{"as_of":"2026-08-13T17:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:cc82aafa16af2229931cda325b9bb061634250d52a4970e4696d598ce1038013","coverage":[{"denominator":73,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":73,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T05:54:22.729190Z","state":"measured"},{"denominator":73,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":73,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.11119/citation-record","integrity":"/paper/2608.11119/integrity","json":"/paper/2608.11119/citation-record.json","paper":"/paper/2608.11119"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-08-12T05:54:22.358535Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.358535Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:6b4668ea92b58c8a7f266c9bf6b5914e59edc0f9227f00f6f8c444f1cd350cb7","observation_id":"8051ce0b-aadf-400d-b69c-ba9c7deb2522","resolution":{"observed_at":"2026-08-12T05:54:22.358535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-08-12T05:54:22.365117Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.365117Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:f327d2b4156b4a1bbd063808545c7e66de021a289d19579c6483606502228146","observation_id":"d97e4b1f-a5ed-4c8b-9931-6d17761c9add","resolution":{"observed_at":"2026-08-12T05:54:22.365117Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14527","last_updated":"2021-03-08T18:36:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:31Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14527","snapshot_observed_at":"2026-08-12T05:54:22.371144Z","title":"Abbottet al.(LIGO Scientific, Virgo), Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.371144Z"},"links":{"cited_paper":"/paper/2010.14527","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:2f308cc4af9901a7c90cfdc72609ed88eb40c791f5d57b15c04628dc98373d95","observation_id":"7d8e5597-3b91-4961-89c2-aaf27982aa14","resolution":{"observed_at":"2026-08-12T05:54:22.371144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03606","last_updated":"2023-10-23T13:37:50Z","snapshot_observed_at":"2026-08-08T16:18:10.684162Z","submitted_at":"2021-11-05T16:43:17Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03606","snapshot_observed_at":"2026-08-12T05:54:22.376361Z","title":"Abbottet al.(KAGRA, Virgo, LIGO Scientific), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.376361Z"},"links":{"cited_paper":"/paper/2111.03606","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:cdfefbdc27de5cd646a7bc026cdd2fe00e07bd6264af734eb5c9efcdc70b598e","observation_id":"e9f072ac-afd5-478a-bbea-84b05cc6da45","resolution":{"observed_at":"2026-08-12T05:54:22.376361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.18082","last_updated":"2026-06-26T11:38:00Z","snapshot_observed_at":"2026-08-05T16:32:29.718291Z","submitted_at":"2025-08-25T14:46:09Z","title":"GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.18082","snapshot_observed_at":"2026-08-12T05:54:22.381983Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.381983Z"},"links":{"cited_paper":"/paper/2508.18082","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:d8e399756313faf9347a5e96c779ea70b81cee37691893130102bc05a2b7d4a8","observation_id":"70192357-0e87-4b79-8fd5-1ffdb1425d7a","resolution":{"observed_at":"2026-08-12T05:54:22.381983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.27225","last_updated":"2026-06-23T16:50:16Z","snapshot_observed_at":"2026-07-06T23:36:58.541051Z","submitted_at":"2026-05-26T16:09:49Z","title":"GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.27225","snapshot_observed_at":"2026-08-12T05:54:22.387449Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.387449Z"},"links":{"cited_paper":"/paper/2605.27225","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:4214d137bc291aa13f6119a473725a3b5ec0af8b8838eb8dd60be460d13f09cb","observation_id":"7478e8df-7047-4b95-9569-4bf0fb03d40c","resolution":{"observed_at":"2026-08-12T05:54:22.387449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.08797","last_updated":"2018-11-21T15:50:01Z","snapshot_observed_at":"2026-08-10T10:13:25.388881Z","submitted_at":"2018-11-21T15:50:01Z","title":"Stochastic Gravitational Wave Backgrounds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.08797","snapshot_observed_at":"2026-08-12T05:54:22.393192Z","title":"Christensen, Rep","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.393192Z"},"links":{"cited_paper":"/paper/1811.08797","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:654c1690f006a8d6abf77fe3c5622ba0f529704c68d9d2a8bb5fed866c36657b","observation_id":"92eb5c87-bc38-44e9-a9f6-a1f7a6930e21","resolution":{"observed_at":"2026-08-12T05:54:22.393192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.00178","last_updated":"2022-02-28T22:08:11Z","snapshot_observed_at":"2026-08-13T16:49:26.074301Z","submitted_at":"2022-02-01T01:25:53Z","title":"Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.00178","snapshot_observed_at":"2026-08-12T05:54:22.398213Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.398213Z"},"links":{"cited_paper":"/paper/2202.00178","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:9c956079c3e0018f437ce87f88e724545bbbdb775d23d77c4d7a22d563e76b40","observation_id":"289c617d-927b-4bef-9e14-c0d4e8921724","resolution":{"observed_at":"2026-08-12T05:54:22.398213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.06889","last_updated":"2017-04-07T16:55:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2016-08-24T16:28:38Z","title":"Detection methods for stochastic gravitational-wave backgrounds: a unified treatment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.06889","snapshot_observed_at":"2026-08-12T05:54:22.403256Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.403256Z"},"links":{"cited_paper":"/paper/1608.06889","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c73022bcfb0731f1ed23782f193f622c99026f54374eb234e9505901d5ee410e","observation_id":"0e2a6001-c389-460f-9f62-ff61b4b42d4e","resolution":{"observed_at":"2026-08-12T05:54:22.403256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.20721","last_updated":"2025-08-28T12:44:13Z","snapshot_observed_at":"2026-08-07T10:34:29.047427Z","submitted_at":"2025-08-28T12:44:13Z","title":"Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.20721","snapshot_observed_at":"2026-08-12T05:54:22.408685Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.408685Z"},"links":{"cited_paper":"/paper/2508.20721","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:0695fea982f63ee2e087b0acdc89a1299340c36873c7f9aa656f338bcb1d2ae3","observation_id":"2e27cf88-0add-4e42-9703-c1035fbd19a1","resolution":{"observed_at":"2026-08-12T05:54:22.408685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:22.413784Z","title":"Abbottet al.