{"as_of":"2026-08-16T07:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f848413b6207aeb4496bd78374468a8e2dafb6e33baef9e09ab51989decca54a","coverage":[{"denominator":113,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T20:02:43.877803Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T09:17:06.785856Z","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":[{"citation":{"cited_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.14366","snapshot_observed_at":"2026-08-03T09:17:06.785856Z","title":"Fu and J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.14412","last_updated":"2026-07-03T09:56:53Z","snapshot_observed_at":"2026-08-12T16:35:18.840084Z","submitted_at":"2026-01-20T19:16:41Z","title":"How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T09:17:06.785856Z"},"links":{"cited_paper":"/paper/2506.14366","citing_paper":"/paper/2601.14412"},"observation_digest":"sha256:b83670e09e715698e449e935355c9086f0907a920f9dafaba63b9cfc44cadb9e","observation_id":"efbb6a49-ae64-4344-9b4e-83ab8921e786","resolution":{"observed_at":"2026-08-03T09:17:06.785856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2506.14366/citation-record","integrity":"/paper/2506.14366/integrity","json":"/paper/2506.14366/citation-record.json","paper":"/paper/2506.14366"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T20:02:42.592620Z","title":"We use vw to denote the velocity of the bubble walls, and set vw = 1 to obtain a conservative estimation of ΩGW","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.592620Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:a1652cda53a6291c929bed256ab15e5ea9afdf7a54babc8b8cd3bba5a8a5fb33","observation_id":"9ed2cd41-b5a6-49f1-bc4c-5e8dc1421d91","resolution":{"observed_at":"2026-08-15T20:02:42.592620Z","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":"2026-08-15T20:02:42.608129Z","title":"The peak frequency of GW energy spectrum can be estimated 6 as fp = 1.1×10−9Hz g∗(Tann) 10 1/2 × g∗s(Tann) 10 −1/3 Tann 10−2GeV","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.608129Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:3b2163e0c7fe9ee643e61c5b5b8fcd21a5ee69c45e9738139132e95de6f41d5e","observation_id":"6c8a61f3-1932-4c7a-9d16-8fd91a11f5c8","resolution":{"observed_at":"2026-08-15T20:02:42.608129Z","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":"2026-08-15T20:02:42.617271Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.617271Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:44ccbdeceab2c8857a1a4eb3aad74c1aa500c128515b49623e70c6ad768cc4ad","observation_id":"a846214e-a0ba-4bfd-9c75-7e7cf68e94b5","resolution":{"observed_at":"2026-08-15T20:02:42.617271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01174","last_updated":"2015-01-23T14:02:18Z","snapshot_observed_at":"2026-08-14T23:05:05.927991Z","submitted_at":"2015-01-06T13:36:50Z","title":"Stochastic background of gravitational waves from cosmological sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01174","snapshot_observed_at":"2026-08-15T20:02:42.623993Z","title":"Caprini, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.623993Z"},"links":{"cited_paper":"/paper/1501.01174","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2975eda7747f2ad28be0ad7b883ab6a670a79b873452cf64f242415ccdd68426","observation_id":"09fad32c-8cd0-494a-b4ec-2501f90164c4","resolution":{"observed_at":"2026-08-15T20:02:42.623993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.00786","last_updated":"2018-11-12T10:20:57Z","snapshot_observed_at":"2026-08-14T18:56:34.764746Z","submitted_at":"2018-07-02T17:01:37Z","title":"Probing the Universe through the Stochastic Gravitational Wave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.00786","snapshot_observed_at":"2026-08-15T20:02:42.630979Z","title":"Kuroyanagi, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.630979Z"},"links":{"cited_paper":"/paper/1807.00786","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:c32ba4e8be9bb82fe35fea3857f9b5a5d01f5286c20df26b95133be326071e2b","observation_id":"d15df7fe-663c-4371-b547-ac18832ae206","resolution":{"observed_at":"2026-08-15T20:02:42.630979Z","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":"2026-08-14T19:55:33.819188Z","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":"2026-08-15T20:02:42.638017Z","title":"Caprini