Paper Citation Record · LEDGER

Reconstructing the growth index $\gamma$ with Gaussian Processes

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2311.14216.

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

pith.paper-citation-record.v1
2311.14216 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T16:14:10.620745Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T21:15:12.060740Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 42c99660-1307-42c9-ba80-3652ee345f7c · inbound

Revisiting the temperature evolution law of the CMB with gaussian processes cites this paper.

Revisiting the temperature evolution law of the CMB with gaussian processes Reconstructing the growth index $\gamma$ with Gaussian Processes

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T12:25:52.239165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b2bb962d-9823-4e74-8a42-709ddf621473 · 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? Reconstructing the growth index $\gamma$ with Gaussian Processes

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-08-06T21:15:12.081248Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 577f8984-b302-4ac4-9544-f4c3813a60af · inbound

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts cites this paper.

Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts Reconstructing the growth index $\gamma$ with Gaussian Processes

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-15T16:14:10.620745Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1366348-45b1-4e52-b2cf-3aba492bb461 · inbound

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime cites this paper.

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime Reconstructing the growth index $\gamma$ with Gaussian Processes

Reference 141

Resolution: unresolved; no resolver link, observed 2026-08-04T12:59:05.781465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.