(KAGRA, Virgo, LIGO Scientific), Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.413784Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:64d9ec25660306261b78ddfcdde299e235cadd5cda6df572591b2837e7520651","observation_id":"0dcc1955-da72-43f3-a108-83aac53ef88a","resolution":{"observed_at":"2026-08-12T05:54:22.413784Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9710117","last_updated":"1997-10-27T21:41:31Z","snapshot_observed_at":"2026-07-07T03:28:08.861130Z","submitted_at":"1997-10-27T21:41:31Z","title":"Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9710117","snapshot_observed_at":"2026-08-12T05:54:22.418941Z","title":"Allen and J","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.418941Z"},"links":{"cited_paper":"/paper/gr-qc/9710117","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c7bbb32079a8f14f6ca2c364ed06c0adf1f0a2eafb525a422498095d50623281","observation_id":"99bdbf41-d6f1-42c9-bfbc-9fdcfeccbe63","resolution":{"observed_at":"2026-08-12T05:54:22.418941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.3847","last_updated":"2012-09-18T05:24:42Z","snapshot_observed_at":"2026-07-06T02:55:48.906418Z","submitted_at":"2012-09-18T05:24:42Z","title":"Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.3847","snapshot_observed_at":"2026-08-12T05:54:22.423918Z","title":"Mandic, E","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.423918Z"},"links":{"cited_paper":"/paper/1209.3847","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:365608414e470d835b6cf444c3c8f0c7782a0d319f055248f32a75b5809b4da1","observation_id":"06820deb-4030-4122-9e44-4d1d7396e31c","resolution":{"observed_at":"2026-08-12T05:54:22.423918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.00907","last_updated":"2020-12-02T00:29:24Z","snapshot_observed_at":"2026-08-13T10:14:10.648868Z","submitted_at":"2020-12-02T00:29:24Z","title":"Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.00907","snapshot_observed_at":"2026-08-12T05:54:22.429043Z","title":"Matas and J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.429043Z"},"links":{"cited_paper":"/paper/2012.00907","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:d4a7c5b2bad78f39bda6d628ab57292905876be9175ccae3c7d80c6657fe9bb6","observation_id":"5b8b79c1-ef38-4ebb-93d6-ef49506ad20d","resolution":{"observed_at":"2026-08-12T05:54:22.429043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0210032","last_updated":"2003-02-05T20:55:23Z","snapshot_observed_at":"2026-08-09T00:16:03.579578Z","submitted_at":"2002-10-10T17:44:44Z","title":"Detection methods for non-Gaussian gravitational wave stochastic backgrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0210032","snapshot_observed_at":"2026-08-12T05:54:22.433719Z","title":"Drasco and E","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.433719Z"},"links":{"cited_paper":"/paper/gr-qc/0210032","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:79a54385467c544d234ebbea5e0e1b1f3863130daf4faa3317f6125bae55e14c","observation_id":"9b727d83-c625-4632-9756-f909284fc7ca","resolution":{"observed_at":"2026-08-12T05:54:22.433719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.00688","last_updated":"2018-04-09T05:13:12Z","snapshot_observed_at":"2026-07-06T06:12:26.699496Z","submitted_at":"2017-12-03T00:55:35Z","title":"The optimal search for an astrophysical gravitational-wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.00688","snapshot_observed_at":"2026-08-12T05:54:22.439244Z","title":"Smith and E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.439244Z"},"links":{"cited_paper":"/paper/1712.00688","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:8139e9af21273e1ce190fa1a2a7fcbdff31972fd0966f8011dd3c8053eb8d693","observation_id":"2f4b54cb-dbd4-4e66-add2-01a2a9200d12","resolution":{"observed_at":"2026-08-12T05:54:22.439244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.04418","last_updated":"2020-12-09T19:52:12Z","snapshot_observed_at":"2026-08-03T08:42:38.391801Z","submitted_at":"2020-09-09T17:06:04Z","title":"Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.04418","snapshot_observed_at":"2026-08-12T05:54:22.444536Z","title":"Biscoveanu, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.444536Z"},"links":{"cited_paper":"/paper/2009.04418","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:d96f836fcc61793c48b7b76c4380b19029e574efbd6fe1fd937e0d7b7d1abe90","observation_id":"f6e30f5d-12b8-489c-aec5-65fd40a8a06a","resolution":{"observed_at":"2026-08-12T05:54:22.444536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07675","last_updated":"2023-01-18T17:52:33Z","snapshot_observed_at":"2026-08-13T13:02:22.537517Z","submitted_at":"2023-01-18T17:52:33Z","title":"A stochastic search for intermittent gravitational-wave backgrounds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07675","snapshot_observed_at":"2026-08-12T05:54:22.449246Z","title":"Lawrence, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.449246Z"},"links":{"cited_paper":"/paper/2301.07675","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:3b9da97b35185d912775e28352eefb410c04895c3be62023cd5abd495e11bd3c","observation_id":"49893544-373f-49ec-9dd6-71e7c877b9f5","resolution":{"observed_at":"2026-08-12T05:54:22.449246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.14179","last_updated":"2025-06-17T04:40:37Z","snapshot_observed_at":"2026-08-13T15:05:38.847568Z","submitted_at":"2025-06-17T04:40:37Z","title":"Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.14179","snapshot_observed_at":"2026-08-12T05:54:22.454620Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.454620Z"},"links":{"cited_paper":"/paper/2506.14179","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:ec343e05bd2e6f82f9aea2c6aaf62a1d23bb85ade0d082dfb9a63d0a6056a128","observation_id":"dcee96ee-a61e-48ea-b365-a89a57791015","resolution":{"observed_at":"2026-08-12T05:54:22.454620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.07657","last_updated":"2020-04-21T16:50:27Z","snapshot_observed_at":"2026-07-06T08:44:55.434934Z","submitted_at":"2019-12-16T19:42:20Z","title":"Time-dependence