONRISE cites this paper.

Galaxy clusters in the VIDEO fields: detection and characterisation in the context of MOONRISE Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-06-27T06:40:38.506485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 7dc75d14-65e9-46a2-9252-c344f63fac2c · inbound

Resolved HI and Environmental Dynamics cites this paper.

Resolved HI and Environmental Dynamics Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-07-03T09:57:55.193305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 352553b9-1e68-4034-80e6-40993b71b74c · inbound

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster cites this paper.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 209

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22cae579-6609-42e7-9bea-e9384dd6f0ea · inbound

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

Fuelling the central region of galaxies with misaligned gas accretion Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-02T01:00:30.072523Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d20f26a-5129-4b59-9816-7104fd3b0183 · inbound

The size of the HI disk across different environments: isolated, compact groups, clusters, and pairs cites this paper.

The size of the HI disk across different environments: isolated, compact groups, clusters, and pairs Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T20:59:43.089946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef1a7d3f-79d3-4d52-bf78-21963efda94a · 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? Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies

Reference 64

Resolution: unresolved; no resolver link, observed 2026-07-31T08:31:39.961548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.