Paper Citation Record · LEDGER

MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0005123.

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

pith.paper-citation-record.v1
astro-ph/0005123 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T22:04:18.459789Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T02:13:10.868809Z

Reference resolution

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verified fuzzy0
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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 b6a65d33-0ed9-49a4-9883-9ecdf046d5b6 · inbound

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations cites this paper.

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-04T16:16:24.072838Z

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.

Observation e9b20d2e-3bb3-4695-a468-a6c7e88cc934 · inbound

Influence of density-dependent bag function $B(n)$ on strange stars for non-zero strange quark mass ($m_s\neq0$) in $f(R,T)$ gravity consistent with observational validation cites this paper.

Influence of density-dependent bag function $B(n)$ on strange stars for non-zero strange quark mass ($m_s\neq0$) in $f(R,T)$ gravity consistent with observational validation MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-15T22:04:18.459789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6484021d-b015-4822-926a-3ad9928450ee · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-06T18:16:05.831207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.