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Paper Citation Record · LEDGER

The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9603099.

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

pith.paper-citation-record.v1
astro-ph/9603099 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:11:50.692647Z

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
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

48
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5d77b6d2-e6f8-4364-b17b-162fadfbc9ba · 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 The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample

Reference 144

Resolution
verified exact
local_arxiv, observed 2026-06-28T17:42:25.657305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:fc3d79246190f463e6a565686d28d2d8f62d4476376e81a843e688adde596224

Observation af60ffdd-a20d-4a4e-bbcc-c3afe893259a · inbound

The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample

Reference 179

Resolution
verified exact
local_arxiv, observed 2026-06-27T21:01:16.017453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e6bcede1f5bba0cc179f2fea4baae2fdc95ae80ae705fc1879b31e3475c225a2

Observation 2606d735-15f7-4518-837f-b43e8410e360 · inbound

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region cites this paper.

Revealing the Physical Driver of the Baldwin Effect: Gas Density in the Broad-Line Region The Relationship Between the High Energy Continuum and Emission Lines in QSOs: A Low-Redshift Sample

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T00:11:50.692647Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:11:50.692647Z digest=sha256:c01cc29aaf0fb038445683b9de9eee52dc86fd59dbd47c0bc409a87fde1f08b0