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Paper Citation Record · LEDGER

Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1807.08757.

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

pith.paper-citation-record.v1
1807.08757 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T17:42:25.577522Z

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 019a43f1-db5b-4b13-a446-ed14ff561994 · inbound

Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds cites this paper.

Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk

Reference 131

Resolution
verified exact
local_arxiv, observed 2026-05-25T05:35:21.994484Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1ce4085936e1cb0e64e2a8438bdcd89e42e070a9758daf4b95bc2610bcd15c2a

Observation eedc50ca-37d6-45b6-99ce-ee832f21232c · inbound

Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes cites this paper.

Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-06-28T17:42:25.579567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:cc43d0e04ecaf6c6421e5e7b87b953dd060a9b1ef9e35797737277482cf1b284