and D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.638017Z"},"links":{"cited_paper":"/paper/1801.04268","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:63a358399cefb1d634187d79837dcf4db1fdf231aac63c45951fe2a33bf201d3","observation_id":"5d6f3494-cdca-483e-89c2-4e79d21e5b34","resolution":{"observed_at":"2026-08-15T20:02:42.638017Z","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":"2026-08-16T00:15:29.463316Z","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":"2026-08-15T20:02:42.646528Z","title":"Christensen, Rept","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.646528Z"},"links":{"cited_paper":"/paper/1811.08797","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:125a8810e6bfb43c17506eed7d6866b6e85def7d6f9fb02971001d8877da2751","observation_id":"ca378ac0-eb94-4a3c-84fe-d8bfaa745f8c","resolution":{"observed_at":"2026-08-15T20:02:42.646528Z","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":"2026-08-14T18:17:16.395573Z","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":"2026-08-15T20:02:42.662493Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.662493Z"},"links":{"cited_paper":"/paper/2202.00178","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:769cfbaa0676270876179e24b4a96b5e07e32dde227c9acb626c06ec62d7f752","observation_id":"dafe2d27-811a-4e41-a317-74f105be4718","resolution":{"observed_at":"2026-08-15T20:02:42.662493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16213","last_updated":"2023-06-28T13:51:01Z","snapshot_observed_at":"2026-08-13T16:50:10.214371Z","submitted_at":"2023-06-28T13:51:01Z","title":"The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16213","snapshot_observed_at":"2026-08-15T20:02:42.676130Z","title":"Agazie et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.676130Z"},"links":{"cited_paper":"/paper/2306.16213","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:c8e667bc0f7f3d25ab16ca11c4b21034dd4377797997b88e504b2a0317097264","observation_id":"fa14cdd4-d2d8-4375-9f9d-fd5183d93412","resolution":{"observed_at":"2026-08-15T20:02:42.676130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16217","last_updated":"2023-06-28T13:51:05Z","snapshot_observed_at":"2026-08-14T19:15:08.563543Z","submitted_at":"2023-06-28T13:51:05Z","title":"The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16217","snapshot_observed_at":"2026-08-15T20:02:42.688327Z","title":"Agazie et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.688327Z"},"links":{"cited_paper":"/paper/2306.16217","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:afa90ed84bc19bc19acb235a480bc2fd66104dcf02eedfc23ce57de21dc0efb7","observation_id":"f44605f0-e3ee-438b-9a09-7f53f2e1778c","resolution":{"observed_at":"2026-08-15T20:02:42.688327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16214","last_updated":"2023-06-28T13:51:02Z","snapshot_observed_at":"2026-08-15T04:04:48.616971Z","submitted_at":"2023-06-28T13:51:02Z","title":"The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16214","snapshot_observed_at":"2026-08-15T20:02:42.694586Z","title":"Antoniadis et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.694586Z"},"links":{"cited_paper":"/paper/2306.16214","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:497af5e7dc552048fd36be14e5a4ba33cad8ef5f1ddb821264d69cf666984480","observation_id":"ea212e78-3e28-45b2-8fe5-d915ca2a43d9","resolution":{"observed_at":"2026-08-15T20:02:42.694586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16224","last_updated":"2023-06-28T13:51:12Z","snapshot_observed_at":"2026-08-13T11:07:35.204668Z","submitted_at":"2023-06-28T13:51:12Z","title":"The second data release from the European Pulsar Timing Array I. The dataset and timing analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16224","snapshot_observed_at":"2026-08-15T20:02:42.702997Z","title":"Antoniadis