Paper Citation Record · LEDGER

Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1603.09348.

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

pith.paper-citation-record.v1
1603.09348 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

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

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:59:38.802191Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-07T23:34:19.347604Z

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 0458e954-c59f-4686-b8fd-dba35767ba50 · inbound

Evolution of SMBHs in light of PTA measurements: implications for growth by mergers and accretion cites this paper.

Evolution of SMBHs in light of PTA measurements: implications for growth by mergers and accretion Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T19:49:22.698253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d56fc13e-8030-400b-9c06-ec09a6619cb6 · inbound

Exploring Ultralight Dark Matter Self-Coupling via the Gravitational Wave Background cites this paper.

Exploring Ultralight Dark Matter Self-Coupling via the Gravitational Wave Background Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-16T05:59:38.802191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad6c5604-95d5-4c40-833e-803996fd7ade · inbound

Prospects for Time-Domain and Multi-Messenger Science with eXTP cites this paper.

Prospects for Time-Domain and Multi-Messenger Science with eXTP Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 2205

Resolution: unresolved; no resolver link, observed 2026-08-07T05:22:30.535397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 18bc2a99-1622-471a-a81a-c0bd9b8700f1 · 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 Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 213

Resolution: verified exact; local_arxiv, observed 2026-06-28T08:51:49.001326Z

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 bacbb565-75c0-49fc-888c-89d8fe74f5af · inbound

Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations cites this paper.

Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 120

Resolution: verified exact; local_arxiv, observed 2026-06-28T01:01:26.929700Z

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 cc6cef0b-c9ed-4099-8e9e-2794a81600b4 · 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 Selection bias in dynamically-measured super-massive black hole samples: consequences for pulsar timing arrays

Reference 132

Resolution: verified exact; local_arxiv, observed 2026-07-07T23:34:19.349134Z

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.