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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 15 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 2026-08-15T06:32:42.880941+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.

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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=sha256:36957c70a0ce200444cabee64dde6e63220175a29ed167985b43101b0d355afa

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:b47677f706f2b82dcb9f484e621426f408dce91af07aaa6baa63168318e39ed2

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-10T12:56:21.466420Z digest=sha256:0ac81e18e08cf110765f7065f6851c0fa541ffa95cb4c4750422d0a794882f2e

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-06-26T19:48:32.340111Z digest=sha256:048533ef771128ca571aaabe22edb4d7d18ca1df0dc56081368345d85043ffcf

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:19e1d545e0439b90eef4f74fe082db8487946745eb44983b9636b556f352afa3

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=sha256:164c0cda203452a3a883b7c0264bb951dc0e93f6ee143cedca279993174fb7f4