Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
PINT: Maximum-likelihood estimation of pulsar timing noise parameters
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2405.01977.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T15:30:15.735333Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T16:16:07.265039Z
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 59b374e6-3269-4a75-b45b-9d4170331e08 · inbound
\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors cites this paper.
\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors PINT: Maximum-likelihood estimation of pulsar timing noise parameters
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:30:15.735333Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 91167255-b274-4c48-9754-e27139704bbe · inbound
Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333 cites this paper.
Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333 PINT: Maximum-likelihood estimation of pulsar timing noise parameters
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T16:16:07.269849Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 2c7a0492-5395-4ea4-ae4e-cecaedb77072 · inbound
PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures cites this paper.
PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures PINT: Maximum-likelihood estimation of pulsar timing noise parameters
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T06:30:42.446982Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d67894f8-8673-45c2-934f-c708e6ea3fe9 · inbound
PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures cites this paper.
PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures PINT: Maximum-likelihood estimation of pulsar timing noise parameters
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:03:27.559681Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.