of the astrophysical stochastic gravitational wave background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.07657","snapshot_observed_at":"2026-08-12T05:54:22.459467Z","title":"Mukherjee and J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.459467Z"},"links":{"cited_paper":"/paper/1912.07657","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:3b9ff955cbd799370dada5213176974945328de2a658000163f36c52660a8bb8","observation_id":"c4573d1f-92f1-48ba-9a2f-6b813de9b753","resolution":{"observed_at":"2026-08-12T05:54:22.459467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.06405","last_updated":"2023-10-31T13:56:33Z","snapshot_observed_at":"2026-08-13T10:57:15.236755Z","submitted_at":"2023-07-12T18:41:52Z","title":"Non-Stationary Astrophysical Stochastic Gravitational-Wave Background: A New Probe to the High Redshift Population of Binary Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.06405","snapshot_observed_at":"2026-08-12T05:54:22.465467Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.465467Z"},"links":{"cited_paper":"/paper/2307.06405","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:ae6213f2b4d21eeec284d97a1e3234716bb0de4d2804e722afd2d9e445c18367","observation_id":"89c0a7cf-f871-49b4-a076-872417662cca","resolution":{"observed_at":"2026-08-12T05:54:22.465467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2511.03262","last_updated":"2026-05-15T09:54:01Z","snapshot_observed_at":"2026-07-06T22:34:58.108904Z","submitted_at":"2025-11-05T07:46:38Z","title":"The First Upper Bound on the Non-Stationary Gravitational Wave Background and its Implication on the High Redshift Binary Black Hole Merger Rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.03262","snapshot_observed_at":"2026-08-12T05:54:22.470618Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.470618Z"},"links":{"cited_paper":"/paper/2511.03262","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:79827b74767da0be65a88679cbe966a014b774309460d480f889c3de6950affb","observation_id":"b48ad393-2525-4c52-8729-9138483e86cf","resolution":{"observed_at":"2026-08-12T05:54:22.470618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.5775","last_updated":"2014-05-22T14:48:26Z","snapshot_observed_at":"2026-08-10T15:32:05.792467Z","submitted_at":"2014-05-22T14:48:26Z","title":"A Semi-Parametric Approach to the Detection of Non-Gaussian Gravitational Wave Stochastic Backgrounds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.5775","snapshot_observed_at":"2026-08-12T05:54:22.476135Z","title":"Martellini and T","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.476135Z"},"links":{"cited_paper":"/paper/1405.5775","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:4dc7e2e3721b44dd21f4fa029893236df558117b3fe4da5ef39decf61629dc23","observation_id":"21f089d2-4eaf-4f74-91ac-58ecc54a4a7e","resolution":{"observed_at":"2026-08-12T05:54:22.476135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.04802","last_updated":"2015-09-16T03:21:31Z","snapshot_observed_at":"2026-07-06T04:30:02.732607Z","submitted_at":"2015-09-16T03:21:31Z","title":"On the (In)Efficiency of the Cross-Correlation Statistic for Gravitational Wave Stochastic Background Signals with Non-Gaussian Noise and Heterogeneous Detector Sensitivities","version":1},"cited_work":{"arxiv_id":"1509.04802","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.04802","snapshot_observed_at":"2026-08-12T05:54:23.693666Z","title":"On the (In)Efficiency of the Cross-Correlation Statistic for Gravitational Wave Stochastic Background Signals with Non-Gaussian Noise and Heterogeneous Detector Sensitivities","venue":"astro-ph.CO","work_id":"5904c847-b4d1-49a8-96ed-00cc0e80d8da","year":2015},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.481066Z"},"links":{"cited_paper":"/paper/1509.04802","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:572959052bc0c2ae39fdaa0d26d60e74b37d909c18ef4e451b26b4c69a57960b","observation_id":"8d53a671-9761-45e6-8501-a9f92be4d9a1","resolution":{"observed_at":"2026-08-12T05:54:23.699705Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2601.10428","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:23.668429Z","title":"Liu and S","venue":null,"work_id":"98349b80-83c9-4c3b-8f62-f0541bd09648","year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.486455Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:dc44ee3700a54601911e084ab97661e32cbf6c5a8c78af8a23ba36675425e3c5","observation_id":"328cdb66-3394-4b60-a54b-a1ea2b77c900","resolution":{"observed_at":"2026-08-12T05:54:23.676370Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:22.491063Z","title":"Punturoet al., Class","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.491063Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:20eadffd436631852a20855b2eb097cd559251a39d5b35c5850a82998609e669","observation_id":"8f3aa34e-a067-439f-a7bb-65bb648244b0","resolution":{"observed_at":"2026-08-12T05:54:22.491063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15923","last_updated":"2023-06-17T10:49:26Z","snapshot_observed_at":"2026-08-08T01:52:18.464766Z","submitted_at":"2023-03-28T12:29:33Z","title":"Science with the Einstein Telescope: a comparison of different designs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15923","snapshot_observed_at":"2026-08-12T05:54:22.495943Z","title":"Branchesiet al., J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.495943Z"},"links":{"cited_paper":"/paper/2303.15923","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:7d2ffaef628daaa352258173486674ec779b1cf37ecf3c554bdb33183c32a324","observation_id":"10c5dd67-12ab-474b-93ed-8254fa37abc1","resolution":{"observed_at":"2026-08-12T05:54:22.495943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.12263","last_updated":"2025-08-29T11:52:35Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-15T21:04:14Z","title":"The Science of the Einstein Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.12263","snapshot_observed_at":"2026-08-12T05:54:22.500855Z","title":"Abacet al.