Paper Citation Record · LEDGER

Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1001.4635.

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

pith.paper-citation-record.v1
1001.4635 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

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

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T04:21:33.284529Z

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

1351
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0ff114e1-8646-4224-bae4-404ef69ab700 · inbound

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model cites this paper.

CMB dipoles and other low-order multipoles in the quasispherical Szekeres model Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-05-24T18:54:50.829403Z

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 4f81ef55-ffaa-4668-854b-917f5712ab8a · inbound

The $\alpha$-Attractor E-Model in Warm Inflation: Observational Viability from Planck 2018 cites this paper.

The $\alpha$-Attractor E-Model in Warm Inflation: Observational Viability from Planck 2018 Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T06:11:28.062240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f71f013c-2c73-46c1-bac4-555a2e4f4676 · inbound

Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data cites this paper.

Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 97

Resolution: verified exact; arxiv_id, observed 2026-05-11T00:45:49.552638Z

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 e8935f3a-1e42-4df0-b709-ed507a657b78 · inbound

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz cites this paper.

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 281

Resolution: metadata mismatch; local_arxiv, observed 2026-05-25T03:56:36.222824Z

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 cbcaa3c4-50ce-4ef0-9c9f-04f84386e96a · inbound

Consistency of DES and DESI distances and the Standard Cosmological Model cites this paper.

Consistency of DES and DESI distances and the Standard Cosmological Model Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 119

Resolution: verified exact; local_arxiv, observed 2026-07-03T22:59:03.425440Z

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 e44c5935-d250-45d4-a51b-8c057a59234c · inbound

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor cites this paper.

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 141

Resolution: verified exact; local_arxiv, observed 2026-06-26T04:28:58.856072Z

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 68721c3a-d7ff-4e65-b7e5-2998c68a1cec · inbound

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction cites this paper.

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

Reference 132

Resolution: unresolved; no resolver link, observed 2026-08-07T11:34:41.508435Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 75ec4fab-aeff-4f98-ae65-56888fef46a0 · inbound

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction cites this paper.

Reference 132

Resolution: unresolved; no resolver link, observed 2026-08-11T04:21:33.284529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.