Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2502.15541.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:40.603587Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T15:55:04.885749Z
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 e71cafa8-ec88-4069-b808-612cd642d8ec · 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 Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 98
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:40.603587Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3df0a110-39d4-4da0-ae7a-8063007c5700 · inbound
Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.
Beyond CPL: Evidence for dynamical dark energy in three-parameter models Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T10:46:16.660741Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation e03d971e-87d5-42dc-a94f-b5e62ac342e1 · inbound
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T07:19:37.649327Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7281ff48-79bc-4abb-93bd-d9727b8626cf · inbound
Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.
Observational constraints on early time non-phantom behaviour of dynamical dark energy Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:40:55.500232Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aa96b343-3d4b-4c00-b858-9dea1042a807 · 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 Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 141
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:36:03.772026Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 58b199f4-d71b-48b0-a00b-0df5d346f7d7 · inbound
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 132
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-01T16:45:51.112107Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation c169f564-163b-47b0-b4b4-d2ef9cce28f2 · inbound
Imprint of swampland-inspired coupled early dark energy cites this paper.
Imprint of swampland-inspired coupled early dark energy Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T15:55:04.887076Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 04284295-17ba-4df9-a40a-8cff70a20902 · inbound
Hubble tension: the shape wall cites this paper.
Hubble tension: the shape wall Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 158
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:08:49.066582Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 42b5eef7-c7e4-4bae-aa23-0df3021f43d1 · inbound
Hubble tension: a short review of theoretical explanations cites this paper.
Hubble tension: a short review of theoretical explanations Status of early dark energy after DESI: the role of $\Omega_m$ and $r_s H_0$
Reference 152
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:20:07.967357Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.