Paper Citation Record · LEDGER

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

As of 23 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 21 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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Pith citing papers itemized under the disclosed page cap.

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

Reference resolution

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Outbound references

Observation 13d91e6c-a428-4dd0-8fe7-50f90fa67864 · outbound

This paper cites an unresolved cited work.

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

Reference 1

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Observation 7ed29ea8-0722-411d-b1a9-422fd3efdd89 · outbound

This paper cites an unresolved cited work.

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

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-14T15:56:28.849171Z

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Observation a15f48d6-596c-4547-b94b-c2f048f4f603 · outbound

This paper cites an unresolved cited work.

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

Reference 3

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Observation 81f41807-9f75-4114-8e30-a038f1811e65 · outbound

This paper cites Combining all of these terms and summing over i and j we then ﬁnd σ2 =⟨ ˆC2⟩ = 1 2 ∫ T/2 −T/2 [N(t1−t2)N(t′ 1−t′.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Combining all of these terms and summing over i and j we then ﬁnd σ2 =⟨ ˆC2⟩ = 1 2 ∫ T/2 −T/2 [N(t1−t2)N(t′ 1−t′

Reference 4

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Observation 5fcfcd26-d026-4531-816e-eab090fb5265 · outbound

This paper cites the duty cycle of usable science data at full (nominal) performance shall be greater than 75%,.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources the duty cycle of usable science data at full (nominal) performance shall be greater than 75%,

Reference 5

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Observation 2f9a29f3-5125-43e7-ab55-59edb376d17b · outbound

This paper cites an unresolved cited work.

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

Reference 6

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Observation f9d608f7-2c09-4320-aaae-bad8a5e2b36d · outbound

This paper cites This gives the integrated sensitivity curve.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources This gives the integrated sensitivity curve

Reference 7

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Observation 6c029727-6ed2-4a5f-a9ab-b843914eed04 · outbound

This paper cites Laser Interferometer Space Antenna.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Laser Interferometer Space Antenna

Reference 8

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Observation c8b0c2a1-16f5-4538-ac79-7ac13b3e71c0 · outbound

This paper cites Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities

Reference 9

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Observation b245b443-da6a-4427-93d5-83d2e241e7b9 · outbound

This paper cites Gravitational Wave Experiments and Early Universe Cosmology.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Gravitational Wave Experiments and Early Universe Cosmology

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.262955Z

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Observation 5188936d-7386-4229-834a-d5d8b8c237c0 · outbound

This paper cites Space missions to detect the cosmic gravitational-wave background.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Space missions to detect the cosmic gravitational-wave background

Reference 11

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Observation 38620eb1-a140-4ea5-a3ce-38d5fcfdf6d6 · outbound

This paper cites Detecting a stochastic gravitational wave background with the Laser Interferometer Space Antenna.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Detecting a stochastic gravitational wave background with the Laser Interferometer Space Antenna

Reference 12

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Observation 64f05e47-3a5f-4366-86c1-13645ddf58c8 · outbound

This paper cites Gravitational-wave sensitivity curves.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Gravitational-wave sensitivity curves

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.276188Z

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Observation 38455a5c-8024-4ab5-82db-d050785c28b2 · outbound

This paper cites Sensitivity curves for searches for gravitational-wave backgrounds.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Sensitivity curves for searches for gravitational-wave backgrounds

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.280784Z

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Observation d54bdf69-508a-4de4-a5ae-25c41e12c79e · outbound

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

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Detection methods for stochastic gravitational-wave backgrounds: a unified treatment

Reference 15

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Observation e3db4411-8a57-416f-aaae-b3d01cd15cab · outbound

This paper cites Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories

Reference 16

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Observation fde15ceb-aa05-4692-9a9f-11e85f2a5026 · outbound

This paper cites an unresolved cited work.

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

Reference 17

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Observation 97dacd06-2461-4ce3-8bfb-55ca6556a4d0 · outbound

This paper cites Tinto, F.

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

Reference 18

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Observation e349e9af-03fc-4c8f-9d2a-f4e6b7dbee0b · outbound

This paper cites The LISA Optimal Sensitivity.

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

Reference 19

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Observation 14cf27ed-e303-47c3-9904-75cf50540158 · outbound

This paper cites The Effects of Orbital Motion on LISA Time Delay Interferometry.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources The Effects of Orbital Motion on LISA Time Delay Interferometry

Reference 20

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Observation dd5c49c4-faf8-4fad-b94a-bf958ee41cee · outbound

This paper cites Estimating Stochastic Gravitational Wave Backgrounds with Sagnac Calibration.

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

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Observation 7ef9ea2a-ede0-44e4-827c-e15c6a9dd950 · outbound

This paper cites Detection of Anisotropies in the Gravitational-Wave Stochastic Background.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Detection of Anisotropies in the Gravitational-Wave Stochastic Background

Reference 22

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Observation f390cbbc-308e-43d1-b2f3-4bb0d4aebd5d · outbound

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

Reference 23

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Observation 9161c428-dc13-42ae-b7d8-e2d44d16b6fa · outbound

This paper cites Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?

