All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background | Paper Citation Record

Observation 8051ce0b-aadf-400d-b69c-ba9c7deb2522 · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 1

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Observation d97e4b1f-a5ed-4c8b-9931-6d17761c9add · outbound

This paper cites GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 2

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Observation 7d8e5597-3b91-4961-89c2-aaf27982aa14 · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 3

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Observation e9f072ac-afd5-478a-bbea-84b05cc6da45 · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 4

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Observation 70192357-0e87-4b79-8fd5-1ffdb1425d7a · outbound

This paper cites GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 5

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Observation 7478e8df-7047-4b95-9569-4bf0fb03d40c · outbound

This paper cites GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog

Reference 6

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Observation 92eb5c87-bc38-44e9-a9f6-a1f7a6930e21 · outbound

This paper cites Stochastic Gravitational Wave Backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Stochastic Gravitational Wave Backgrounds

Reference 7

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Observation 289c617d-927b-4bef-9e14-c0d4e8921724 · outbound

This paper cites Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects

Reference 8

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Observation 0e2a6001-c389-460f-9f62-ff61b4b42d4e · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Detection methods for stochastic gravitational-wave backgrounds: a unified treatment

Reference 9

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Observation 2e27cf88-0add-4e42-9703-c1035fbd19a1 · outbound

This paper cites Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run

Reference 10

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Observation 0dcc1955-da72-43f3-a108-83aac53ef88a · outbound

This paper cites Abbottet al.(KAGRA, Virgo, LIGO Scientific), Phys.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Abbottet al.(KAGRA, Virgo, LIGO Scientific), Phys

Reference 11

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Observation 99bdbf41-d6f1-42c9-bfbc-9fdcfeccbe63 · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities

Reference 12

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Observation 06820deb-4030-4122-9e44-4d1d7396e31c · outbound

This paper cites Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background

Reference 13

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Observation 5b8b79c1-ef38-4ebb-93d6-ef49506ad20d · outbound

This paper cites Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches

Reference 14

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Observation 9b727d83-c625-4632-9756-f909284fc7ca · outbound

This paper cites Detection methods for non-Gaussian gravitational wave stochastic backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Detection methods for non-Gaussian gravitational wave stochastic backgrounds

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.433719Z

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Observation 2f4b54cb-dbd4-4e66-add2-01a2a9200d12 · outbound

This paper cites The optimal search for an astrophysical gravitational-wave background.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The optimal search for an astrophysical gravitational-wave background

Reference 16

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Observation f6e30f5d-12b8-489c-aec5-65fd40a8a06a · outbound

This paper cites Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds

Reference 17

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Observation 49893544-373f-49ec-9dd6-71e7c877b9f5 · outbound

This paper cites A stochastic search for intermittent gravitational-wave backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background A stochastic search for intermittent gravitational-wave backgrounds

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.449246Z

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Observation dcee96ee-a61e-48ea-b365-a89a57791015 · outbound

This paper cites Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge

Reference 19

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Observation c4573d1f-92f1-48ba-9a2f-6b813de9b753 · outbound

This paper cites Time-dependence of the astrophysical stochastic gravitational wave background.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Time-dependence of the astrophysical stochastic gravitational wave background

Reference 20

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Observation 89c0a7cf-f871-49b4-a076-872417662cca · outbound

This paper cites Non-Stationary Astrophysical Stochastic Gravitational-Wave Background: A New Probe to the High Redshift Population of Binary Black Holes.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Non-Stationary Astrophysical Stochastic Gravitational-Wave Background: A New Probe to the High Redshift Population of Binary Black Holes

Reference 21

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Observation b48ad393-2525-4c52-8729-9138483e86cf · outbound

This paper cites The First Upper Bound on the Non-Stationary Gravitational Wave Background and its Implication on the High Redshift Binary Black Hole Merger Rate.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The First Upper Bound on the Non-Stationary Gravitational Wave Background and its Implication on the High Redshift Binary Black Hole Merger Rate

Reference 22

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Observation 21f089d2-4eaf-4f74-91ac-58ecc54a4a7e · outbound

This paper cites A Semi-Parametric Approach to the Detection of Non-Gaussian Gravitational Wave Stochastic Backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background A Semi-Parametric Approach to the Detection of Non-Gaussian Gravitational Wave Stochastic Backgrounds

Reference 23

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Observation 8d53a671-9761-45e6-8501-a9f92be4d9a1 · outbound

This paper cites On the (In)Efficiency of the Cross-Correlation Statistic for Gravitational Wave Stochastic Background Signals with Non-Gaussian Noise and Heterogeneous Detector Sensitivities.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background On the (In)Efficiency of the Cross-Correlation Statistic for Gravitational Wave Stochastic Background Signals with Non-Gaussian Noise and Heterogeneous Detector Sensitivities

