Paper Citation Record · LEDGER

Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1210.3578.

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

pith.paper-citation-record.v1
1210.3578 v2

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:16:05.813249Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

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External citation measurements

134
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d1bc6439-818d-4d3c-8ddf-402b039106d1 · inbound

Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy cites this paper.

Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T14:26:32.135862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f204ea8-eada-4842-aa4a-a2fd59a68926 · inbound

Searching beyond the fiducial stochastic gravitational wave background in pulsar timing array data using likelihood reweighting cites this paper.

Searching beyond the fiducial stochastic gravitational wave background in pulsar timing array data using likelihood reweighting Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-16T05:16:05.813249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0291d45a-20be-40be-9e72-806c836036f4 · inbound

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis cites this paper.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:37.878500Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6142079-44a4-4ef6-ae55-9b8c70ffb222 · inbound

Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy cites this paper.

Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:16:13.870449Z

Source-reported events for the cited work

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Observation 461b2d05-973a-422c-865d-1f0c5f806608 · inbound

Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data cites this paper.

Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:01:13.833564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 206e4d0e-2c63-400a-9a8c-f09198f5656c · inbound

Non-stationary noise in gravitational wave analyses: The wavelet domain noise covariance matrix cites this paper.

Non-stationary noise in gravitational wave analyses: The wavelet domain noise covariance matrix Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-03T22:25:51.146456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 54c43271-e200-41b5-93e7-1a4b7837ba3e · inbound

A practical theorem on gravitational-wave background statistics cites this paper.

A practical theorem on gravitational-wave background statistics Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-11T13:26:06.012392Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 4c0cc5f4-3e84-454f-9b7a-96a58d198249 · inbound

Temporal Correlation Statistic for Intrinsic Phase Fluctuation in Double White Dwarf Gravitational-Wave Signals cites this paper.

Temporal Correlation Statistic for Intrinsic Phase Fluctuation in Double White Dwarf Gravitational-Wave Signals Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-07-04T21:00:09.026855Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 953fd68f-8c65-4593-9c76-701d4daf56ab · 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 Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 244

Resolution: verified exact; local_arxiv, observed 2026-06-30T00:44:06.276940Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 387edd83-dd24-4ed3-b4c0-66a0b7382896 · inbound

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models cites this paper.

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 253

Resolution: verified exact; local_arxiv, observed 2026-06-30T01:24:08.853522Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation a773f742-9bb9-41bb-b09c-85a6e7cb6869 · inbound

Evaluating the Fourier Approximation in Pulsar Timing Array Analysis cites this paper.

Evaluating the Fourier Approximation in Pulsar Timing Array Analysis Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-06-30T16:14:54.031596Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation ebd50c41-6474-461a-ad59-f32f727cbf3b · inbound

Population statistics of nanohertz gravitational wave sources cites this paper.

Population statistics of nanohertz gravitational wave sources Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-07-09T09:56:10.552759Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation efe9cc4a-4296-43ce-ac4c-d067cf6a2166 · inbound

Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays cites this paper.

Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T17:59:59.038401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c1efc5b-dd2e-480a-afce-cee0ffa93e09 · inbound

Insights into the Pulsar Timing Array hypothesis space cites this paper.

Insights into the Pulsar Timing Array hypothesis space Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T04:18:59.874286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.