et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.702997Z"},"links":{"cited_paper":"/paper/2306.16224","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:efbf36abbdcd1871fb43f70e229a6bf91da8bd111db19b67e5376ab8beef82d0","observation_id":"75ae9511-69de-4eba-ac6b-1009f3c856f2","resolution":{"observed_at":"2026-08-15T20:02:42.702997Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16227","last_updated":"2024-05-15T21:59:54Z","snapshot_observed_at":"2026-08-14T11:05:59.787839Z","submitted_at":"2023-06-28T13:51:15Z","title":"The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16227","snapshot_observed_at":"2026-08-15T20:02:42.718408Z","title":"Antoniadis et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.718408Z"},"links":{"cited_paper":"/paper/2306.16227","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:57fa055df740934b9f0c05e1cb328f2410fc8339c33512b40feb4544dbed4021","observation_id":"9322b158-9ed5-4dca-92e8-140ec713fc55","resolution":{"observed_at":"2026-08-15T20:02:42.718408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16215","last_updated":"2023-06-28T13:51:03Z","snapshot_observed_at":"2026-08-12T23:01:24.461267Z","submitted_at":"2023-06-28T13:51:03Z","title":"Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16215","snapshot_observed_at":"2026-08-15T20:02:42.727773Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.727773Z"},"links":{"cited_paper":"/paper/2306.16215","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:4c32844d90ab7f7ede0466d45d27610eea6e3a9efa2abb4dc5afd0508ce84346","observation_id":"cffa2289-94b4-4420-9319-cf80451bc966","resolution":{"observed_at":"2026-08-15T20:02:42.727773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16216","last_updated":"2023-06-28T13:51:04Z","snapshot_observed_at":"2026-08-08T13:18:07.452026Z","submitted_at":"2023-06-28T13:51:04Z","title":"Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16216","snapshot_observed_at":"2026-08-15T20:02:42.949250Z","title":"Xu et al., Res","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.949250Z"},"links":{"cited_paper":"/paper/2306.16216","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:8f81c8b7aa61388b5600fe199cb928fbc34e5fc3f63029a965d4a77143dd9673","observation_id":"6b5301e7-75f6-4113-b10e-7388aadc1e9e","resolution":{"observed_at":"2026-08-15T20:02:42.949250Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16220","last_updated":"2023-07-18T21:46:28Z","snapshot_observed_at":"2026-08-13T18:26:24.557829Z","submitted_at":"2023-06-28T13:51:08Z","title":"The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16220","snapshot_observed_at":"2026-08-15T20:02:42.957786Z","title":"Agazie et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.957786Z"},"links":{"cited_paper":"/paper/2306.16220","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:80af4f9881e7d1203e2270c349e274ff5c9ee3cf9ac6f537308847a8975bb5cf","observation_id":"2c406fe5-d471-45e7-bff0-6b36f8955bf3","resolution":{"observed_at":"2026-08-15T20:02:42.957786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17021","last_updated":"2024-01-12T16:51:20Z","snapshot_observed_at":"2026-08-13T11:06:01.050916Z","submitted_at":"2023-06-29T15:13:27Z","title":"Gravitational Waves from SMBH Binaries in Light of the NANOGrav 15-Year Data","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17021","snapshot_observed_at":"2026-08-15T20:02:42.969692Z","title":"Ellis, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.969692Z"},"links":{"cited_paper":"/paper/2306.17021","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f3d950dd897d89f805e1ac267838bff2325544044bdc86d684d805623845fb59","observation_id":"f852978d-3310-49f4-a024-c94eddd6e23b","resolution":{"observed_at":"2026-08-15T20:02:42.969692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17143","last_updated":"2025-06-26T06:30:08Z","snapshot_observed_at":"2026-08-13T11:05:53.230588Z","submitted_at":"2023-06-29T17:46:37Z","title":"Dark Matter Spike surrounding Supermassive Black Holes Binary and the Nanohertz Stochastic Gravitational Wave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17143","snapshot_observed_at":"2026-08-15T20:02:42.979538Z","title":"Shen, G.