Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1811.01519.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T15:10:35.924972Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T15:10:38.507783Z
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 cbf8dabb-b646-4bf8-80fd-e54cd8e9cc1b · inbound
Probing the independence within the dark sector in the fluid approximation cites this paper.
Probing the independence within the dark sector in the fluid approximation A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T15:10:38.515374Z
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.
Observation 8e4c2acc-bb7a-422b-ba21-2e222aaba6ad · 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 A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T18:51:48.192203Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.