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:23.699705Z

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Observation 328cdb66-3394-4b60-a54b-a1ea2b77c900 · outbound

This paper cites Liu and S.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Liu and S

Reference 25

Resolution: verified exact; raw_fallback, observed 2026-08-12T05:54:23.676370Z

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Observation 8f3aa34e-a067-439f-a7bb-65bb648244b0 · outbound

This paper cites Punturoet al., Class.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Punturoet al., Class

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.491063Z

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Observation 10c5dd67-12ab-474b-93ed-8254fa37abc1 · outbound

This paper cites Science with the Einstein Telescope: a comparison of different designs.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Science with the Einstein Telescope: a comparison of different designs

Reference 27

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Observation 579c4210-a092-42e6-b531-85c4bf8c9b13 · outbound

This paper cites The Science of the Einstein Telescope.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The Science of the Einstein Telescope

Reference 28

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Observation d80a4947-2967-4d49-aa5b-9503bdaf1460 · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 29

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Observation 3003b66f-e826-4e6d-b167-8a3da8383c67 · outbound

This paper cites A Horizon Study for Cosmic Explorer: Science, Observatories, and Community.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background A Horizon Study for Cosmic Explorer: Science, Observatories, and Community

Reference 30

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Observation b9a21474-ec13-46a7-a97f-cb1d44b0f187 · outbound

This paper cites Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee

Reference 31

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Observation 0a3a01b3-523b-4b8b-a759-8992be61e38c · outbound

This paper cites Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:23.516268Z

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Observation bba5db92-0b06-4bb4-bc29-1863357e7bdc · outbound

This paper cites Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors

Reference 33

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Observation a31a8e41-7fb7-4986-bfb5-dd579a03bc00 · outbound

This paper cites Zhong and V.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Zhong and V

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.532103Z

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Observation 1be27502-5ef6-45ba-8df1-1803c0edf0e6 · outbound

This paper cites Cosmological Backgrounds of Gravitational Waves.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Cosmological Backgrounds of Gravitational Waves

Reference 35

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Observation 9134e29b-808b-4f3d-9483-580dc9e5d6c1 · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Planck 2018 results. VI. Cosmological parameters

Reference 36

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Observation 16143bc7-0543-4a30-bd5e-8effafee1c11 · outbound

This paper cites Understanding $\Omega_\mathrm{gw}(f)$ in Gravitational Wave Experiments.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Understanding $\Omega_\mathrm{gw}(f)$ in Gravitational Wave Experiments

Reference 37

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Observation d680623b-ea41-49cc-911a-79d8571c3227 · outbound

This paper cites A thorough investigation of cross-correlation estimators for stochastic gravitational-wave background searches in ground-based detector data.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background A thorough investigation of cross-correlation estimators for stochastic gravitational-wave background searches in ground-based detector data

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:23.357827Z

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Observation 60a0fddf-2bf4-4fc5-94fb-521d126df6bf · outbound

This paper cites pygwb: Python-based library for gravitational-wave background searches.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background pygwb: Python-based library for gravitational-wave background searches

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.556999Z

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Observation 5b9cca82-4b56-4ff0-97e3-9f65d83c8bdf · outbound

This paper cites GWTC-5.0: Population Properties of Merging Compact Binaries.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background GWTC-5.0: Population Properties of Merging Compact Binaries

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.562752Z

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Observation f3387c0c-e90c-4c0d-a26c-4b9bec50c2b5 · outbound

This paper cites Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:23.304604Z

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Observation caf7ceba-35d6-489f-90c7-a20b6e9a0c93 · outbound

This paper cites The spectral density of astrophysical stochastic backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The spectral density of astrophysical stochastic backgrounds

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.572158Z

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Observation a1f4742f-641c-4963-90c4-ab84bbe08fbf · outbound

This paper cites Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.577509Z

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Observation 6fb8688b-2fff-458b-9c5c-8f41b4eb3d2a · outbound

This paper cites Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.582320Z

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Observation 337265b5-9b5f-4cbb-8866-e55cb94a71b9 · outbound

This paper cites The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors

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Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.587260Z

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Observation 352bf180-5935-480a-b6b2-e99b1f95b7a6 · outbound

This paper cites Projections of the uncertainty on the compact binary population background using popstock.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Projections of the uncertainty on the compact binary population background using popstock

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.592046Z

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Observation 77b4dd3c-60a7-4792-9c6a-7e9c22999b61 · outbound

This paper cites Ebersold and T.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Ebersold and T

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.597362Z

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Observation 7dd9aea5-66a9-4924-a50b-fe5a8f3402ec · outbound

This paper cites Spectral Variance in a Stochastic Gravitational-Wave Background From a Binary Population.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Spectral Variance in a Stochastic Gravitational-Wave Background From a Binary Population