-W","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.979538Z"},"links":{"cited_paper":"/paper/2306.17143","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:9b1a25bc3cbb611c5edda8fc5cfd8ec91a56d8cb000359efb2754577de50bb31","observation_id":"e4fec0aa-9dbb-43cb-842c-8c29138ca202","resolution":{"observed_at":"2026-08-15T20:02:42.979538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17158","last_updated":"2023-07-03T12:45:58Z","snapshot_observed_at":"2026-08-13T11:05:51.090712Z","submitted_at":"2023-06-29T17:57:55Z","title":"Probing the Dark Matter density with gravitational waves from super-massive binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17158","snapshot_observed_at":"2026-08-15T20:02:42.985294Z","title":"Ghoshal and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.985294Z"},"links":{"cited_paper":"/paper/2306.17158","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:83d3240c93bc371f39bc1e725d2e2389fc2ab455dd15c9482fdfb130f22a30da","observation_id":"076021a1-9a42-41fe-9295-4155403eb064","resolution":{"observed_at":"2026-08-15T20:02:42.985294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.00722","last_updated":"2023-11-15T02:03:33Z","snapshot_observed_at":"2026-08-13T11:04:07.035551Z","submitted_at":"2023-07-03T03:01:11Z","title":"Implications for the Supermassive Black Hole Binaries from the NANOGrav 15-year Data Set","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.00722","snapshot_observed_at":"2026-08-15T20:02:42.995259Z","title":"Bi, Y.-M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:42.995259Z"},"links":{"cited_paper":"/paper/2307.00722","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:64ef44322f8664739007a375929385b562ca3d08b187aa26d015276dee57fa49","observation_id":"8b55335a-958f-4477-8098-7f2363dfd87b","resolution":{"observed_at":"2026-08-15T20:02:42.995259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01093","last_updated":"2023-07-03T15:13:03Z","snapshot_observed_at":"2026-08-13T11:03:40.416432Z","submitted_at":"2023-07-03T15:13:03Z","title":"Detecting new fundamental fields with Pulsar Timing Arrays","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01093","snapshot_observed_at":"2026-08-15T20:02:43.007896Z","title":"Zhang, N","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.007896Z"},"links":{"cited_paper":"/paper/2307.01093","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e25a141e36d1515b468ac0b3e4d577173a8339b1d54d675e06740edcd380b8b7","observation_id":"223d00b4-d3ed-42f0-9e5a-4c830a4a3bf3","resolution":{"observed_at":"2026-08-15T20:02:43.007896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17086","last_updated":"2023-07-08T03:12:45Z","snapshot_observed_at":"2026-08-13T11:05:56.257653Z","submitted_at":"2023-06-29T16:40:39Z","title":"NANOGrav Signal from a Dark Conformal Phase Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17086","snapshot_observed_at":"2026-08-15T20:02:43.017075Z","title":"Fujikura, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.017075Z"},"links":{"cited_paper":"/paper/2306.17086","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:c25c7550eeb3e6bbc586b9dcf2d5ec087cf82ce0e4c238be334646d968884f4c","observation_id":"cdcd28ab-513a-41d0-ba90-5e168416d163","resolution":{"observed_at":"2026-08-15T20:02:43.017075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17205","last_updated":"2023-06-29T14:42:24Z","snapshot_observed_at":"2026-08-13T11:06:03.842686Z","submitted_at":"2023-06-29T14:42:24Z","title":"Have pulsar timing array methods detected a cosmological phase transition?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17205","snapshot_observed_at":"2026-08-15T20:02:43.027833Z","title":"Addazi, Y.