Paper Citation Record · LEDGER

Cosmological constraints on neutrinos after BICEP2

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1404.3598.

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pith.paper-citation-record.v1
1404.3598 v3

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T15:18:26.714825Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T02:19:23.743251Z

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Outbound references

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Pith citing papers

Observation 63c39db1-669f-4abf-b00c-f082cc5720e8 · inbound

Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations cites this paper.

Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations Cosmological constraints on neutrinos after BICEP2

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-12T15:18:26.714825Z

Source-reported events for the cited work

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Observation 84da9976-fd29-4531-ab2c-e99fc9a19d70 · inbound

Prospects for measuring neutrino mass with 21-cm forest cites this paper.

Prospects for measuring neutrino mass with 21-cm forest Cosmological constraints on neutrinos after BICEP2

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T22:48:20.932378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2aeca336-20c5-496c-8dc1-a09d45a73c4a · inbound

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Cosmological constraints on neutrinos after BICEP2

Reference 5

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03948f46-a6d8-4a14-be0c-3c7bd2b90927 · inbound

Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays cites this paper.

Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays Cosmological constraints on neutrinos after BICEP2

Reference 39

Resolution: verified exact; local_arxiv, observed 2026-07-02T05:06:39.185609Z

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Observation 7c21f549-9e3b-44b7-b5ca-bc05369236dc · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Cosmological constraints on neutrinos after BICEP2

Reference 138

Resolution: verified exact; local_arxiv, observed 2026-07-02T10:56:52.455932Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 25b08091-f21d-4a5f-a162-bb4338f27f92 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Cosmological constraints on neutrinos after BICEP2

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-07-04T02:19:23.744866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9bc84c67-61ef-4d7c-bade-79c9d31fd9af · inbound

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Cosmological constraints on neutrinos after BICEP2

Reference 198

Resolution: unresolved; no resolver link, observed 2026-07-12T04:18:55.037825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.