Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2103.15862.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T22:09:16.493063Z
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
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
24
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation e871248f-71ef-4cc8-adb8-34f96cf18ee8 · inbound
Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography cites this paper.
Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
Reference 115
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:09:16.493063Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e1f13213-037d-45b1-a2e0-541c1619fbf7 · inbound
Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? cites this paper.
Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:15:09.565296Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ff6a7ab1-98a7-4afb-86b2-f40550cd25f0 · inbound
Low-redshift constraints on structure growth from CMB lensing tomography cites this paper.
Low-redshift constraints on structure growth from CMB lensing tomography First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T10:37:57.106168Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ec2b36c-9ff4-455e-9fd0-b94a66f34ec2 · inbound
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
Reference 285
- Resolution
- verified exact
- local_arxiv, observed 2026-07-14T14:30:37.643525Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 65c28dde-ad06-4985-8ab1-5c4b1b3d44ff · inbound
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
Reference 291
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:33:07.235672Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.