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Paper Citation Record · LEDGER

Toward a Self Consistent Model of the Ionized Absorber in NGC 3783

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0306460.

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

pith.paper-citation-record.v1
astro-ph/0306460 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:49:39.898670Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T21:49:39.946868Z

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 96ba0784-0fc4-41df-9da4-589148af5e44 · inbound

Structured ionized winds shooting out from a quasar at relativistic speeds cites this paper.

Structured ionized winds shooting out from a quasar at relativistic speeds Toward a Self Consistent Model of the Ionized Absorber in NGC 3783

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-08-15T21:49:39.953954Z

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.

source=pdf_text observed=2026-08-15T21:49:39.898670Z digest=sha256:a1a35806c9ce6c7898c6c34a81af9d165494027c6f6ddf604ce1ec33e4eaa2ca

Observation 78c877eb-8f49-47a0-8fd3-bc888253b05e · inbound

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve cites this paper.

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve Toward a Self Consistent Model of the Ionized Absorber in NGC 3783

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-02T06:14:12.981529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:14:12.981529Z digest=sha256:3b387487da6e2826f295342c6e6fd03f5ca1e65987a9496220cc60d3e0c78122