Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
ALMA 360 pc high-frequency observations reveal warm dust in the center of a $z=6.9$ quasar
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.14539.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:06:32.030328Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
3
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 4b214801-4131-4612-aa5b-82227bdd6eff · inbound
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? cites this paper.
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? ALMA 360 pc high-frequency observations reveal warm dust in the center of a $z=6.9$ quasar
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:06:32.030328Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cb6732e0-3342-43b1-861b-6adf54559d38 · inbound
Testing the AGN unified model with simulated emission lines from the circumgalactic medium (CGM) cites this paper.
Testing the AGN unified model with simulated emission lines from the circumgalactic medium (CGM) ALMA 360 pc high-frequency observations reveal warm dust in the center of a $z=6.9$ quasar
Reference 86
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-06T14:22:58.380687Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.