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Paper Citation Record · LEDGER

Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2410.10559.

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

pith.paper-citation-record.v1
2410.10559 v3

Coverage vector

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 2026-08-22T06:32:14.747728+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:25:17.452060Z

measured 1 of 1 external citation measurements

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

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External citation measurements

3
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b53cb856-f56f-4822-a6ef-6ba7c1050fcc · inbound

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics cites this paper.

Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-11T12:25:17.452060Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T12:25:17.452060Z digest=sha256:b20a12be66bd666229934bd2822b4d461598b1ff98d706361554d9bc43361122

Observation 7b1e8409-19bb-40f8-91c1-447d48a6a9ae · inbound

Can the sound horizon-free measurement of $H_0$ constrain early new physics? cites this paper.

Can the sound horizon-free measurement of $H_0$ constrain early new physics? Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-10T05:59:55.744105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T05:59:55.744105Z digest=sha256:71d553f78bd2cf426ad3e1b6b04cce04832b36f50dddc50faf6aa661e823e9b7

Observation 02466509-7aae-4b64-943e-5738ec3f82fe · inbound

BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:39.321325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:39.321325Z digest=sha256:1f5ab9181851776724a1a6a669424d35246d5071f2d177e2692d39f268fb8425

Observation 6dbcbbd9-d6cd-4d6d-b59b-3710ed2b6c44 · inbound

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 137

Resolution
verified exact
arxiv_id, observed 2026-05-11T11:41:01.817857Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-10T12:56:21.466420Z digest=sha256:cddcbba6dde5eff2f82f6440d1f7beef42de3e6a1f3e0cc88a50f349b9135575

Observation c0bba374-4291-49cb-bc9a-8c7e5b3e54c0 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 132

Resolution
verified exact
arxiv_id, observed 2026-07-04T02:19:23.564909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-26T19:48:32.340111Z digest=sha256:a3c591fdca527556fa7008eecf9c34972f297aa7ef5ccc7fc417e70793c79488

Observation 004560b3-b626-48c2-b3c9-a18635b192a4 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 142

Resolution
verified exact
local_arxiv, observed 2026-07-08T15:55:04.696857Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:674aea282a7a2e4f1702b9266d386a3fcfb8b74b1f6a5b20c19b03ecf2b70c04

Observation b069ab79-8815-40f5-a7ce-ac62cd2467a0 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Scale-dependence in $\Lambda$CDM parameters inferred from the CMB: a possible sign of Early Dark Energy

Reference 150

Resolution
unresolved
no resolver link, observed 2026-08-01T08:08:48.173777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T08:08:48.173777Z digest=sha256:0dc8a63feec97203d0a4d510ef96e42904b5c898720525b2c321ceee8618493e