(ET), J","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.500855Z"},"links":{"cited_paper":"/paper/2503.12263","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:8c954a43b0378b3efc3f39e17a6c9eb8a1aac86d2e59df2c6da4a30fbf3d6365","observation_id":"579c4210-a092-42e6-b531-85c4bf8c9b13","resolution":{"observed_at":"2026-08-12T05:54:22.500855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04833","last_updated":"2019-07-10T17:27:49Z","snapshot_observed_at":"2026-08-13T08:09:53.331668Z","submitted_at":"2019-07-10T17:27:49Z","title":"Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04833","snapshot_observed_at":"2026-08-12T05:54:22.505992Z","title":"Reitzeet al., Bull","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.505992Z"},"links":{"cited_paper":"/paper/1907.04833","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:b3544192ab1ab4aee43788a188b72fb37a0db89e805686c43a419b95b13f6c9c","observation_id":"d80a4947-2967-4d49-aa5b-9503bdaf1460","resolution":{"observed_at":"2026-08-12T05:54:22.505992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09882","last_updated":"2021-10-06T14:54:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-09-20T23:34:33Z","title":"A Horizon Study for Cosmic Explorer: Science, Observatories, and Community","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09882","snapshot_observed_at":"2026-08-12T05:54:22.511099Z","title":"Evanset al., (2021), arXiv:2109.09882 [astro-ph.IM]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.511099Z"},"links":{"cited_paper":"/paper/2109.09882","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:6fac9eb5c190b529024a4afe82829c69cd40ef7a75d52c66e5d7375303aabbb5","observation_id":"3003b66f-e826-4e6d-b167-8a3da8383c67","resolution":{"observed_at":"2026-08-12T05:54:22.511099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.13745","last_updated":"2023-06-23T19:05:12Z","snapshot_observed_at":"2026-08-13T11:10:24.054092Z","submitted_at":"2023-06-23T19:05:12Z","title":"Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.13745","snapshot_observed_at":"2026-08-12T05:54:22.516247Z","title":"Evanset al., (2023), arXiv:2306.13745 [astro-ph.IM]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.516247Z"},"links":{"cited_paper":"/paper/2306.13745","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:fcfe5d2f60b4b156444d1db2d2c234676644e51ab5916d9a9abf73c4152c9ed1","observation_id":"b9a21474-ec13-46a7-a97f-cb1d44b0f187","resolution":{"observed_at":"2026-08-12T05:54:22.516247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11877","last_updated":"2022-09-23T22:02:27Z","snapshot_observed_at":"2026-08-13T14:20:07.161132Z","submitted_at":"2022-09-23T22:02:27Z","title":"Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors","version":1},"cited_work":{"arxiv_id":"2209.11877","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.11877","snapshot_observed_at":"2026-08-12T05:54:23.511123Z","title":"Detecting cosmological gravitational waves background after removal of compact binary coalescences in future gravitational wave detectors","venue":"gr-qc","work_id":"191cc4c1-d67f-4dc0-a0db-5f043a3d6d71","year":2022},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.521751Z"},"links":{"cited_paper":"/paper/2209.11877","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:4b0d3868e67b3f891991aea2e7f46cf949999c2db896af48523799d9182a6cba","observation_id":"0a3a01b3-523b-4b8b-a759-8992be61e38c","resolution":{"observed_at":"2026-08-12T05:54:23.516268Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10757","last_updated":"2024-09-30T14:41:53Z","snapshot_observed_at":"2026-08-13T13:52:44.352375Z","submitted_at":"2024-06-15T23:07:39Z","title":"Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10757","snapshot_observed_at":"2026-08-12T05:54:22.527086Z","title":"Zhong, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.527086Z"},"links":{"cited_paper":"/paper/2406.10757","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:e8ef33c5ed7bdabd742d6f9204ebd7d533cfe31271dce61ac3e5b4eadf87bf47","observation_id":"bba5db92-0b06-4bb4-bc29-1863357e7bdc","resolution":{"observed_at":"2026-08-12T05:54:22.527086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:22.532103Z","title":"Zhong and V","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.532103Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:f62c6618ea07cde6c2f897d9d4319eafe2bbf1813ad994e5ef908f89041afee3","observation_id":"a31a8e41-7fb7-4986-bfb5-dd579a03bc00","resolution":{"observed_at":"2026-08-12T05:54:22.532103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04268","last_updated":"2020-07-22T11:15:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-01-12T18:57:34Z","title":"Cosmological Backgrounds of Gravitational Waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04268","snapshot_observed_at":"2026-08-12T05:54:22.536653Z","title":"Caprini and D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.536653Z"},"links":{"cited_paper":"/paper/1801.04268","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:678f0ddcaef9dd555f5b0ff734836570ef291912524b687c41accc4aa8dc8b83","observation_id":"1be27502-5ef6-45ba-8df1-1803c0edf0e6","resolution":{"observed_at":"2026-08-12T05:54:22.536653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-12T05:54:22.541916Z","title":"Aghanimet al.(Planck), Astron","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.541916Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:ec79888317f39892b343759fbe27ac3853bd57c0875b22a325dc5766afdccdce","observation_id":"9134e29b-808b-4f3d-9483-580dc9e5d6c1","resolution":{"observed_at":"2026-08-12T05:54:22.541916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.09745","last_updated":"2025-02-28T21:17:56Z","snapshot_observed_at":"2026-08-11T17:36:59.140180Z","submitted_at":"2019-11-21T20:58:08Z","title":"Understanding $\\Omega_\\mathrm{gw}(f)$ in Gravitational Wave Experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.09745","snapshot_observed_at":"2026-08-12T05:54:22.546759Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.546759Z"},"links":{"cited_paper":"/paper/1911.09745","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:d909522a7cacb91b55db9ea1468f83bce5ff2cbd3e329689d73ccde506614a31","observation_id":"16143bc7-0543-4a30-bd5e-8effafee1c11","resolution":{"observed_at":"2026-08-12T05:54:22.546759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.23816","last_updated":"2026-06-22T18:01:21Z","snapshot_observed_at":"2026-08-05T20:00:24.130733Z","submitted_at":"2026-06-22T18:01:21Z","title":"A thorough investigation of cross-correlation estimators for stochastic gravitational-wave background searches in ground-based detector data","version":1},"cited_work":{"arxiv_id":"2606.23816","doi":null,"metadata_source":"pith","pith_arxiv_id":"2606.23816","snapshot_observed_at":"2026-08-12T05:54:23.352400Z","title":"A