Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1702.06964.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T13:52:14.662184Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
42
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 7ee7a184-9535-47a8-9ccf-8065cf68df76 · 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? The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:52:14.662184Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fe96b90a-2aee-4bde-b071-5f25771e39d0 · 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 The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays
Reference 214
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T08:51:48.963703Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 47af05bb-e7a1-45c8-adb9-17a731370687 · 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 The nightmare scenario: measuring the stochastic gravitational-wave background from stalling massive black-hole binaries with pulsar-timing arrays
Reference 139
- Resolution
- verified exact
- local_arxiv, observed 2026-07-07T23:34:19.190988Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.