Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1912.08720.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-31T03:00:27.608606Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-07T22:24:10.847391Z
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 468634b4-c893-436d-9cb8-a29ef1d54e50 · inbound
The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 cites this paper.
The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-07-07T22:24:10.849311Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation c352279e-d6f5-44b8-9193-d1026adc66d9 · inbound
How massive and clumpy must a quasar wind be to create emission line blueshifts? cites this paper.
How massive and clumpy must a quasar wind be to create emission line blueshifts? NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T03:00:27.608606Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.