thorough investigation of cross-correlation estimators for stochastic gravitational-wave background searches in ground-based detector data","venue":"gr-qc","work_id":"fdf3c3aa-89bb-4516-a0d9-62b06f85c081","year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.552108Z"},"links":{"cited_paper":"/paper/2606.23816","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:18e74e8d371a026833b716178e34e49e6840b7108f29c47eb14afffa65ba9001","observation_id":"d680623b-ea41-49cc-911a-79d8571c3227","resolution":{"observed_at":"2026-08-12T05:54:23.357827Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15696","last_updated":"2023-03-28T02:49:28Z","snapshot_observed_at":"2026-08-13T12:15:11.635206Z","submitted_at":"2023-03-28T02:49:28Z","title":"pygwb: Python-based library for gravitational-wave background searches","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15696","snapshot_observed_at":"2026-08-12T05:54:22.556999Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.556999Z"},"links":{"cited_paper":"/paper/2303.15696","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:b4efbd68f65f17015db824157aa0f28c301d4892ef1ed8b38a396bd2cbcc2b54","observation_id":"60a0fddf-2bf4-4fc5-94fb-521d126df6bf","resolution":{"observed_at":"2026-08-12T05:54:22.556999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.27226","last_updated":"2026-07-01T12:07:47Z","snapshot_observed_at":"2026-08-12T13:35:25.757868Z","submitted_at":"2026-05-26T16:09:50Z","title":"GWTC-5.0: Population Properties of Merging Compact Binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.27226","snapshot_observed_at":"2026-08-12T05:54:22.562752Z","title":"GWTC-5.0: Popula- tion Properties of Merging Compact Binaries,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.562752Z"},"links":{"cited_paper":"/paper/2605.27226","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:042d983cee155cac26a604beab0bf620955dff1d42a951bb437eba1640edd686","observation_id":"5b9cca82-4b56-4ff0-97e3-9f65d83c8bdf","resolution":{"observed_at":"2026-08-12T05:54:22.562752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.25772","last_updated":"2026-05-25T12:22:14Z","snapshot_observed_at":"2026-08-08T03:08:46.796144Z","submitted_at":"2026-05-25T12:22:14Z","title":"Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks","version":1},"cited_work":{"arxiv_id":"2605.25772","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.25772","snapshot_observed_at":"2026-08-12T05:54:23.299388Z","title":"Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks","venue":"gr-qc","work_id":"870ae441-ec62-46a6-8608-4737ae2b87fb","year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.567343Z"},"links":{"cited_paper":"/paper/2605.25772","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c42ac2664e7395e4e8cbd69589ab5465b5de4319c8d798f8a0e41add736b799b","observation_id":"f3387c0c-e90c-4c0d-a26c-4b9bec50c2b5","resolution":{"observed_at":"2026-08-12T05:54:23.304604Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.04028","last_updated":"2025-03-16T11:46:39Z","snapshot_observed_at":"2026-08-12T22:06:22.243448Z","submitted_at":"2024-11-06T16:26:39Z","title":"The spectral density of astrophysical stochastic backgrounds","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.04028","snapshot_observed_at":"2026-08-12T05:54:22.572158Z","title":"Belgacem, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.572158Z"},"links":{"cited_paper":"/paper/2411.04028","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:4eb776d58a45ef4e9b7a86fab72c261e119c510e33ac35ab2d82337643068d4c","observation_id":"caf7ceba-35d6-489f-90c7-a20b6e9a0c93","resolution":{"observed_at":"2026-08-12T05:54:22.572158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.01310","last_updated":"2023-09-24T18:45:43Z","snapshot_observed_at":"2026-08-13T14:33:41.523314Z","submitted_at":"2022-09-03T01:49:42Z","title":"Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.01310","snapshot_observed_at":"2026-08-12T05:54:22.577509Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.577509Z"},"links":{"cited_paper":"/paper/2209.01310","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:1126a81daf2b1444bb6b6207cd922b5fc1b5ba5ae658ce6f5e3da478d732c5db","observation_id":"a1f4742f-641c-4963-90c4-ab84bbe08fbf","resolution":{"observed_at":"2026-08-12T05:54:22.577509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.01221","last_updated":"2022-09-02T18:00:01Z","snapshot_observed_at":"2026-08-13T14:33:47.078943Z","submitted_at":"2022-09-02T18:00:01Z","title":"Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.01221","snapshot_observed_at":"2026-08-12T05:54:22.582320Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.582320Z"},"links":{"cited_paper":"/paper/2209.01221","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:71d0d3aa8627ab3b1c71881c1b0339539d22bf654edd2369dcf3acb98e35cec0","observation_id":"6fb8688b-2fff-458b-9c5c-8f41b4eb3d2a","resolution":{"observed_at":"2026-08-12T05:54:22.582320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.00984","last_updated":"2024-05-14T03:44:25Z","snapshot_observed_at":"2026-08-13T10:47:02.383674Z","submitted_at":"2024-01-02T01:18:34Z","title":"The Impact of Spin in Compact Binary Foreground Subtraction for Estimating the Residual Stochastic Gravitational-wave Background in Ground-based Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.00984","snapshot_observed_at":"2026-08-12T05:54:22.587260Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.587260Z"},"links":{"cited_paper":"/paper/2401.00984","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:db6b3e232396efa692b8667b6fbd108ec8dbe2d95671b31d2d94bd9ec7abab0b","observation_id":"337265b5-9b5f-4cbb-8866-e55cb94a71b9","resolution":{"observed_at":"2026-08-12T05:54:22.587260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.03742","last_updated":"2024-07-04T08:54:00Z","snapshot_observed_at":"2026-08-12T23:29:00.814802Z","submitted_at":"2024-07-04T08:54:00Z","title":"Projections of the uncertainty on the compact binary population background using popstock","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.03742","snapshot_observed_at":"2026-08-12T05:54:22.592046Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.592046Z"},"links":{"cited_paper":"/paper/2407.03742","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:42f9e9d831cb71f06e457ad1f8d39fcaca8cd534f9071aa89dbfe7dd78f93f5a","observation_id":"352bf180-5935-480a-b6b2-e99b1f95b7a6","resolution":{"observed_at":"2026-08-12T05:54:22.592046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:22.597362Z","title":"Ebersold