Paper Citation Record · LEDGER

Cluster Abundance Constraints on Quintessence Models

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:astro-ph/9804015.

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

pith.paper-citation-record.v1
astro-ph/9804015 v1

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measured 0 of 0 reference resolution

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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 2026-08-08T06:32:00.761636+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T17:56:52.529032Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T14:19:54.201306Z

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Outbound references

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Pith citing papers

Observation 9e855dea-a84c-48a2-a10d-eaa28d063ee3 · inbound

Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution cites this paper.

Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution Cluster Abundance Constraints on Quintessence Models

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-05-15T17:32:24.481605Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 9b820157-b334-4609-8c29-5be47b9e5d68 · inbound

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions cites this paper.

Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions Cluster Abundance Constraints on Quintessence Models

Reference 136

Resolution: unresolved; no resolver link, observed 2026-08-08T17:56:52.529032Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49bc99e2-ea55-4e8b-8629-1d2c191d0e72 · inbound

Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear cites this paper.

Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear Cluster Abundance Constraints on Quintessence Models

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-08T14:44:45.831731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea7e8b3a-1587-469b-8845-5445c5b77da2 · inbound

Teleparallel dark energy in a nonflat universe cites this paper.

Teleparallel dark energy in a nonflat universe Cluster Abundance Constraints on Quintessence Models

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-07T13:42:46.748128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e7eb2666-5f93-46a9-8aca-f270715ae7aa · inbound

Testing Quasi-Linear Coasting Cosmologies with Late-Time Large-Scale Structure Growth cites this paper.

Testing Quasi-Linear Coasting Cosmologies with Late-Time Large-Scale Structure Growth Cluster Abundance Constraints on Quintessence Models

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T04:10:28.069532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8017c411-457b-44a3-bd9c-4b76a3d88394 · inbound

Realizing the phantom-divide crossing with vector and scalar fields cites this paper.

Realizing the phantom-divide crossing with vector and scalar fields Cluster Abundance Constraints on Quintessence Models

Reference 140

Resolution: unresolved; no resolver link, observed 2026-08-03T07:07:20.238451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8678ad2-1b92-4f0c-b87d-43bf2007b6ad · inbound

A short course in general relativity cites this paper.

A short course in general relativity Cluster Abundance Constraints on Quintessence Models

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-10T06:06:18.690078Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation ce3ab6b9-1f88-4485-b5aa-214e9bddeb4a · inbound

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations cites this paper.

Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations Cluster Abundance Constraints on Quintessence Models

Reference 109

Resolution: verified exact; local_arxiv, observed 2026-06-26T23:00:12.089517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation ea6a6da1-a354-4b82-b084-1897778d3192 · inbound

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy cites this paper.

Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy Cluster Abundance Constraints on Quintessence Models

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-07-04T14:19:54.202566Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.