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Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2412.04430.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T03:21:43.406790Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T02:19:23.500241Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
No source-named external measurement is stored.
Outbound references
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Pith citing papers
Observation 9993121d-9b7f-4333-957b-0b7d2b150524 · inbound
DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints cites this paper.
DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 132
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T09:56:03.389538Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 4223870c-fcd3-4353-b672-110070e4ebd3 · inbound
Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape cites this paper.
Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 183
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T17:46:23.344612Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 95f5c847-7450-46a4-bf3c-b222113d08fd · inbound
Type II Seesaw Leptogenesis in a Majoron background cites this paper.
Type II Seesaw Leptogenesis in a Majoron background Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 104
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T07:52:10.077139Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 2d9419cd-0934-4a96-8f49-f247a0805eab · inbound
Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM cites this paper.
Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T18:51:47.363889Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d54483b9-4972-48cf-8324-1d7d29194ec8 · inbound
Reconstructing dark energy with fewer assumptions cites this paper.
Reconstructing dark energy with fewer assumptions Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 81
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T14:57:04.202699Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 15dd65d8-2966-4e59-b25c-72e77564f7b6 · 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 Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 134
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:19:23.501584Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 300bd0d5-b445-44ec-b1cf-39072b9d7e22 · inbound
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T17:17:51.239532Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4fed44a3-6c62-4e3e-9406-45a3d145bb04 · inbound
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T03:21:43.406790Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.