and T","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.597362Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:ce237d2614ec335430d417ac375e2c924ccc5c1669f423fd8e8d7682912ff253","observation_id":"77b4dd3c-60a7-4792-9c6a-7e9c22999b61","resolution":{"observed_at":"2026-08-12T05:54:22.597362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.06270","last_updated":"2024-08-05T16:22:31Z","snapshot_observed_at":"2026-08-12T23:26:29.021546Z","submitted_at":"2024-07-08T18:00:04Z","title":"Spectral Variance in a Stochastic Gravitational-Wave Background From a Binary Population","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.06270","snapshot_observed_at":"2026-08-12T05:54:22.601947Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.601947Z"},"links":{"cited_paper":"/paper/2407.06270","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:5432a6a3c0fe309ac23158a31fe1adbd9a05d9b4fb287f163a30ea8104031364","observation_id":"7dd9aea5-66a9-4924-a50b-fe5a8f3402ec","resolution":{"observed_at":"2026-08-12T05:54:22.601947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2511.09659","last_updated":"2026-06-26T16:07:05Z","snapshot_observed_at":"2026-08-03T22:40:15.951793Z","submitted_at":"2025-11-12T19:05:59Z","title":"Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.09659","snapshot_observed_at":"2026-08-12T05:54:22.606897Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.606897Z"},"links":{"cited_paper":"/paper/2511.09659","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:f34e4774b118b5ce411ccccc500ff5f9ada87032f29ae5fba424b4d97ab5c106","observation_id":"46fd026e-ec93-4fce-acf0-ae890c557d62","resolution":{"observed_at":"2026-08-12T05:54:22.606897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6231","last_updated":"2014-03-17T10:03:10Z","snapshot_observed_at":"2026-07-06T03:36:55.289462Z","submitted_at":"2014-02-25T16:35:55Z","title":"Statistical properties of astrophysical gravitational-wave backgrounds","version":2},"cited_work":{"arxiv_id":"1402.6231","doi":null,"metadata_source":"pith","pith_arxiv_id":"1402.6231","snapshot_observed_at":"2026-08-12T05:54:23.079797Z","title":"Statistical properties of astrophysical gravitational-wave backgrounds","venue":"astro-ph.CO","work_id":"54786695-7386-4f7b-aaeb-38fca6b06e7d","year":2014},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.612046Z"},"links":{"cited_paper":"/paper/1402.6231","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:817647c2742f910dac8147cb56342c154c918bbc2fbb79a513b2b22879549e15","observation_id":"97df58e1-c26e-4892-89f3-88e473704d66","resolution":{"observed_at":"2026-08-12T05:54:23.084782Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.06642","last_updated":"2020-01-27T19:32:24Z","snapshot_observed_at":"2026-08-05T14:12:49.454091Z","submitted_at":"2019-07-15T18:00:00Z","title":"Estimating the angular power spectrum of the gravitational-wave background in the presence of shot noise","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.06642","snapshot_observed_at":"2026-08-12T05:54:22.617190Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.617190Z"},"links":{"cited_paper":"/paper/1907.06642","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:084f469991603d0b74be3e7f0452b17198a55c5d98b9929336ea2e5bc4997947","observation_id":"9c527a19-15a8-486c-874e-e9f95ab2ebd0","resolution":{"observed_at":"2026-08-12T05:54:22.617190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.07719","last_updated":"2020-01-27T19:28:11Z","snapshot_observed_at":"2026-08-13T15:19:50.151571Z","submitted_at":"2019-02-20T19:00:01Z","title":"Shot noise in the astrophysical gravitational-wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.07719","snapshot_observed_at":"2026-08-12T05:54:22.621906Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.621906Z"},"links":{"cited_paper":"/paper/1902.07719","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:dc922b95cda6f047d4e47b953f9f4fc488a327c24d68063533ab0cc5a71f6c20","observation_id":"fde54ba7-032f-450e-a06f-0f3cac78569a","resolution":{"observed_at":"2026-08-12T05:54:22.621906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.09110","last_updated":"2024-09-24T14:03:27Z","snapshot_observed_at":"2026-08-13T05:02:19.280895Z","submitted_at":"2023-12-14T16:46:12Z","title":"Unbiased estimation of gravitational-wave anisotropies from noisy data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.09110","snapshot_observed_at":"2026-08-12T05:54:22.627297Z","title":"Kouvatsos, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.627297Z"},"links":{"cited_paper":"/paper/2312.09110","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:16f90b873f4471bc9f84b9f43659aac6e09a36872b496fc88b6642931a9da865","observation_id":"1d66da7f-cd89-4a9b-8a1e-50457cf42f3f","resolution":{"observed_at":"2026-08-12T05:54:22.627297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.16813","last_updated":"2025-07-02T00:58:59Z","snapshot_observed_at":"2026-08-12T23:35:55.331681Z","submitted_at":"2024-06-24T17:24:11Z","title":"PixelPop: High Resolution Nonparameteric Inference of Gravitational-Wave Populations in Multiple Dimensions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.16813","snapshot_observed_at":"2026-08-12T05:54:22.632835Z","title":"Heinzel, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.632835Z"},"links":{"cited_paper":"/paper/2406.16813","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:90487ed3ae3609029a5b466da2e8c46eeafcb8d589c00aa0750b3439434cb12c","observation_id":"4d779d14-0ac6-48c6-9e7d-f27a3119128b","resolution":{"observed_at":"2026-08-12T05:54:22.632835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.0007","last_updated":"2014-06-13T01:11:59Z","snapshot_observed_at":"2026-08-04T05:19:08.451508Z","submitted_at":"2014-02-28T21:00:32Z","title":"Cosmic Star Formation History","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.0007","snapshot_observed_at":"2026-08-12T05:54:22.638179Z","title":"Madau and M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.638179Z"},"links":{"cited_paper":"/paper/1403.0007","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:e04dc028358d8f91c0d2b4b94df8f82a369d3a22ba5d68502e2a544e5cf3cd19","observation_id":"92136b6d-0786-454b-8826-86a26efab7c5","resolution":{"observed_at":"2026-08-12T05:54:22.638179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03634","last_updated":"2025-01-30T17:06:46Z","snapshot_observed_at":"2026-08-04T10:06:39.982302Z","submitted_at":"2021-11-05T17:35:45Z","title":"The population of merging compact binaries inferred using gravitational waves through GWTC-3","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03634","snapshot_observed_at":"2026-08-12T05:54:22.643494Z","title":"Abbottet al.