Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z=1
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2209.04245.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T18:15:24.343272Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T21:31:37.145727Z
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 2c6cc850-0163-4f9f-9666-58546359468c · inbound
MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ cites this paper.
MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z=1
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:15:24.343272Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 12efbe93-11ed-449e-bf56-315daace46b7 · inbound
MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis cites this paper.
MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z=1
Reference 28
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-11T21:31:37.149696Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.