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Paper Citation Record · LEDGER

Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2108.11671.

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

pith.paper-citation-record.v1
2108.11671 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:52:14.678272Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T20:06:29.683905Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 50df48d7-89d9-4f4b-ad16-70134c637a1f · inbound

Can quasars, triggered by mergers, account for NANOGrav's stochastic gravitational wave background? cites this paper.

Can quasars, triggered by mergers, account for NANOGrav's stochastic gravitational wave background? Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-11T13:52:14.678272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:52:14.678272Z digest=sha256:2c79f2481f88bdab07dc87d53af55bd9504973a994ab1c1e01f50848f1672851

Observation c8b246d2-6675-44b4-bb28-e362af3a38de · inbound

A critical look at low-scale cosmological phase transitions in the PTA era cites this paper.

A critical look at low-scale cosmological phase transitions in the PTA era Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 19

Resolution
metadata mismatch
arxiv_id, observed 2026-07-03T09:27:48.961076Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-03T09:23:17.300830Z digest=sha256:af7d8f505a4ce2a4065f2e60a424a61db9aa0b9497a7c8b22931022298f8c047

Observation 1b9b801a-cf5f-4ab1-ab70-8e80c4636a94 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 195

Resolution
unresolved
no resolver link, observed 2026-07-12T05:10:13.912506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:10:13.912506Z digest=sha256:64124d4cd7fb467263201d09bfc0258549a01ac24b8a2096dbe9871c4ad24214

Observation 3400aa85-76e2-4366-ae88-c70c373abdd5 · inbound

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations cites this paper.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 51

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.343272Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3a97d4acd3024c4598558e37bbe27d9dac54b80c9d0e2b52f82e189fddea7e9c

Observation fd90c9e7-0ebd-422b-985d-6012bf394d4a · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 102

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:06:29.685141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4f4c6f8fe03b72ebeeded31996237d67b3a45751f7eb9fd0b68084dbfcce9598