Reference 24

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Observation 8ea7589b-10db-41c8-a4c5-1b162a8ed27d · outbound

This paper cites Realistic sensitivity curves for pulsar timing arrays.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Realistic sensitivity curves for pulsar timing arrays

Reference 25

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Observation 5b34d669-907c-47f0-9f1f-62f9a39ca8b8 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Planck 2018 results. VI. Cosmological parameters

Reference 26

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Observation 51288ee1-96af-4b96-bfac-3c7b4f55afd8 · outbound

This paper cites Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.332215Z

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Observation 39b863da-acc1-47bb-a61c-c402b4d252ba · outbound

This paper cites Probing the Universe through the Stochastic Gravitational Wave Background.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Probing the Universe through the Stochastic Gravitational Wave Background

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.335987Z

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Observation 93772979-0c8c-4d8e-aadc-fa27920f2a91 · outbound

This paper cites Assessing the detectability of a Stochastic Gravitational Wave Background with LISA, using an excess of power approach.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Assessing the detectability of a Stochastic Gravitational Wave Background with LISA, using an excess of power approach

Reference 29

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This paper cites Reconstructing the spectral shape of a stochastic gravitational wave background with LISA.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Reconstructing the spectral shape of a stochastic gravitational wave background with LISA

Reference 30

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Observation 6010d599-362a-4074-84b0-49042711a254 · outbound

This paper cites Fisher Matrices and Confidence Ellipses: A Quick-Start Guide and Software.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Fisher Matrices and Confidence Ellipses: A Quick-Start Guide and Software

Reference 31

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Observation e4fe8bb4-29ce-4818-b05f-5866ef3aca3f · outbound

This paper cites The construction and use of LISA sensitivity curves.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources The construction and use of LISA sensitivity curves

Reference 32

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Observation 2a4519df-c733-4ba0-aa71-1340b7205540 · outbound

This paper cites Observation of Gravitational Waves from a Binary Black Hole Merger.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 33

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This paper cites The promise of multi-band gravitational wave astronomy.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources The promise of multi-band gravitational wave astronomy

Reference 34

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

Reference 35

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Observation 987d8a70-f68e-4a75-aa63-763d0455e236 · outbound

This paper cites General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T15:56:28.368975Z

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This paper cites Prospects for Gravitational Wave Measurement of ZTFJ1539+5027.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources Prospects for Gravitational Wave Measurement of ZTFJ1539+5027

Reference 37

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This paper cites TianQin: a space-borne gravitational wave detector.

LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources TianQin: a space-borne gravitational wave detector

Reference 38

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

Reference 39

Resolution: unresolved; raw_fallback, observed 2026-08-14T15:56:28.722075Z

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Observation ce63edf2-892f-422b-b1a4-0a5dc9c5f759 · outbound

This paper cites an unresolved cited work.

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

Reference 40

Resolution: unresolved; raw_fallback, observed 2026-08-14T15:56:28.709938Z

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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

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Observation 7a1906a1-52e9-425e-b342-c7bb966769a4 · inbound

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum cites this paper.

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T04:42:52.330689Z

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Observation 2568302a-d171-4870-b77d-64509ba26754 · inbound

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Testing inflation on all scales: a case study with $\alpha$-attractors LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 131

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Observation fa2656b2-581d-4a2a-878e-e816fef42f25 · inbound

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PhaseTracer2: from the effective potential to gravitational waves LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 88

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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

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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

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Observation d123bc8d-fae7-4147-a058-fc62d3eff65c · inbound

A Fog Over the Cosmological SGWB: Unresolved Massive Black Hole Binaries in the LISA Band cites this paper.

A Fog Over the Cosmological SGWB: Unresolved Massive Black Hole Binaries in the LISA Band LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 58

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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

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

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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

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Observation 48188199-6486-4471-a0fe-554d434e6082 · inbound

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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

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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 2026-08-23T06:30:58.430688+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

Unavailable: canonical work link unavailable.

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 2026-08-23T06:30:58.430688+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 2026-08-23T06:30:58.430688+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 2026-08-23T06:30:58.430688+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.

Observation 7ffa8d0e-9fd3-45df-82b6-250471bcccfe · inbound

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation cites this paper.

Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T10:59:30.801673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7739cf3b-c74d-4b8f-97d1-195b5886caa5 · inbound

Full-Covariance Bayesian Inference of Stochastic Gravitational Wave Backgrounds with Time-Domain Simulations for Taiji-like Missions cites this paper.

Full-Covariance Bayesian Inference of Stochastic Gravitational Wave Backgrounds with Time-Domain Simulations for Taiji-like Missions LISA for Cosmologists: Calculating the Signal-to-Noise Ratio for Stochastic and Deterministic Sources

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T14:19:05.604338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.