-F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.027833Z"},"links":{"cited_paper":"/paper/2306.17205","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e07e97105173ffaefaa1050b56140fe1e85de208cc37a16f7f1fb0fe32c5eba9","observation_id":"80edcdad-13d0-4a63-9dcb-7e797ec200c1","resolution":{"observed_at":"2026-08-15T20:02:43.027833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17071","last_updated":"2023-08-04T15:17:09Z","snapshot_observed_at":"2026-08-13T11:05:57.224744Z","submitted_at":"2023-06-29T16:17:56Z","title":"Pulsar Timing Array Stochastic Background from light Kaluza-Klein resonances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17071","snapshot_observed_at":"2026-08-15T20:02:43.033742Z","title":"Megias, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.033742Z"},"links":{"cited_paper":"/paper/2306.17071","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f5e0a5f3a36d8786c6e1496b75abea0738ad41e249a3f048932e799cad84de60","observation_id":"30433485-3667-4a9f-a2c4-c6a01b604b64","resolution":{"observed_at":"2026-08-15T20:02:43.033742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01072","last_updated":"2023-11-20T13:19:30Z","snapshot_observed_at":"2026-08-13T11:03:42.378113Z","submitted_at":"2023-07-03T14:53:57Z","title":"Implications of Nano-Hertz Gravitational Waves on Electroweak Phase Transition in the Singlet Dark Matter Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01072","snapshot_observed_at":"2026-08-15T20:02:43.042177Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.042177Z"},"links":{"cited_paper":"/paper/2307.01072","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:188aab281d7b64e977ce415de35081b71ca7be6b8440ef00fd9418221ba9ee61","observation_id":"d0f7f96a-74ef-4e46-9fc4-bfe9af028efe","resolution":{"observed_at":"2026-08-15T20:02:43.042177Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01086","last_updated":"2023-09-06T01:24:06Z","snapshot_observed_at":"2026-08-13T11:03:41.084956Z","submitted_at":"2023-07-03T15:07:43Z","title":"A collider test of nano-Hertz gravitational waves from pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01086","snapshot_observed_at":"2026-08-15T20:02:43.048835Z","title":"Li and K.-P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.048835Z"},"links":{"cited_paper":"/paper/2307.01086","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:9f85a69fc693da7efbce599c36e24514c65ff3eba41e73aaeb92c50fd5a0ed20","observation_id":"1d2c683c-6b66-4e24-bdfd-05846d200023","resolution":{"observed_at":"2026-08-15T20:02:43.048835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.12385","last_updated":"2023-12-15T11:51:59Z","snapshot_observed_at":"2026-08-13T10:49:35.225052Z","submitted_at":"2023-07-23T17:28:01Z","title":"Heavy QCD axion model in light of pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.12385","snapshot_observed_at":"2026-08-15T20:02:43.055303Z","title":"Ahmadvand, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.055303Z"},"links":{"cited_paper":"/paper/2307.12385","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e9413010341a88ac4e2d5dd4859228728f07721968254ce015f7fc9a6d8a6ade","observation_id":"dcd52cf5-dd22-46e6-9bd9-334b0791949b","resolution":{"observed_at":"2026-08-15T20:02:43.055303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04239","last_updated":"2023-11-15T13:51:03Z","snapshot_observed_at":"2026-08-13T10:59:26.755897Z","submitted_at":"2023-07-09T17:57:20Z","title":"First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04239","snapshot_observed_at":"2026-08-15T20:02:43.064082Z","title":"Gouttenoire, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.064082Z"},"links":{"cited_paper":"/paper/2307.04239","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:04ef30e457b98c5bd143d37b5b7c58f8e289e933261dd9e310f02a2631a23511","observation_id":"c77272ae-d3f7-4e75-9c06-7a1aa5476314","resolution":{"observed_at":"2026-08-15T20:02:43.064082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17830","last_updated":"2023-06-30T17:50:20Z","snapshot_observed_at":"2026-08-14T22:28:40.024933Z","submitted_at":"2023-06-30T17:50:20Z","title":"Axionic domain walls at Pulsar Timing Arrays: QCD bias and particle