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Paper Citation Record · LEDGER

Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1902.07108.

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

pith.paper-citation-record.v1
1902.07108 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T21:04:17.828395Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T22:08:59.635673Z

Reference resolution

0 of 0 outbound references displayed

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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 967cf023-f28c-4d17-9efe-acab9242c168 · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-08T21:04:17.828395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 4f019b52-bd92-40c9-afeb-81993921878c · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 175

Resolution
unresolved
no resolver link, observed 2026-08-07T18:51:43.917056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T18:51:43.917056Z digest=sha256:e74b4554e61002025b1152dc3ed1415164ea2136011fbec434866abccf407f75

Observation 69c701b0-d441-475f-be1e-e3389bab504b · inbound

Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.

Extended Dark Energy analysis using DESI DR2 BAO measurements Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 106

Resolution
verified exact
arxiv_id, observed 2026-05-14T21:04:03.786542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation d251ef30-b056-4a0e-8e5d-afe82113e4e0 · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-07T00:54:47.158702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:54:47.158702Z digest=sha256:6acb90e792fb5ea2fa3ac8244578ea80a8fba63a0c1448d29ea349f2186ce4a0

Observation 2ba7c547-5c43-4fac-8dee-a0f4338fe019 · inbound

Revisiting Heat Flux Analysis of Tungsten Monoblock Divertor on EAST using Physics-Informed Neural Network cites this paper.

Revisiting Heat Flux Analysis of Tungsten Monoblock Divertor on EAST using Physics-Informed Neural Network Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-06T04:31:57.320342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T04:31:57.320342Z digest=sha256:604d03f0eedc3fa8e4a9e4ee7cdc6f4a90bb935b6c53aa9ef02d601a1ff9ffc2

Observation 5f0646cb-7963-4b13-83dd-80b1f8b39261 · inbound

Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff cites this paper.

Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-03T12:39:04.805892Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T12:39:04.805892Z digest=sha256:62f0a4236ee911097ab99aa8a4acf17fa8813adfaa968e8f11a7db8f325b7d62

Observation a70708ff-1dfc-4caa-b5d8-f89fd9800792 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 110

Resolution
verified exact
arxiv_id, observed 2026-05-10T14:20:30.997291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

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Observation d6aa6a94-f350-44cc-af36-05c322552681 · inbound

Data-Driven Discovery of a Simple Phantom-Crossing Dark Energy Parametrization cites this paper.

Data-Driven Discovery of a Simple Phantom-Crossing Dark Energy Parametrization Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 50

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:08:59.637489Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-06-26T23:43:53.400685Z digest=sha256:eef706aef3e20085be8af727648f09b9595d76d4f194d72fc76694bc2be3e6ed

Observation 3afcc579-a1b7-46af-a985-a5bbf5c32eb4 · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-01T16:29:59.403877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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