Paper Citation Record · LEDGER

The high-Eddington NLS1 Ark 564 has the coolest corona

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1703.09815.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1703.09815 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:25:55.201617Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
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External citation measurements

88
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7be52d74-c23c-4200-89aa-d8bf927e8222 · inbound

Relativistic reflection spectra of super-spinning black holes cites this paper.

Relativistic reflection spectra of super-spinning black holes The high-Eddington NLS1 Ark 564 has the coolest corona

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-14T13:25:55.201617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6365f78e-f581-4e79-a7d8-50357c21b146 · inbound

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates The high-Eddington NLS1 Ark 564 has the coolest corona

Reference 286

Resolution: verified exact; local_arxiv, observed 2026-05-19T16:17:39.480536Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 7c4c1d48-ac56-4fe5-a55e-9c57698b6b9f · 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 The high-Eddington NLS1 Ark 564 has the coolest corona

Reference 252

Resolution: unresolved; no resolver link, observed 2026-07-12T03:29:42.101488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b5c41fe-ffdd-405b-a8e6-b0f0e667c442 · inbound

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations cites this paper.

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations The high-Eddington NLS1 Ark 564 has the coolest corona

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T02:20:50.991700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.