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Paper Citation Record · LEDGER

Using the Evolution of Clusters to Constrain Omega

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:astro-ph/9601088.

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

pith.paper-citation-record.v1
astro-ph/9601088 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 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 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:04:03.489751Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T23:46:22.974370Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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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 72ed4681-c9b7-4cb3-ad1b-893384ae82aa · inbound

Void spin distribution as a powerful probe of $\sigma_{8}$ cites this paper.

Void spin distribution as a powerful probe of $\sigma_{8}$ Using the Evolution of Clusters to Constrain Omega

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-10T20:04:03.489751Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T20:04:03.489751Z digest=sha256:f81fc183759bf0f88aa8b01c006dafbaa4d60ebcbca75fa82014c53504b58ff5

Observation 7896d62a-b980-4f6c-b7f3-9582ea4043f1 · inbound

Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions cites this paper.

Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions Using the Evolution of Clusters to Constrain Omega

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-06T20:29:16.275848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T20:29:16.275848Z digest=sha256:e5c4bb2a710fb05d096281334813a98944013f1db7f5966a0b9d12e4a085b398

Observation 1c4b5fa1-40ad-4b79-943c-9ce0873626dd · inbound

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter cites this paper.

Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter Using the Evolution of Clusters to Constrain Omega

Reference 55

Resolution
verified exact
arxiv_id, observed 2026-05-11T15:56:10.437386Z

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.

source=pdf_text observed=2026-05-09T19:03:26.030535Z digest=sha256:dddf82380f556351d51fdb318a5b6e76f8ff3d5d9799f6e691ec6f362d553a90

Observation 5af27fc0-bd13-4cb7-99eb-8d539af234dc · inbound

Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts cites this paper.

Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts Using the Evolution of Clusters to Constrain Omega

Reference 131

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T23:46:22.976163Z

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.

source=arxiv_source observed=2026-06-28T14:03:32.034571Z digest=sha256:dd18fef13ea47baa8250176a095256430f677b9e2ef705f8ec850303863a14b4

Observation 4edd283a-1e82-40ab-a6a7-7c96f47fde70 · inbound

A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations cites this paper.

A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations Using the Evolution of Clusters to Constrain Omega

Reference 36

Resolution
verified exact
local_arxiv, observed 2026-06-27T09:40:48.003975Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:eb3a5ebfc065b2a3c7586bc9b57713753fe4c94cc2cc12ed54aea3bc72728c8f

Observation 377a089f-1d18-49d8-813b-7cee54be4b95 · inbound

CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \leq 4$ cites this paper.

CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \leq 4$ Using the Evolution of Clusters to Constrain Omega

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-06-27T06:10:36.768413Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b6386cc6f385c0ea2aeb8483a8e6a63913615f8e73200e5533d0d982eb25e801

Observation e3f5396a-0979-4545-83a7-14db12ec3166 · inbound

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses cites this paper.

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses Using the Evolution of Clusters to Constrain Omega

Reference 10

Resolution
unresolved
no resolver link, observed 2026-07-11T06:41:50.562143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:41:50.562143Z digest=sha256:cd1cff44df4debe3bd5d81321fb39f6f3b51593869be62b61116241bf505f246

Observation 32649607-984e-419f-9ff7-69bb20de7909 · inbound

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Using the Evolution of Clusters to Constrain Omega

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-01T13:07:52.095000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:07:52.095000Z digest=sha256:5d89c83e2aa09dcc8737d51e1c07bf0a86e1c1cc589e4b1c1f87f128645e5bde