Paper Citation Record · LEDGER

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

As of 18 August 2026, this Paper Citation Record lists 35 of 35 outbound references and 21 inbound Pith citation observations for arXiv:2506.13866.

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

pith.paper-citation-record.v1
2506.13866 v1

Coverage vector

measured 35 of 35 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:33:39.277066Z

measured 56 of 56 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 21 of 21 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T14:35:53.614876Z

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

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation bae195a6-9d24-46b3-bff3-d58a4ab159ed · outbound

This paper cites Timing a millisecond pulsar array,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Timing a millisecond pulsar array,

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:44.473594Z

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Observation f3f38aaa-7993-419d-b7a9-e205d549e91f · outbound

This paper cites Constructing a Pulsar Timing Array,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Constructing a Pulsar Timing Array,

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:44.203949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 94ced665-622d-4fe3-879c-e99f8bcba124 · outbound

This paper cites Upper limits on the isotropic gravitational radiation background from pulsar timing analysis,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Upper limits on the isotropic gravitational radiation background from pulsar timing analysis,

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:43.896646Z

Source-reported events for the cited work

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Observation 3299f16f-3e7a-47d0-acad-5608160b3e5f · outbound

This paper cites Expected properties of the first gravitational wave signal detected with pulsar timing arrays,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Expected properties of the first gravitational wave signal detected with pulsar timing arrays,

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:43.626225Z

Source-reported events for the cited work

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Observation 239a2b98-4136-4158-9fa0-f62f3d862c69 · outbound

This paper cites Optimal strategies for gravitational wave stochastic background searches in pulsar timing data.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Optimal strategies for gravitational wave stochastic background searches in pulsar timing data

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:35.482158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e613b48-5ebe-4ee1-a7cc-ddc6a3b3af6d · outbound

This paper cites Time-domain Implementation of the Optimal Cross-Correlation Statistic for Stochastic Gravitational-Wave Background Searches in Pulsar Timing Data.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Time-domain Implementation of the Optimal Cross-Correlation Statistic for Stochastic Gravitational-Wave Background Searches in Pulsar Timing Data

Reference 6

Resolution: malformed identifier; no resolver link, observed 2026-08-07T00:33:35.644793Z

Source-reported events for the cited work

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Observation 823ec605-36f4-41ce-a9d1-6ac57132981c · outbound

This paper cites Noise-marginalized optimal statistic: A robust hybrid frequentist-Bayesian statistic for the stochastic gravitational-wave background in pulsar timing arrays.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Noise-marginalized optimal statistic: A robust hybrid frequentist-Bayesian statistic for the stochastic gravitational-wave background in pulsar timing arrays

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:35.752683Z

Source-reported events for the cited work

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Observation 372a0eab-01dc-4e0d-bc3a-0e2b6bc2db12 · outbound

This paper cites Detection methods for stochastic gravitational-wave backgrounds: a unified treatment.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Detection methods for stochastic gravitational-wave backgrounds: a unified treatment

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:35.929922Z

Source-reported events for the cited work

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Observation 082a750a-0365-47bb-8cd9-768318f45d0b · outbound

This paper cites an unresolved cited work.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Unresolved cited work

Reference 9

Resolution: unresolved; raw_fallback, observed 2026-08-07T00:33:43.350171Z

Source-reported events for the cited work

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Observation dd8a6dbe-b1b8-4b10-9f9e-f65494c08a7c · outbound

This paper cites Low-rank approximations for large stationary covariance matrices, as used in the Bayesian and generalized-least-squares analysis of pulsar-timing data.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Low-rank approximations for large stationary covariance matrices, as used in the Bayesian and generalized-least-squares analysis of pulsar-timing data

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:36.164758Z

Source-reported events for the cited work

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Observation 26a54b0d-4399-4e12-83d7-5014a68bcbc7 · outbound

This paper cites Realistic sensitivity curves for pulsar timing arrays.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Realistic sensitivity curves for pulsar timing arrays

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:36.342880Z

Source-reported events for the cited work

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Observation 0c422e41-9bef-4b07-b46f-1aea4ac0ab20 · outbound

This paper cites Pulsar timing array sensitivity to anisotropies in the gravitational wave background.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:36.426292Z

Source-reported events for the cited work

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Observation 8e42e1ae-da05-4364-8b6b-fadf0e664b24 · outbound

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

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Mitigating cosmic variance in the Hellings-Downs curve: a Cosmic Microwave Background analogy

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:36.546722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4f42fbfb-6e16-48e9-9c59-9ccf80dfd59f · outbound

