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Paper Citation Record · LEDGER

Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0712.3445.

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

pith.paper-citation-record.v1
0712.3445 v1

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 2026-08-15T15:15:04.708476Z

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

21
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 06cc79c0-b58c-4be0-a756-ba40d7a70183 · inbound

The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 cites this paper.

The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234

Reference 254

Resolution
verified exact
local_arxiv, observed 2026-07-07T22:24:11.051693Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2fb9234029764fce0636ee3e68c0bbe85d99bf06ff9ab2268f81a0172a2cc9dd

Observation 5f43b020-28be-46d4-bebb-b9e8d63d1a9e · inbound

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Heavy absorption and soft X-ray emission lines in the XMM-Newton spectrum of the Type 2 radio-loud quasar 3C 234

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-15T15:15:04.708476Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:15:04.708476Z digest=sha256:730f3d16116485e5e3aa0eeb6b348d18c7f2ace0d64411dedc071918d082f309