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Paper Citation Record · LEDGER

Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2408.00609.

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

pith.paper-citation-record.v1
2408.00609 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 2026-08-09T06:31:02.800959+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T17:08:38.589969Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T21:38:59.261158Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 808cec01-0885-4bca-b14f-0d094cd66bac · inbound

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies cites this paper.

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

Reference 97

Resolution
verified exact
arxiv_id, observed 2026-05-18T04:50:54.066513Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-18T04:48:55.126852Z digest=sha256:b255241bd4a339f9194affb417f2c9b54102a514ea069c1ab2fe07d8b611b3f2

Observation 04cc0201-d45c-44f9-9e4a-1a5c4f030eec · inbound

Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves cites this paper.

Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-03T17:08:38.589969Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:08:38.589969Z digest=sha256:8c1b3ae825ebc21cabf2e72175524b6388fd4c4adc47227a0136742eab3a011e

Observation a14b283f-204c-4dfb-9fc4-f9b5d3260dcf · inbound

Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays cites this paper.

Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-07-02T04:56:39.597887Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-28T08:37:43.649043Z digest=sha256:b39c786d174674e11f8336ba8f7e9398b35d420bf7dd241525580eb106f8d80e

Observation 7861466f-35bf-4658-b459-1daab09d1f7a · inbound

Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies cites this paper.

Synergy between CSST and future gravitational-wave detectors: Probing primordial black holes by cross-correlating dark sirens with galaxies Nanohertz gravitational waves from a quasar-based supermassive black hole binary population model as dark sirens

Reference 78

Resolution
verified exact
arxiv_id, observed 2026-07-03T21:38:59.262297Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-27T00:15:57.187962Z digest=sha256:7c785dd0aa8e47be3f1d3d4f61b555fd138bf63b7bf4fd5d1789ce82578554ea