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Paper Citation Record · LEDGER

Matter power spectrum and the challenge of percent accuracy

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:10:22.496250Z

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

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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 8ca005e1-1df7-4b4d-8f64-d17c5324a827 · inbound

Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection cites this paper.

Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection Matter power spectrum and the challenge of percent accuracy

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-14T15:10:22.496250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 00982f65-537f-4e08-9a9f-74a4b82b3afa · inbound

Cosmological N-body simulations: a challenge for scalable generative models cites this paper.

Cosmological N-body simulations: a challenge for scalable generative models Matter power spectrum and the challenge of percent accuracy

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T13:16:02.612378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:16:02.612378Z digest=sha256:3ae219ad39f3184cf6a64ca33e29d7c167eadfd65564240b6f36d61ac24f302b

Observation 77648203-1066-4d4b-b452-72f862b8dd9a · inbound

Einstein-Vlasov Calculations of Structure Formation cites this paper.

Einstein-Vlasov Calculations of Structure Formation Matter power spectrum and the challenge of percent accuracy

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-14T13:12:39.368584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:12:39.368584Z digest=sha256:2d79b3aa2e0ca81dc855d23e1c14abc10daa305cba37cb3d372848da20d2d939

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 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-18T06:13:13.345307Z digest=sha256:6b4646017667f9d8ef50ca4c85da39c7b5dccaeec632696d58cc1f6f0ed11789

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 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-27T11:43:20.857862Z digest=sha256:3c363dc965659a7747ca638e7e5d87cacea0e58c7fa582a2fa5ea7b63982993a

Observation d9613f9e-55ba-40e5-a9c3-954cc2adc20e · inbound

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models Matter power spectrum and the challenge of percent accuracy

Reference 189

Resolution
unresolved
no resolver link, observed 2026-07-31T05:29:30.286704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:29:30.286704Z digest=sha256:042515dcc29df150c623b95e8544d0e34ba025edd3a8ed2ff1aae85b97521566