friction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17830","snapshot_observed_at":"2026-08-15T20:02:43.082762Z","title":"Blasi, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.082762Z"},"links":{"cited_paper":"/paper/2306.17830","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:ff273c0596aa3ba26b8bda0e33ec126bb0430edf1ddd76e76b6df339a223c9d0","observation_id":"d0028d87-6322-4eb3-9966-93ede59d0e32","resolution":{"observed_at":"2026-08-15T20:02:43.082762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.00656","last_updated":"2023-09-20T08:14:17Z","snapshot_observed_at":"2026-08-13T11:04:12.293869Z","submitted_at":"2023-07-02T20:21:15Z","title":"Scale of Dirac leptogenesis and left-right symmetry in the light of recent PTA results","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.00656","snapshot_observed_at":"2026-08-15T20:02:43.101382Z","title":"Barman, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.101382Z"},"links":{"cited_paper":"/paper/2307.00656","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2c2821687a89274f8718c703b429fb5e19d07b039e841dc10f71a27e528bf3ea","observation_id":"cc8123be-95dd-4d50-86d2-ab3472ed7e65","resolution":{"observed_at":"2026-08-15T20:02:43.101382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04582","last_updated":"2023-12-08T17:56:58Z","snapshot_observed_at":"2026-08-13T10:59:02.306473Z","submitted_at":"2023-07-10T14:19:55Z","title":"NANOGrav spectral index $\\gamma=3$ from melting domain walls","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04582","snapshot_observed_at":"2026-08-15T20:02:43.108785Z","title":"Babichev, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.108785Z"},"links":{"cited_paper":"/paper/2307.04582","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:58341a83be98a11e5bba8dee5207c8d2b15d65e88244dc846e4f6d5dbf0af1c3","observation_id":"f804f64a-2a2c-4d9e-95d9-7e3538e27826","resolution":{"observed_at":"2026-08-15T20:02:43.108785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.07665","last_updated":"2023-11-28T21:15:05Z","snapshot_observed_at":"2026-08-13T10:55:10.295253Z","submitted_at":"2023-07-15T00:26:26Z","title":"Catastrogenesis with unstable ALPs as the origin of the NANOGrav 15 yr gravitational wave signal","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.07665","snapshot_observed_at":"2026-08-15T20:02:43.116280Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.116280Z"},"links":{"cited_paper":"/paper/2307.07665","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e53841a804978584f0cebe5b7f2621f963a55c8cba4ec30f8d8432c7489a9bba","observation_id":"4792cbd4-91ca-4267-a96f-1530f15ebfb5","resolution":{"observed_at":"2026-08-15T20:02:43.116280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11495","last_updated":"2023-11-22T03:14:23Z","snapshot_observed_at":"2026-08-14T09:34:26.395885Z","submitted_at":"2023-07-21T10:58:15Z","title":"Nano-Hertz gravitational waves from collapsing domain walls associated with freeze-in dark matter in light of pulsar timing array observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.11495","snapshot_observed_at":"2026-08-15T20:02:43.125287Z","title":"Zhang, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.125287Z"},"links":{"cited_paper":"/paper/2307.11495","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:b8a233dd3fd9f192c16ce6aac1304e7f48b3595666902127a18a70f91f648a24","observation_id":"070cca09-b4c6-44a1-ba6f-622e54469805","resolution":{"observed_at":"2026-08-15T20:02:43.125287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17147","last_updated":"2023-07-05T17:41:47Z","snapshot_observed_at":"2026-08-13T11:06:04.308054Z","submitted_at":"2023-06-29T17:49:59Z","title":"Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17147","snapshot_observed_at":"2026-08-15T20:02:43.134778Z","title":"Ellis, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.134778Z"},"links":{"cited_paper":"/paper/2306.17147","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:935df7061f76820112113fe034a1b57e0f796cbd85d0baa2b226decef8168c4f","observation_id":"21d71f63-4304-41d6-80ef-c0ddad007e18","resolution":{"observed_at":"2026-08-15T20:02:43.134778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17390","last_updated":"2023-06-30T03:48:05Z","snapshot_observed_at":"2026-08-13T11:05:38.560942Z","submitted_at":"2023-06-30T03:48:05Z","title":"Nanohertz