Paper Citation Record · LEDGER

Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:astro-ph/0210148.

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

pith.paper-citation-record.v1
astro-ph/0210148 v2

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 13 of 13 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:41:51.330085Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T09:56:10.323869Z

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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 dfadc4d5-2b6c-4610-850e-5e14d6f993d6 · inbound

Deep Neural Emulation of the Supermassive Black-hole Binary Population cites this paper.

Deep Neural Emulation of the Supermassive Black-hole Binary Population Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-12T19:41:51.330085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e03b3397-bf1a-4996-abb6-b0cc1ad61135 · inbound

The Sound of Dark Sectors in Pulsar Timing Arrays cites this paper.

The Sound of Dark Sectors in Pulsar Timing Arrays Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T10:48:50.494849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b09a387-b6fa-453f-b999-00033367f480 · inbound

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization cites this paper.

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:21:14.678799Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ada75396-ef0c-46c8-8456-e3020b84f6da · inbound

Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions cites this paper.

Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-04T00:09:27.978079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05f47ea6-fd64-4441-968d-9b1ca2def9eb · inbound

NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots cites this paper.

NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-03T23:49:29.608203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1410adb8-fb6e-4eef-86b7-7cf9e72f0b61 · inbound

Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays cites this paper.

Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-11T14:11:04.030779Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a1d77e39-6ca7-46dd-90cd-a296d6577005 · inbound

Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions cites this paper.

Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 136

Resolution: verified exact; local_arxiv, observed 2026-06-30T12:14:39.411649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 735c8d6d-4d78-47e3-8632-30f55c9ada60 · inbound

Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks cites this paper.

Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 206

Resolution: verified exact; local_arxiv, observed 2026-06-28T08:51:49.008668Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 04001137-db8e-4c54-8f81-93a6e6ecf6e7 · inbound

A Joint Optimal Search for Gravitational Waves from Resolved and Unresolved Supermassive Binary Black Holes with Pulsar Timing Arrays cites this paper.

A Joint Optimal Search for Gravitational Waves from Resolved and Unresolved Supermassive Binary Black Holes with Pulsar Timing Arrays Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-07-03T23:09:01.306461Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 828aa26b-51d7-4677-8773-80872a483520 · inbound

Dual AGN and Multiple SMBH Systems in the Era of SKAO cites this paper.

Dual AGN and Multiple SMBH Systems in the Era of SKAO Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-06-30T01:34:10.471201Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation cd9df319-edc2-4c85-8d75-55a5b7833a9b · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 92

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation afc32bbc-315d-4d3c-aaa7-92527c85464d · 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 Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 136

Resolution: verified exact; local_arxiv, observed 2026-07-07T23:34:19.526764Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 2053d9c2-a81e-4b50-8d8a-97637364825f · inbound

Population statistics of nanohertz gravitational wave sources cites this paper.

Population statistics of nanohertz gravitational wave sources Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-07-09T09:56:10.325406Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.