Paper Citation Record · LEDGER

The rapid growth phase of supermassive black holes

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1805.08293.

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

pith.paper-citation-record.v1
1805.08293 v2

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 2026-08-03T06:30:56.289259+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 2026-07-02T18:27:16.328017Z

Reference resolution

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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 f7d51b8c-c270-4151-a5f9-a624c13fa93e · inbound

The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes cites this paper.

The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes The rapid growth phase of supermassive black holes

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-06-27T15:31:01.092675Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 31641949-afd8-497c-929b-a7ea30c754a3 · inbound

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ cites this paper.

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ The rapid growth phase of supermassive black holes

Reference 247

Resolution: verified exact; local_arxiv, observed 2026-06-26T20:09:57.399206Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation db50534a-8e8f-41c8-ac31-835bf154061c · inbound

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium The rapid growth phase of supermassive black holes

Reference 170

Resolution: verified exact; local_arxiv, observed 2026-06-27T01:00:20.710855Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation b24eb6dc-760b-40ac-b9cb-5f3b9a4f9bde · inbound

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 cites this paper.

Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5 The rapid growth phase of supermassive black holes

Reference 205

Resolution: verified exact; local_arxiv, observed 2026-07-02T18:27:16.329274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.