(KAGRA, Virgo, LIGO Scientific), Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.643494Z"},"links":{"cited_paper":"/paper/2111.03634","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c3693affa04f9c1e756159cc790cb7c07f2c6b4f8df71eb1f4f06cec59823c0e","observation_id":"1812d2fd-1381-409f-9184-2f9bb0c7ea1f","resolution":{"observed_at":"2026-08-12T05:54:22.643494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.04559","last_updated":"2021-11-04T16:12:13Z","snapshot_observed_at":"2026-08-11T21:51:19.406689Z","submitted_at":"2021-07-09T17:23:07Z","title":"The Mass Distribution of Neutron Stars in Gravitational-wave Binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.04559","snapshot_observed_at":"2026-08-12T05:54:22.648396Z","title":"Landry and J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.648396Z"},"links":{"cited_paper":"/paper/2107.04559","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:dfc9d530327429af246efb39e8e175efbdec401852bbf6c1912317623e3c1fee","observation_id":"229a33d7-e8f2-4165-9f6f-baccd66fc130","resolution":{"observed_at":"2026-08-12T05:54:22.648396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.17717","last_updated":"2025-09-08T18:48:42Z","snapshot_observed_at":"2026-08-11T17:47:46.594066Z","submitted_at":"2025-01-29T15:36:48Z","title":"Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.17717","snapshot_observed_at":"2026-08-12T05:54:22.653482Z","title":"Zhong, L","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.653482Z"},"links":{"cited_paper":"/paper/2501.17717","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:f264baade3349cf2c2a917ca008e059a681721243330ee6f9a57f88e6890467b","observation_id":"ece1a62c-93e0-4888-841b-9a1e03aeb29b","resolution":{"observed_at":"2026-08-12T05:54:22.653482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07887","last_updated":"2017-04-18T00:45:06Z","snapshot_observed_at":"2026-08-12T20:45:30.262331Z","submitted_at":"2016-06-25T08:58:38Z","title":"Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07887","snapshot_observed_at":"2026-08-12T05:54:22.658306Z","title":"Madau and T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.658306Z"},"links":{"cited_paper":"/paper/1606.07887","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:e8ccd57547de77db99724d0df965d0187671f48d6bae3529ab87028841c32f0c","observation_id":"5c5dcfca-97f0-4ca5-87bf-7cdb8e561f2f","resolution":{"observed_at":"2026-08-12T05:54:22.658306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3563","last_updated":"2012-08-07T09:52:02Z","snapshot_observed_at":"2026-07-06T02:41:16.997007Z","submitted_at":"2012-01-17T17:20:40Z","title":"A Mock Data Challenge for the Einstein Gravitational-Wave Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3563","snapshot_observed_at":"2026-08-12T05:54:22.663155Z","title":"Regimbauet al., Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.663155Z"},"links":{"cited_paper":"/paper/1201.3563","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:ec1d54deb7e8fc6c7fee50bb080c9af032a965d2d5f808f320f9160a54697d43","observation_id":"dc6ee6c9-8947-4857-806f-b93ad1ae2507","resolution":{"observed_at":"2026-08-12T05:54:22.663155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.01568","last_updated":"2023-06-20T20:51:11Z","snapshot_observed_at":"2026-08-13T15:10:49.868531Z","submitted_at":"2022-07-04T16:41:18Z","title":"Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.01568","snapshot_observed_at":"2026-08-12T05:54:22.668255Z","title":"Biscoveanu, P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.668255Z"},"links":{"cited_paper":"/paper/2207.01568","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:3a263a80dfd6c363c67ba1256e7a7d42f18e953f8753bbe00564f6c509c5c4ab","observation_id":"fb490f68-0716-48c8-b6e3-3e3a96919c30","resolution":{"observed_at":"2026-08-12T05:54:22.668255Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.04248","last_updated":"2024-07-26T22:16:00Z","snapshot_observed_at":"2026-08-13T00:36:54.454694Z","submitted_at":"2024-04-05T17:54:11Z","title":"Observation of Gravitational Waves from the Coalescence of a $2.5\\text{-}4.5~M_\\odot$ Compact Object and a Neutron Star","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.04248","snapshot_observed_at":"2026-08-12T05:54:22.673948Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.673948Z"},"links":{"cited_paper":"/paper/2404.04248","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:dbd488462d7324bcd81123d8ff7ce9a251929fccf8a6ebd13b8948faa450a9fa","observation_id":"1ceb3b21-8dde-478a-b871-8f959429cbff","resolution":{"observed_at":"2026-08-12T05:54:22.673948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.11412","last_updated":"2020-01-30T15:46:20Z","snapshot_observed_at":"2026-08-10T13:27:34.841880Z","submitted_at":"2020-01-30T15:46:20Z","title":"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","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.11412","snapshot_observed_at":"2026-08-12T05:54:22.679586Z","title":"Pratten, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.679586Z"},"links":{"cited_paper":"/paper/2001.11412","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c19a80f3a71a164d1d5e288bb2b6916cd019f3a4bbc7fe515d2f533980048b43","observation_id":"3806a4cf-0bfa-47d2-bdfd-22780143ed22","resolution":{"observed_at":"2026-08-12T05:54:22.679586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.0700","last_updated":"2009-07-03T19:31:53Z","snapshot_observed_at":"2026-08-12T19:16:18.975117Z","submitted_at":"2009-07-03T19:31:53Z","title":"Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.0700","snapshot_observed_at":"2026-08-12T05:54:22.684536Z","title":"Buonanno, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.684536Z"},"links":{"cited_paper":"/paper/0907.0700","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:3d69ba5f7a2d06a118800533621f8d58cc64c5986aa2a51b4f35a62f583f3816","observation_id":"be3e0f4f-bec3-478f-92e5-0de1f0656b95","resolution":{"observed_at":"2026-08-12T05:54:22.684536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:24.181210Z","title":"vegas: