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Paper Citation Record · LEDGER

Matter power spectrum and the challenge of percent accuracy

As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1503.05920.

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

pith.paper-citation-record.v1
1503.05920 v3

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 2026-07-22T06:31:00.163083+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-27T11:43:20.857862Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T07:47:45.297822Z

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 62e10300-cd79-4161-af73-82d99bca12a0 · inbound

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA cites this paper.

Modeling nonlinear scales for dynamical dark energy cosmologies with COLA Matter power spectrum and the challenge of percent accuracy

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-05-18T06:15:58.396588Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-05-18T06:13:13.345307Z digest=sha256:2a61fc1cb005f0d6d4fd9b65d411554ee912ecd238b5644be2a827c2167ecf6f

Observation 30a1c723-2cdf-4fac-9738-085f56490a22 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Matter power spectrum and the challenge of percent accuracy

Reference 98

Resolution
verified exact
local_arxiv, observed 2026-07-03T07:47:45.299161Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.

source=pdf_text observed=2026-06-27T11:43:20.857862Z digest=sha256:4f58076606af103a87f1731ca55476fc36f3914bf2f722dd096040383c71415a