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Paper Citation Record · LEDGER

Parametrizing the Hubble function instead of dark energy: Many possibilities

As of 9 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 4 inbound Pith citation observations for arXiv:2508.08072.

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

pith.paper-citation-record.v1
2508.08072 v1

Coverage vector

measured 2 of 2 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T21:42:24.770083Z

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T21:43:50.271228Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T21:43:50.375133Z

Reference resolution

2 of 2 outbound references displayed

  • verified exact0
  • verified fuzzy1
  • unresolved1
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 4af6ae78-8d67-46a4-9588-540f222472e0 · outbound

This paper cites Straightforward Bayesian A/B testing with Dirichlet posteriors.

Parametrizing the Hubble function instead of dark energy: Many possibilities Straightforward Bayesian A/B testing with Dirichlet posteriors

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-05T21:42:24.740539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T21:42:24.740539Z digest=sha256:a88dc3bf4f536690e215fba7cdc2dc312e9f02240699e2616fd862f4135615b3

Observation 34c03c48-7c8b-4b7b-bdec-bb87f4117702 · outbound

This paper cites Bayesian histogram.

Parametrizing the Hubble function instead of dark energy: Many possibilities Bayesian histogram

Reference 2

Resolution
verified fuzzy
raw_fallback, observed 2026-08-05T21:42:24.934945Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-08-05T21:42:24.770083Z digest=sha256:da6f0364e06be8feafa7ab1fafdf5642dead438c02ec0549db5df74e6590dde0

Pith citing papers

Observation 23401293-2ffb-4668-95bc-58b283866812 · inbound

ExpVG: Investigating the Design Space of Visual Grounding in Multimodal Large Language Model cites this paper.

ExpVG: Investigating the Design Space of Visual Grounding in Multimodal Large Language Model Parametrizing the Hubble function instead of dark energy: Many possibilities

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-08-05T21:43:50.533612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-08-05T21:43:50.271228Z digest=sha256:a3d3d97b5b3ba132fbbe84df32c578eca2fe872475a870583dc937e70d5cee70

Observation 3b843227-c2b2-4fc7-9dfe-b4f2bdd7294c · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Parametrizing the Hubble function instead of dark energy: Many possibilities

Reference 154

Resolution
unresolved
no resolver link, observed 2026-08-04T09:59:26.637234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T09:59:26.637234Z digest=sha256:b70972c6e2fedec87fb61198333c8f9164825e9e78767a654ed5625308e0a0f4

Observation 375f8713-ae5a-4b14-84f6-87dc935e304e · inbound

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Parametrizing the Hubble function instead of dark energy: Many possibilities

Reference 130

Resolution
unresolved
no resolver link, observed 2026-08-04T07:19:40.584495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T07:19:40.584495Z digest=sha256:d86ae1639ae10e1a917e0d1d8f7819ea9835185fcd4540645ae9c27b8498f405

Observation a87c4a6b-7203-47dc-8568-ab2060da61c9 · inbound

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Parametrizing the Hubble function instead of dark energy: Many possibilities

Reference 129

Resolution
unresolved
no resolver link, observed 2026-07-12T04:18:55.037825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T04:18:55.037825Z digest=sha256:911321cc2e9e3cdf6aebd04ac23597f4e474334f1bb8472e9b5082b44d153981