Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Estimating the sensitivity of pulsar timing arrays
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1406.5199.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T19:07:26.462338Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T01:24:08.929088Z
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 a55a4e69-abef-454e-9912-6e36c22164a1 · inbound
New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions cites this paper.
New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions Estimating the sensitivity of pulsar timing arrays
Reference 203
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T22:35:50.507447Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 17a4deb1-b10f-4035-a25d-86b78e46783a · inbound
Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites cites this paper.
Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites Estimating the sensitivity of pulsar timing arrays
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T05:13:56.246138Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation af5ee59c-6128-4d8c-9815-1cf76bac7a37 · inbound
Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves cites this paper.
Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Estimating the sensitivity of pulsar timing arrays
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T19:07:26.462338Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2605fabd-8e9e-4fd9-a818-c210a50d2a69 · inbound
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays cites this paper.
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays Estimating the sensitivity of pulsar timing arrays
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T14:11:04.296029Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 6fac2ae8-8e41-43fe-8b8d-c99641b6c322 · inbound
Forecasting graviton-mass constraints from the full covariance of PTA-astrometry ORF estimators cites this paper.
Forecasting graviton-mass constraints from the full covariance of PTA-astrometry ORF estimators Estimating the sensitivity of pulsar timing arrays
Reference 53
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T20:56:10.134275Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 6e6a4d2a-a5fe-47d2-804a-14f01a6bd440 · inbound
The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses cites this paper.
The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses Estimating the sensitivity of pulsar timing arrays
Reference 136
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T00:44:05.848109Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 4482d7ab-6f7b-4e16-9f23-ec3e6beacd37 · inbound
The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models cites this paper.
The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models Estimating the sensitivity of pulsar timing arrays
Reference 146
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T01:24:08.935838Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation da6af2b2-4feb-41ec-9342-b0ec3ae6cd56 · inbound
A Non-Holomorphic Modular $A_4$ Framework for Resonant Leptogenesis with Gravitational Wave Signatures cites this paper.
A Non-Holomorphic Modular $A_4$ Framework for Resonant Leptogenesis with Gravitational Wave Signatures Estimating the sensitivity of pulsar timing arrays
Reference 148
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:27:37.555144Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.