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Paper Citation Record · LEDGER

SMBH Formation via Gas Accretion in Nuclear Stellar Clusters

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1106.5943.

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

pith.paper-citation-record.v1
1106.5943 v2

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 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T19:03:20.653492Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T06:27:50.128267Z

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 82276625-04e1-445b-8439-8db10aa05cf8 · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories SMBH Formation via Gas Accretion in Nuclear Stellar Clusters

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-05T19:03:20.653492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T19:03:20.653492Z digest=sha256:4ccde133341ccfd876a1426dea707be4e31d7bb4574e09a3dfcc4cc9f1ccfa1f

Observation 6f04c597-17a7-4310-92b4-5d85e9f9f8fa · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ SMBH Formation via Gas Accretion in Nuclear Stellar Clusters

Reference 169

Resolution
verified exact
local_arxiv, observed 2026-07-11T06:27:50.130098Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:0333114a9467602e31ae9b3e959151749bc02fbe9617c1e55d0432146e5df397

Observation cafc3214-c47e-477a-8a8f-d2c2227355f7 · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars SMBH Formation via Gas Accretion in Nuclear Stellar Clusters

Reference 229

Resolution
unresolved
no resolver link, observed 2026-08-01T13:38:42.263080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:38:42.263080Z digest=sha256:5e308e4fa9041e2c35b7629093e08f717780874f269a396f3c346eff97ba441f