Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Exploring the role of the halo mass function for inferring astrophysical parameters during reionisation
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2403.14061.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T16:14:56.687672Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T16:14:57.517432Z
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 b6d50138-6bb2-43a3-95dd-75af7b48f801 · inbound
Simulation-based inference on warm dark matter from HERA forecasts cites this paper.
Simulation-based inference on warm dark matter from HERA forecasts Exploring the role of the halo mass function for inferring astrophysical parameters during reionisation
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T16:14:57.521827Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b6b4648b-9328-47e3-8d29-265772c1242e · inbound
21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter cites this paper.
21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Exploring the role of the halo mass function for inferring astrophysical parameters during reionisation
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T21:29:41.807350Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.