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Paper Citation Record · LEDGER

Sharpening the predictions of big-bang nucleosynthesis

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9901157.

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

pith.paper-citation-record.v1
astro-ph/9901157 v1

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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:12:52.786501Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T11:12:54.201137Z

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 211e7c3f-a2a2-45d1-b859-5123b730ca04 · inbound

CAPMAP: A New Instrument to Measure the E-mode CMB Polarization on Angular Scales of 4 arcmin to 40 arcmin cites this paper.

CAPMAP: A New Instrument to Measure the E-mode CMB Polarization on Angular Scales of 4 arcmin to 40 arcmin Sharpening the predictions of big-bang nucleosynthesis

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-08-12T11:12:54.205600Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-12T11:12:52.786501Z digest=sha256:76f816fd88d3915a8305f6605dab252e169824d26f6ce4aeaeb6803026bdfd53

Observation b3240929-380d-4291-a2d1-a7e4ffee0196 · inbound

The art of simulating the early Universe. Part III: Scalar-Gauge-Fluid Dynamics cites this paper.

The art of simulating the early Universe. Part III: Scalar-Gauge-Fluid Dynamics Sharpening the predictions of big-bang nucleosynthesis

Reference 272

Resolution
malformed identifier
no resolver link, observed 2026-07-30T11:24:09.790880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-30T11:24:09.790880Z digest=sha256:5ae1cfa4a9489567d073c2dfb800561cc44af038c87757b727598caed0479e59