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Paper Citation Record · LEDGER

Model independent reconstruction of cosmological accelerated-decelerated phase

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2106.15579.

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

pith.paper-citation-record.v1
2106.15579 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 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:17:14.605852Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-13T18:38:07.464998Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 854f4721-6f8a-41a3-88bb-e4a927d0d565 · inbound

Cosmological implications and causality in $f(R, L_{m}, T)$ gravity theory with observational constraints cites this paper.

Cosmological implications and causality in $f(R, L_{m}, T)$ gravity theory with observational constraints Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 105

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no resolver link, observed 2026-08-10T20:17:14.605852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c891d5ef-7fd8-4c4b-9a62-d02d08112af1 · inbound

Cosmic distance duality after DESI 2024 data release and dark energy evolution cites this paper.

Cosmic distance duality after DESI 2024 data release and dark energy evolution Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 39

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unresolved
no resolver link, observed 2026-08-10T14:34:39.736716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2b0e192b-74db-44bd-8682-69d4a362becc · inbound

Transit dark energy cosmological models in generalized matter-geometry coupling theory using a non-linear form of $f(R,T,L_{m})$ function cites this paper.

Transit dark energy cosmological models in generalized matter-geometry coupling theory using a non-linear form of $f(R,T,L_{m})$ function Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 91

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unresolved
no resolver link, observed 2026-08-04T18:30:54.581086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 4a5d9f02-68b0-4b05-a271-237318bb07b4 · inbound

Mapping the redshift drift at various redshifts through cosmography cites this paper.

Mapping the redshift drift at various redshifts through cosmography Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 49

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verified exact
arxiv_id, observed 2026-05-13T18:38:07.466355Z

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=2026-05-13T18:35:55.346976Z digest=sha256:4fc563c8350e3f1f538ebd12c19f7fbe456ab30350f1a64e8349b817b22a63a9

Observation da245f49-b2ad-4778-a6b0-696a3769f522 · inbound

Cosmological consequences of scale-dependent Barrow-Tsallis entropy cites this paper.

Cosmological consequences of scale-dependent Barrow-Tsallis entropy Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 123

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unresolved
no resolver link, observed 2026-08-01T02:30:08.300992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a3331199-29c3-4f4d-963b-76912ead4a7e · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Model independent reconstruction of cosmological accelerated-decelerated phase

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-06T00:32:12.180001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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