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.601947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46fd026e-ec93-4fce-acf0-ae890c557d62 · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.606897Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97df58e1-c26e-4892-89f3-88e473704d66 · outbound

This paper cites Statistical properties of astrophysical gravitational-wave backgrounds.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Statistical properties of astrophysical gravitational-wave backgrounds

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:23.084782Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 9c527a19-15a8-486c-874e-e9f95ab2ebd0 · outbound

This paper cites Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.617190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fde54ba7-032f-450e-a06f-0f3cac78569a · outbound

This paper cites Shot noise in the astrophysical gravitational-wave background.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Shot noise in the astrophysical gravitational-wave background

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.621906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d66da7f-cd89-4a9b-8a1e-50457cf42f3f · outbound

This paper cites Unbiased estimation of gravitational-wave anisotropies from noisy data.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Unbiased estimation of gravitational-wave anisotropies from noisy data

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.627297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4d779d14-0ac6-48c6-9e7d-f27a3119128b · outbound

This paper cites PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.632835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92136b6d-0786-454b-8826-86a26efab7c5 · outbound

This paper cites Cosmic Star Formation History.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Cosmic Star Formation History

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.638179Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1812d2fd-1381-409f-9184-2f9bb0c7ea1f · outbound

This paper cites The population of merging compact binaries inferred using gravitational waves through GWTC-3.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The population of merging compact binaries inferred using gravitational waves through GWTC-3

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.643494Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 229a33d7-e8f2-4165-9f6f-baccd66fc130 · outbound

This paper cites The Mass Distribution of Neutron Stars in Gravitational-wave Binaries.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The Mass Distribution of Neutron Stars in Gravitational-wave Binaries

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.648396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ece1a62c-93e0-4888-841b-9a1e03aeb29b · outbound

This paper cites Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.653482Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c5dcfca-97f0-4ca5-87bf-7cdb8e561f2f · outbound

This paper cites Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.658306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc6ee6c9-8947-4857-806f-b93ad1ae2507 · outbound

This paper cites A Mock Data Challenge for the Einstein Gravitational-Wave Telescope.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background A Mock Data Challenge for the Einstein Gravitational-Wave Telescope

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.663155Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb490f68-0716-48c8-b6e3-3e3a96919c30 · outbound

This paper cites Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.668255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ceb3b21-8dde-478a-b871-8f959429cbff · outbound

This paper cites Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5~M_\odot$ Compact Object and a Neutron Star.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Observation of Gravitational Waves from the Coalescence of a $2.5\text{-}4.5~M_\odot$ Compact Object and a Neutron Star

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.673948Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3806a4cf-0bfa-47d2-bdfd-22780143ed22 · outbound

This paper cites Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.679586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation be3e0f4f-bec3-478f-92e5-0de1f0656b95 · outbound

This paper cites Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.684536Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c8249226-7c10-4072-973d-dc7ae7593d80 · outbound

This paper cites vegas: Adaptive multidimensional monte carlo integration,.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background vegas: Adaptive multidimensional monte carlo integration,

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T05:54:24.186393Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation aafa86c2-c162-4f67-aaa6-9990c680f4d9 · outbound

This paper cites an unresolved cited work.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Unresolved cited work

Reference 66

Resolution: unresolved; raw_fallback, observed 2026-08-12T05:54:24.169780Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 92cef7ef-0154-44f5-8cf7-ea7c5b48dfbd · outbound

This paper cites Adaptive Multidimensional Integration: VEGAS Enhanced.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Adaptive Multidimensional Integration: VEGAS Enhanced

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.699231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cdd76dfd-b05d-4009-a5a8-8c3cb64f036c · outbound

This paper cites Advanced LIGO.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Advanced LIGO

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.704179Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39bbac5f-5bdb-49f9-8994-f7443141245d · outbound

This paper cites The A+ design curve,.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background The A+ design curve,

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T05:54:24.154192Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation bb9ccd7a-5b2a-46d8-810d-c03c5c1890b4 · outbound

This paper cites Chandra,https://github.com/koustavchandra/ gwforge/tree/main/GWForge/ifo/noise_curves (2025).

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Chandra,https://github.com/koustavchandra/ gwforge/tree/main/GWForge/ifo/noise_curves (2025)

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T05:54:24.138216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 08b1b03e-f884-4d14-b4fa-84a9c149cc34 · outbound

This paper cites gwforge: A user-friendly package to generate gravitational-wave mock data.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background gwforge: A user-friendly package to generate gravitational-wave mock data

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.718463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03df566e-ca91-42c3-a838-91d0ec8bfae8 · outbound

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

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Sensitivity curves for searches for gravitational-wave backgrounds

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.723789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 127f67cc-73e3-417a-ba3d-a14b652d98df · outbound

This paper cites Expansions for nearly Gaussian distributions.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Expansions for nearly Gaussian distributions

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-08-12T05:54:22.775431Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

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Reference resolution

Outbound references

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