Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0104266.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T15:56:28.308376Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-25T07:35:29.087783Z
Reference resolution
0 of 0 outbound references displayed
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- 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 dd5c49c4-faf8-4fad-b94a-bf958ee41cee · inbound
LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources cites this paper.
LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T15:56:28.308376Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6707ed5a-f170-4c95-b0ad-ce6535339119 · inbound
Enhancing Taiji's Parameter Estimation under Non-Stationarity: a Time-Frequency Domain Framework for Galactic Binaries and Instrumental Noises cites this paper.
Enhancing Taiji's Parameter Estimation under Non-Stationarity: a Time-Frequency Domain Framework for Galactic Binaries and Instrumental Noises Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Reference 97
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T04:28:58.844871Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 32dae270-daa3-41e8-b0a2-7cd476ac750a · inbound
Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison cites this paper.
Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Reference 270
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T23:25:36.932833Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50ddeb15-433b-47fd-b57b-8609bdc6c541 · inbound
Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors cites this paper.
Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T07:36:36.488480Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc0db034-f2c9-4a45-9462-fb895b72a591 · inbound
Model Parameter Reconstruction of Electroweak Phase Transition with TianQin and LISA: Insights from the Dimension-Six Model cites this paper.
Model Parameter Reconstruction of Electroweak Phase Transition with TianQin and LISA: Insights from the Dimension-Six Model Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration
Reference 71
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T07:35:29.090845Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.