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Paper Citation Record · LEDGER

Robust model comparison disfavors power law cosmology

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1502.05416.

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

pith.paper-citation-record.v1
1502.05416 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T23:21:52.934868Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T23:22:00.664742Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 6c0fb9a4-250d-4a2d-b6b3-3946af9bdd8c · inbound

Comparison of $R_h=ct$ and $\Lambda$CDM using DESI DR1 measurements cites this paper.

Comparison of $R_h=ct$ and $\Lambda$CDM using DESI DR1 measurements Robust model comparison disfavors power law cosmology

Reference 29

Resolution
verified exact
local_arxiv, observed 2026-08-06T23:22:00.784788Z

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=2026-08-06T23:21:52.934868Z digest=sha256:36994e334ae8db08d42551df40eab44a60685bd9c6d8cb59471cb8d1ebc0066e

Observation e4942abf-f435-464a-986c-310027aec2df · inbound

Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ cites this paper.

Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ Robust model comparison disfavors power law cosmology

Reference 135

Resolution
unresolved
no resolver link, observed 2026-07-31T11:14:47.104876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T11:14:47.104876Z digest=sha256:8278a789feffe786c6197c41791bd938a3a6794540621beb7595608dc8f97f37