Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Disentangling the AGN and Star-Formation Contributions to the Radio-X-ray Emission of Radio-Loud Quasars at 1<z<2
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2011.03130.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T22:06:53.103870Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-01T11:05:42.596009Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 f80ad3ff-4956-460a-bdf6-b1ed829b3e55 · inbound
Estimating the spins of supermassive black holes in distant ultraluminous quasars cites this paper.
Estimating the spins of supermassive black holes in distant ultraluminous quasars Disentangling the AGN and Star-Formation Contributions to the Radio-X-ray Emission of Radio-Loud Quasars at 1<z<2
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:06:53.103870Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1b299ef-8e94-4466-b4b5-48e6d57c4927 · inbound
Estimation of black hole spins in low-mass AGNs and comparison with other types of AGNs cites this paper.
Estimation of black hole spins in low-mass AGNs and comparison with other types of AGNs Disentangling the AGN and Star-Formation Contributions to the Radio-X-ray Emission of Radio-Loud Quasars at 1<z<2
Reference 59
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T11:05:42.597417Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 39643337-1782-4e56-9d45-d2e105fbb820 · inbound
The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.
The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Disentangling the AGN and Star-Formation Contributions to the Radio-X-ray Emission of Radio-Loud Quasars at 1<z<2
Reference 122
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:15:05.089352Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.