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Paper Citation Record · LEDGER

PINT: Maximum-likelihood estimation of pulsar timing noise parameters

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.01977.

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

pith.paper-citation-record.v1
2405.01977 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T23:06:25.762597Z

measured 0 of 1 external citation measurements

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

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  • verified fuzzy0
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  • malformed identifier0
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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 5fb04c6c-9cdd-4bdc-91ef-6c5b67bd8dbd · inbound

A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing cites this paper.

A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing PINT: Maximum-likelihood estimation of pulsar timing noise parameters

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-11T23:06:25.762597Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T23:06:25.762597Z digest=sha256:866f0f258428b6b1732e4c319aafc1edfc46fc0f97b8cdfbbcd80af85d439825

Observation 58603a0c-b655-4ab4-86d0-e5acebab8160 · inbound

Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data cites this paper.

Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data PINT: Maximum-likelihood estimation of pulsar timing noise parameters

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-11T20:47:19.962154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T20:47:19.962154Z digest=sha256:e4205c7ca500d33104876a9cba5f88b3f710216973033b46a02ceaae0e3993cf

Observation 366da0a0-ac76-400d-ad7f-099d57764420 · inbound

Regularizing the Pulsar Timing Array likelihood: A path towards Fourier Space cites this paper.

Regularizing the Pulsar Timing Array likelihood: A path towards Fourier Space PINT: Maximum-likelihood estimation of pulsar timing noise parameters

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-11T14:35:53.571168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:35:53.571168Z digest=sha256:b6c59455fa20ca2ee8f3e029be0e6ab4325aeb536288d483772fb788c6934667

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.

source=pdf_text observed=2026-08-06T15:30:15.735333Z digest=sha256:da24ee37a472d137d5611fed371ef30c7b513e7861705dcf4fc4b5c181bc6825

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 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-09T18:22:31.315236Z digest=sha256:a2d5fc7e79dbbdbbc5bf451755a2aca2486c8fb465dd15840462d7ebf86d1b5c

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.

source=arxiv_source observed=2026-08-02T06:30:42.446982Z digest=sha256:425c7f00d925a3f36335817a5f7cab6b91b4e52460fd1ed316b57ee2a593eef0

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.

source=arxiv_source observed=2026-08-03T02:03:27.559681Z digest=sha256:566b8e7a0ebdc698a572d3cf731b390e8f20c7de99f4e304ad1b683e780286e9