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Paper Citation Record · LEDGER

X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1503.02085.

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

pith.paper-citation-record.v1
1503.02085 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 2026-08-06T06:34:29.942622+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T19:48:52.668705Z

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 9a0ad164-7d44-4f98-ab05-3409154e01dd · 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 X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?

Reference 9

Resolution
verified exact
local_arxiv, observed 2026-05-25T05:35:22.061475Z

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=sha256:61f2f95f441291a92623160a8911dad1b762fe7670bb35f0fac70984c9e49a35

Observation 77f8100d-19a5-4527-9bdb-d9e72ff0045e · 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 X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-06-28T17:32:25.208762Z

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:aac1c7afd83150c064782b4213c2c7737b34af0ca01df94366ea004749c6309d

Observation f521a358-3ae5-42fb-ad28-612e221fc22f · inbound

A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\sim$3-15 cites this paper.

A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\sim$3-15 X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?

Reference 156

Resolution
metadata mismatch
local_arxiv, observed 2026-07-01T03:45:19.903944Z

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:aec51814d75b26ed69738f92e26028940348c5dab6b11209edabe468c5524afc

Observation 65f86a6a-1557-4255-9787-58fa6c2abcd1 · inbound

Extreme outflow velocities and weak UV emission lines indicate quasars shedding their dust cocoons cites this paper.

Extreme outflow velocities and weak UV emission lines indicate quasars shedding their dust cocoons X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?

Reference 96

Resolution
verified exact
local_arxiv, observed 2026-07-03T19:48:52.673432Z

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=sha256:5ff496994ce253ad8bf915a8cdcc2adcc37f3acb043c253046ca814e96814e0b