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Paper Citation Record · LEDGER

Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1904.07887.

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

pith.paper-citation-record.v1
1904.07887 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 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 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T22:13:50.084261Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T06:47:43.690689Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 77396707-6789-4466-bfb2-975f762d7ac4 · inbound

Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning cites this paper.

Using X-Ray Morphological Parameters to Strengthen Galaxy Cluster Mass Estimates via Machine Learning Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 74

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no resolver link, observed 2026-08-14T14:41:19.960878Z

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Observation efc3b63f-3900-4b7f-95a3-c3b7e01bbc71 · inbound

The Cosmic Microwave Background -- Secondary Anisotropies cites this paper.

The Cosmic Microwave Background -- Secondary Anisotropies Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 202

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malformed identifier
no resolver link, observed 2026-08-10T15:33:40.890678Z

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Observation 943a8371-edea-4e00-a604-d606883494d2 · inbound

Cosmology with Galaxy Clusters cites this paper.

Cosmology with Galaxy Clusters Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 128

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Observation 429f174a-a69e-420c-a261-09f314fadf17 · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 23

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unresolved
no resolver link, observed 2026-08-07T04:48:07.545636Z

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Unavailable: canonical work link unavailable.

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Observation 85e82125-31d2-4d03-ac21-b78302b4bdab · inbound

Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications cites this paper.

Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 16

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arxiv_id, observed 2026-05-11T21:26:14.233469Z

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Observation bb55a8ce-b564-435a-9afe-a1ef4c9359bf · inbound

Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity cites this paper.

Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 49

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verified exact
arxiv_id, observed 2026-07-03T06:47:43.692084Z

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Observation 70917074-85c3-44f5-ae21-9661d1d6e967 · inbound

Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity cites this paper.

Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity Cosmological constraints from Planck galaxy clusters with CMB lensing mass bias calibration

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-02T11:57:28.552489Z

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