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Paper Citation Record · LEDGER

The primordial helium abundance and the number of neutrino families

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1608.02062.

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

pith.paper-citation-record.v1
1608.02062 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:47:00.980463Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

3
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1caac62a-ee12-425c-a501-edf6cb68641c · inbound

Planck 2018 results. VI. Cosmological parameters cites this paper.

Planck 2018 results. VI. Cosmological parameters The primordial helium abundance and the number of neutrino families

Reference 259

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verified exact
arxiv_id, observed 2026-05-10T14:45:47.082999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation c430e3ec-0ea0-4359-bc4b-1a60b64bbe58 · inbound

Efficient Search for Extremely Metal Poor Galaxies in the Local Universe using Convolutional Neural Networks cites this paper.

Efficient Search for Extremely Metal Poor Galaxies in the Local Universe using Convolutional Neural Networks The primordial helium abundance and the number of neutrino families

Reference 63

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unresolved
no resolver link, observed 2026-08-09T14:47:00.980463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation f3abf06c-eabb-401d-98eb-91f1826e7b76 · inbound

C-parity, magnetic monopoles and higher frequency gravitational waves cites this paper.

C-parity, magnetic monopoles and higher frequency gravitational waves The primordial helium abundance and the number of neutrino families

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-07T19:23:50.456530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 6e404170-2d3e-42d5-8555-b933eaa8c3d6 · inbound

EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low $Y_\mathrm{P}$ Value cites this paper.

EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low $Y_\mathrm{P}$ Value The primordial helium abundance and the number of neutrino families

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:08.997234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 33f41ba2-972b-441c-937b-5cf725853532 · inbound

The AURORA Survey: Robust Helium Abundances at High Redshift Reveal A Subpopulation of Helium-Enhanced Galaxies in the Early Universe cites this paper.

The AURORA Survey: Robust Helium Abundances at High Redshift Reveal A Subpopulation of Helium-Enhanced Galaxies in the Early Universe The primordial helium abundance and the number of neutrino families

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-06T15:04:35.804310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d1e4cbfa-b1d2-4b6b-9c14-cdb18e6fd680 · inbound

Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison cites this paper.

Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison The primordial helium abundance and the number of neutrino families

Reference 250

Resolution
unresolved
no resolver link, observed 2026-08-05T23:25:36.873529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 3922b3a5-7a30-463f-817f-7450715cc5d1 · inbound

Magnetic monopoles and high frequency gravitational waves from quasi-stable strings cites this paper.

Magnetic monopoles and high frequency gravitational waves from quasi-stable strings The primordial helium abundance and the number of neutrino families

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-02T19:17:02.074845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 223d43a1-7307-42b9-b198-3ea06964b6c0 · inbound

Dartmouth Stellar Evolution Emulator (DSEE) 1: Generative Stellar Evolution Model Database cites this paper.

Dartmouth Stellar Evolution Emulator (DSEE) 1: Generative Stellar Evolution Model Database The primordial helium abundance and the number of neutrino families

Reference 77

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verified exact
arxiv_id, observed 2026-05-10T18:40:43.266484Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 69caead4-35bf-4032-9a6c-7683699278bd · inbound

Fifty years of primordial helium abundances: A statistical reanalysis cites this paper.

Fifty years of primordial helium abundances: A statistical reanalysis The primordial helium abundance and the number of neutrino families

Reference 133

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:21:49.706152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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