Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A physical model for the broadband energy spectrum of X-ray illuminated accretion discs: fitting the spectral energy distribution of NGC 5548
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2110.01249.
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 2026-08-06T21:45:13.901178Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-12T03:38:27.117802Z
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 b2ef4691-d65e-491b-bfc6-106a78492a77 · inbound
Continuum optical-UV and X-ray variability of AGN: current results and future challenges cites this paper.
Continuum optical-UV and X-ray variability of AGN: current results and future challenges A physical model for the broadband energy spectrum of X-ray illuminated accretion discs: fitting the spectral energy distribution of NGC 5548
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:45:13.901178Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fdc418a8-70de-43e3-bca0-049aecf09299 · inbound
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.
Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference A physical model for the broadband energy spectrum of X-ray illuminated accretion discs: fitting the spectral energy distribution of NGC 5548
Reference 142
- Resolution
- verified exact
- local_arxiv, observed 2026-07-12T03:38:27.119890Z
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.
Observation 96b86f07-9a46-4752-b994-18716ec53268 · inbound
X-ray disc reverberation modelling of the X-ray/UV/optical spectral/timing properties of Fairall 9 cites this paper.
X-ray disc reverberation modelling of the X-ray/UV/optical spectral/timing properties of Fairall 9 A physical model for the broadband energy spectrum of X-ray illuminated accretion discs: fitting the spectral energy distribution of NGC 5548
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:01:33.459504Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.