This paper cites Accurate pulsar timing array residual variances and correlation of the stochastic gravitational wave background,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Accurate pulsar timing array residual variances and correlation of the stochastic gravitational wave background,

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:36.686612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a330851-4145-4c80-8df5-faaea39c8cc6 · outbound

This paper cites ENTERPRISE: Enhanced Numerical Toolbox Enabling a Robust PulsaR Inference SuitE,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis ENTERPRISE: Enhanced Numerical Toolbox Enabling a Robust PulsaR Inference SuitE,

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:43.015022Z

Source-reported events for the cited work

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Observation 109348ec-02ef-4df6-9cdd-305c5f04b4b3 · outbound

This paper cites DISCOVERY: the next-generation pulsar-timing-array data-analysis package,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis DISCOVERY: the next-generation pulsar-timing-array data-analysis package,

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:42.845949Z

Source-reported events for the cited work

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Observation ebc2b074-0300-455e-ae08-36b3670032d7 · outbound

This paper cites JAX: composable transformations of Python+NumPy programs,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis JAX: composable transformations of Python+NumPy programs,

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:42.506998Z

Source-reported events for the cited work

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Observation 9ae47fb1-5a64-462e-888e-bcb7045051fa · outbound

This paper cites Automatic differentiation in machine learning: a survey,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Automatic differentiation in machine learning: a survey,

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:42.217599Z

Source-reported events for the cited work

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Observation d0316245-2091-4bcd-9e13-c613eb72e6b5 · outbound

This paper cites The No-U-Turn sampler: adaptively setting path lengths in Hamiltonian Monte Carlo,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The No-U-Turn sampler: adaptively setting path lengths in Hamiltonian Monte Carlo,

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:42.036060Z

Source-reported events for the cited work

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Observation df757220-19bd-416e-937d-07cf7decb789 · outbound

This paper cites Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Composable Effects for Flexible and Accelerated Probabilistic Programming in NumPyro

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:37.354632Z

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Observation e1c59592-2967-4e3f-ac0f-c6f656b8af3c · outbound

This paper cites Pyro: Deep universal probabilistic programming,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Pyro: Deep universal probabilistic programming,

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:41.565685Z

Source-reported events for the cited work

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Observation a1ed8636-29e0-425c-af75-cbd5501e57b7 · outbound

This paper cites On measuring the gravitational-wave background using Pulsar Timing Arrays.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis On measuring the gravitational-wave background using Pulsar Timing Arrays

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:37.623481Z

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Observation d2a59d70-c5a9-4fee-9146-dc76a3fb8d90 · outbound

This paper cites The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:37.735329Z

Source-reported events for the cited work

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

This paper cites Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data.

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

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Observation 98e66c6c-8307-452f-bede-db4cdb2c4d7b · outbound

This paper cites Understanding and analysing time-correlated stochastic signals in pulsar timing.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Understanding and analysing time-correlated stochastic signals in pulsar timing

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:37.968332Z

Source-reported events for the cited work

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Observation 3d4469b8-b1d0-4fae-8474-b7854b09f40a · outbound

This paper cites New advances in the Gaussian-process approach to pulsar-timing data analysis.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis New advances in the Gaussian-process approach to pulsar-timing data analysis

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.074904Z

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Observation 2497235b-6e11-492f-899f-d03359c5569b · outbound

This paper cites The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.197810Z

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Observation 1d5868f3-519a-40bd-8a3c-f9408dd764c9 · outbound

This paper cites The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.370193Z

Source-reported events for the cited work

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Observation fb3780ea-de18-497e-8808-2681a4b60cd1 · outbound

This paper cites Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.524168Z

Source-reported events for the cited work

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Observation 60ca9677-2d8c-443d-9eef-abe4ae915049 · outbound

This paper cites The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.634761Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fa34420-36e6-41b1-baa5-bff12fb1a1b9 · outbound

This paper cites Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:38.703944Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1e8c2e5-3f52-482b-bff5-d2ea7257ac1e · outbound

This paper cites Fourier’s Series,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Fourier’s Series,

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:41.214769Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b4e95ae8-8ba9-420b-a802-59f64dced6c7 · outbound

This paper cites On a certain periodic function,.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis On a certain periodic function,

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:40.957402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 54eec3b2-d462-4223-a73c-3db3269987aa · outbound

This paper cites Strang, Introduction to Applied Mathematics.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis Strang, Introduction to Applied Mathematics

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T00:33:40.763336Z

Source-reported events for the cited work

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Observation 7babd853-7931-4522-bf5b-d8ab4f411c3a · outbound

This paper cites The NANOGrav 15-year Gravitational-Wave Background Methods.

Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis The NANOGrav 15-year Gravitational-Wave Background Methods

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T00:33:39.277066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 4595cdd0-4d3a-4b43-b483-cfae610fecb0 · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 59

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Observation c70e0316-1fe0-4081-b419-5cbf6300c612 · inbound

Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic cites this paper.

Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 61

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Observation ebabde58-62b1-4bf6-8bf9-e160f847f447 · inbound

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization cites this paper.

Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 79

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Observation 2c67f2c9-d003-42e7-adcd-a1154fc1fa70 · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 93

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Observation ef1bdd23-7d4f-4c28-8392-6e7a154374d9 · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 62

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Source-reported events for the cited work

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Observation 046cef3a-2767-461c-a51c-ad005732396f · inbound

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background cites this paper.

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-05-21T19:04:19.023765Z

Source-reported events for the cited work

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Observation c72e66d6-c467-4ef3-9f89-c4769f698057 · inbound

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background cites this paper.

Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-03T22:40:19.142561Z

Source-reported events for the cited work

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Observation 118a01b8-91a3-48b9-bfb9-c692a8f90342 · inbound

Data span and frequency coverage requirements for robust detection and inference in PTAs: A case study with EPTA DR2 cites this paper.

Data span and frequency coverage requirements for robust detection and inference in PTAs: A case study with EPTA DR2 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-03T19:58:06.620381Z

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Observation ff465348-5c0c-4320-9cf3-dc152b34408b · inbound

Stochastic gravitational-wave background search using data from five pulsar timing arrays cites this paper.

Stochastic gravitational-wave background search using data from five pulsar timing arrays Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-17T00:08:43.411184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 2b3dc2f5-d708-41db-8099-d7e6ee68c871 · inbound

Timing Gamma-ray Pulsars using Gibbs Sampling cites this paper.

Timing Gamma-ray Pulsars using Gibbs Sampling Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-21T16:10:20.344542Z

Source-reported events for the cited work

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Observation 6be38fdf-c299-40b8-97dd-1820ddee9d8f · inbound

Stochastic problems in pulsar timing cites this paper.

Stochastic problems in pulsar timing Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 41

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T05:21:01.932099Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 01570339-e0e7-499e-a46d-c7137eacad57 · inbound

A comprehensive framework for phase-coherent mapping of the gravitational-wave sky with pulsar timing arrays cites this paper.

A comprehensive framework for phase-coherent mapping of the gravitational-wave sky with pulsar timing arrays Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-05-10T02:32:49.705650Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a94b0937-1dce-48fa-83f4-00aec324c557 · inbound

Are PTA measurements sensitive to gravitational wave non-Gaussianities? cites this paper.

Are PTA measurements sensitive to gravitational wave non-Gaussianities? Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 79

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:06:08.775654Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 22a009f3-bcb1-40e5-b0d2-0170d14b1059 · inbound

Are PTA measurements sensitive to gravitational wave non-Gaussianities? cites this paper.

Are PTA measurements sensitive to gravitational wave non-Gaussianities? Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 79

Resolution: verified exact; arxiv_id, observed 2026-06-30T23:15:07.560809Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 796fe9f5-45e2-4000-ad6f-a567916415c0 · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 271

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T00:44:05.742610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b1f77a3f-e5b6-4219-bda6-f979307257ef · inbound

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

The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 269

Resolution: metadata mismatch; arxiv_id, observed 2026-06-30T01:24:08.949466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ea581edf-accf-4e9a-95a2-b5998b065eee · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 114

Resolution: metadata mismatch; local_arxiv, observed 2026-07-07T23:34:19.410319Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f2bdd64e-59aa-48e0-840c-957d81ef32bb · inbound

A new framework for lightning-fast gravitational wave analysis of pulsar timing data cites this paper.

A new framework for lightning-fast gravitational wave analysis of pulsar timing data Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 88

Resolution: verified exact; local_arxiv, observed 2026-07-10T20:27:36.663644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9f5e5a2b-61f0-481d-9044-9b74a60a2a64 · inbound

Modeling non-stationary noise: applications in gravitational wave astronomy cites this paper.

Modeling non-stationary noise: applications in gravitational wave astronomy Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T06:07:45.808211Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09b08869-d1a2-488f-8684-2562b20581cf · inbound

Directional Anisotropic Sensitivity Curves for Pulsar Timing Arrays cites this paper.

Directional Anisotropic Sensitivity Curves for Pulsar Timing Arrays Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-04T01:00:57.202952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aca9b29f-73d7-41de-9391-9dfd0a0d6b77 · 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 Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T17:59:59.046390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.