Paper Citation Record · LEDGER

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:1908.00546.

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

pith.paper-citation-record.v1
1908.00546 v2

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measured 15 of 15 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:30:21.079126Z

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

Source: arxiv_reference, observed 2026-07-03T02:17:35.065778Z

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Outbound references

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Pith citing papers

Observation a89f5169-a34e-4d4a-bc2a-6595c1b3a269 · inbound

New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions cites this paper.

New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 215

Resolution: verified exact; arxiv_id, observed 2026-05-23T22:35:50.563416Z

Source-reported events for the cited work

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Observation 21381778-2f39-4dd1-9c4d-e5918990ea80 · inbound

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order cites this paper.

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 120

Resolution: verified exact; arxiv_id, observed 2026-05-22T01:55:55.846896Z

Source-reported events for the cited work

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Observation 56964f6d-e13e-4705-a550-4cbbddc95211 · inbound

GW170817 Viable Einstein-Gauss-Bonnet Inflation Compatible with the Atacama Cosmology Telescope Data cites this paper.

GW170817 Viable Einstein-Gauss-Bonnet Inflation Compatible with the Atacama Cosmology Telescope Data LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T05:30:21.079126Z

Source-reported events for the cited work

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Observation e9bd8972-c101-4ec6-b23f-d915e648fabd · inbound

The Persistence of Nonlinear Gravitational Wave Memory cites this paper.

The Persistence of Nonlinear Gravitational Wave Memory LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-06T22:57:37.365225Z

Source-reported events for the cited work

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Observation 8ee7b311-a355-49bc-9ab4-a01f3c340e12 · inbound

Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter cites this paper.

Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T11:25:20.930060Z

Source-reported events for the cited work

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Observation 48188199-6486-4471-a0fe-554d434e6082 · 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 LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T07:36:36.567916Z

Source-reported events for the cited work

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Observation 44e47412-5d91-470d-8c82-67294f94ac38 · inbound

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings cites this paper.

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-21T19:14:19.291566Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 7b4d2d13-ab76-4d92-85b8-60eec5ab8b7e · inbound

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings cites this paper.

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-04T00:32:12.976237Z

Source-reported events for the cited work

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Observation 92c7240b-1750-4d09-bd88-74ffb44643f6 · inbound

Bayesian analysis of the complex singlet model with phase transition gravitational waves cites this paper.

Bayesian analysis of the complex singlet model with phase transition gravitational waves LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-21T17:54:18.485998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 134413b3-fe7a-43ee-ac09-0680986e60a2 · inbound

Bayesian analysis of the complex singlet model with phase transition gravitational waves cites this paper.

Bayesian analysis of the complex singlet model with phase transition gravitational waves LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T20:05:43.660492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a721cf67-eef8-4572-b136-c86194c76dc4 · inbound

Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors cites this paper.

Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T17:45:19.412677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b3a55af-9c87-4b76-b6e6-47aa8a56bf54 · inbound

PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference cites this paper.

PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 45

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:17:35.067200Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 480e7f3c-aea4-4283-8d19-14104049d331 · inbound

Construction of Sensitivity Curves for Dynamic LISA and Taiji cites this paper.

Construction of Sensitivity Curves for Dynamic LISA and Taiji LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-01T17:35:51.886119Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 2362fe0d-e54e-4016-bbd8-672d1dea5482 · inbound

LISA Reconstruction Landscape for Metastable Cosmic Strings cites this paper.

LISA Reconstruction Landscape for Metastable Cosmic Strings LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 85

Resolution: unresolved; no resolver link, observed 2026-07-31T02:53:21.819893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae67b8e1-705a-40ce-9311-44ada1a58290 · inbound

From Quantum Correlations to Inflationary Tracking Scalar Field Evolution cites this paper.

From Quantum Correlations to Inflationary Tracking Scalar Field Evolution LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T00:31:00.535646Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.