Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1406.5297.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-07T23:34:19.350396Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 f8b0eb7c-e297-41be-a27b-5724d1ca08ca · 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 Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
Reference 211
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T08:51:48.998544Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 24f0780c-3c33-4d90-90ab-2f14fb6a2010 · 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 Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays
Reference 87
- Resolution
- verified exact
- local_arxiv, observed 2026-07-07T23:34:19.351808Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.