Adaptive multidimensional monte carlo integration,","venue":null,"work_id":"b8808fc2-3780-4340-baf6-18b7b27f5d04","year":2024},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.689892Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:07666dc6240fb29804a1a45083a82491e15641f4ceaa853b592d312d11741415","observation_id":"c8249226-7c10-4072-973d-dc7ae7593d80","resolution":{"observed_at":"2026-08-12T05:54:24.186393Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:24.164804Z","title":null,"venue":null,"work_id":"8f35d6b3-cfd2-41b0-b547-5735c6bed924","year":1978},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.694429Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:087ccce65b77a2459abcc713a3c440c5c478ff2e855ff15641c6d1fabdd5bcdf","observation_id":"aafa86c2-c162-4f67-aaa6-9990c680f4d9","resolution":{"observed_at":"2026-08-12T05:54:24.169780Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.05112","last_updated":"2021-04-20T19:19:34Z","snapshot_observed_at":"2026-08-11T01:54:32.328357Z","submitted_at":"2020-09-10T19:29:52Z","title":"Adaptive Multidimensional Integration: VEGAS Enhanced","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.05112","snapshot_observed_at":"2026-08-12T05:54:22.699231Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.699231Z"},"links":{"cited_paper":"/paper/2009.05112","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:a52d2e28212245903e49b75c035cf0b4682af43cd083946ccc319b2ab228c547","observation_id":"92cef7ef-0154-44f5-8cf7-ea7c5b48dfbd","resolution":{"observed_at":"2026-08-12T05:54:22.699231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4547","last_updated":"2014-11-17T16:55:23Z","snapshot_observed_at":"2026-08-12T13:34:30.122295Z","submitted_at":"2014-11-17T16:55:23Z","title":"Advanced LIGO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.4547","snapshot_observed_at":"2026-08-12T05:54:22.704179Z","title":"Aasiet al.(LIGO Scientific), Class","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.704179Z"},"links":{"cited_paper":"/paper/1411.4547","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:56d1099b1f087ae539e112d445a325ff5fd972b727389636d103fe88f4fa224c","observation_id":"cdd76dfd-b05d-4009-a5a8-8c3cb64f036c","resolution":{"observed_at":"2026-08-12T05:54:22.704179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:24.149197Z","title":"The A+ design curve,","venue":null,"work_id":"2aff2d4c-eaed-4514-8c28-e64fd76a500b","year":2018},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.709306Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:215d7f3a5dff4de5a852d67dc8fb8cdd75be735e89995a588b12b58e93181377","observation_id":"39bbac5f-5bdb-49f9-8994-f7443141245d","resolution":{"observed_at":"2026-08-12T05:54:24.154192Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T05:54:24.133186Z","title":"Chandra,https://github.com/koustavchandra/ gwforge/tree/main/GWForge/ifo/noise_curves (2025)","venue":null,"work_id":"5942767e-2344-4da7-babe-ede5da5406a1","year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.713776Z"},"links":{"citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:c8cb7e62c61a3e40cedfefc582a17a980343c3e6f7e4a0bcc3731e12244919b4","observation_id":"bb9ccd7a-5b2a-46d8-810d-c03c5c1890b4","resolution":{"observed_at":"2026-08-12T05:54:24.138216Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.21109","last_updated":"2024-07-30T18:01:57Z","snapshot_observed_at":"2026-08-12T23:11:46.966704Z","submitted_at":"2024-07-30T18:01:57Z","title":"gwforge: A user-friendly package to generate gravitational-wave mock data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.21109","snapshot_observed_at":"2026-08-12T05:54:22.718463Z","title":"Chandra, Class","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.718463Z"},"links":{"cited_paper":"/paper/2407.21109","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:32707a4279a5e3585159c3a56640a3d4d1a8077b9421b54731f10185e6694dc2","observation_id":"08b1b03e-f884-4d14-b4fa-84a9c149cc34","resolution":{"observed_at":"2026-08-12T05:54:22.718463Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.5300","last_updated":"2013-11-25T17:13:47Z","snapshot_observed_at":"2026-07-06T03:26:03.309810Z","submitted_at":"2013-10-20T04:08:41Z","title":"Sensitivity curves for searches for gravitational-wave backgrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.5300","snapshot_observed_at":"2026-08-12T05:54:22.723789Z","title":"Thrane and J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.723789Z"},"links":{"cited_paper":"/paper/1310.5300","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:b10bbb91ece1b007d062c213ffcb32b2c9923c15c33b0cde470aeffc510bcbcb","observation_id":"03df566e-ca91-42c3-a838-91d0ec8bfae8","resolution":{"observed_at":"2026-08-12T05:54:22.723789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9711239","last_updated":"1997-11-20T15:51:53Z","snapshot_observed_at":"2026-07-07T01:19:01.650748Z","submitted_at":"1997-11-20T15:51:53Z","title":"Expansions for nearly Gaussian distributions","version":1},"cited_work":{"arxiv_id":"astro-ph/9711239","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9711239","snapshot_observed_at":"2026-08-12T05:54:22.768037Z","title":"Expansions for nearly Gaussian distributions","venue":"astro-ph","work_id":"3b7b79b9-449d-4816-97c5-a5a7c7367ddf","year":1997},"citing_paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T05:54:22.729190Z"},"links":{"cited_paper":"/paper/astro-ph/9711239","citing_paper":"/paper/2608.11119"},"observation_digest":"sha256:60c16783e8898f68f55231102bac305adb36fd2242fa249e5dd49f8f5fee0f83","observation_id":"127f67cc-73e3-417a-ba3d-a14b652d98df","resolution":{"observed_at":"2026-08-12T05:54:22.775431Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2608.11119","last_updated":"2026-08-11T16:26:47Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-13T17:31:02.279108Z","submitted_at":"2026-08-11T16:26:47Z","title":"All You Need is not $\\Omega_\\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background"},"reference_resolution":{"displayed":73,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":63,"verified_exact":7,"verified_fuzzy":3},"total_outbound_references":73},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 73 of 73 outbound references and 0 inbound Pith citation observations for arXiv:2608.11119."}