gravitational waves from cosmic strings and dark photon dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17390","snapshot_observed_at":"2026-08-15T20:02:43.144212Z","title":"Kitajima and K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.144212Z"},"links":{"cited_paper":"/paper/2306.17390","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:73474137176221e36bebdf977c3edae9e271d0c9e50341b1a954e194c378045c","observation_id":"862b277f-855e-49f7-9cd8-9227770bfe98","resolution":{"observed_at":"2026-08-15T20:02:43.144212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17150","last_updated":"2023-11-15T04:53:02Z","snapshot_observed_at":"2026-08-13T11:05:51.908567Z","submitted_at":"2023-06-29T17:51:33Z","title":"The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17150","snapshot_observed_at":"2026-08-15T20:02:43.152438Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.152438Z"},"links":{"cited_paper":"/paper/2306.17150","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f0d1858234cb9e02adfa1a09b4ef6167176cb11cfe595c0f496c36631e9f3c14","observation_id":"841b6d70-5bfa-4769-8691-923aa1b46d5b","resolution":{"observed_at":"2026-08-15T20:02:43.152438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17788","last_updated":"2023-11-27T17:00:44Z","snapshot_observed_at":"2026-08-13T11:05:00.421425Z","submitted_at":"2023-06-30T16:42:37Z","title":"Superheavy quasi-stable strings and walls bounded by strings in the light of NANOGrav 15 year data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17788","snapshot_observed_at":"2026-08-15T20:02:43.162975Z","title":"Lazarides, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.162975Z"},"links":{"cited_paper":"/paper/2306.17788","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:45680fbd7edc778f44f2369df660e90ad9ea864c2b9b458c74cd8cc181e7f28f","observation_id":"2de2edae-f3a7-45b1-812a-4e7ccf72a68b","resolution":{"observed_at":"2026-08-15T20:02:43.162975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17718","last_updated":"2024-01-31T17:53:58Z","snapshot_observed_at":"2026-08-13T11:05:06.834227Z","submitted_at":"2023-06-30T15:02:29Z","title":"From quantum gravity to gravitational waves through cosmic strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17718","snapshot_observed_at":"2026-08-15T20:02:43.184174Z","title":"Eichhorn, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.184174Z"},"links":{"cited_paper":"/paper/2306.17718","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:93333f5119c1ff2f14674bafb1c726c2ca3016cebce90de4c3b10074d6c9cf25","observation_id":"9b45f2fe-a4cc-4d4a-b23c-3103e6a53ebc","resolution":{"observed_at":"2026-08-15T20:02:43.184174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.06586","last_updated":"2023-08-17T09:58:27Z","snapshot_observed_at":"2026-08-13T10:57:02.234011Z","submitted_at":"2023-07-13T07:06:49Z","title":"Dark baryon from pure Yang-Mills theory and its GW signature from cosmic strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.06586","snapshot_observed_at":"2026-08-15T20:02:43.195712Z","title":"Yamada and K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.195712Z"},"links":{"cited_paper":"/paper/2307.06586","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e9cd30281387aa02cc6e79a27a6182badaa0b26f9cb4c55e1850437252cfe44b","observation_id":"3e8c1bd3-3bca-4d58-b811-d5b287adda1a","resolution":{"observed_at":"2026-08-15T20:02:43.195712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17149","last_updated":"2023-11-14T21:32:00Z","snapshot_observed_at":"2026-08-13T11:05:52.210017Z","submitted_at":"2023-06-29T17:51:16Z","title":"The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17149","snapshot_observed_at":"2026-08-15T20:02:43.226553Z","title":"Franciolini, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.226553Z"},"links":{"cited_paper":"/paper/2306.17149","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2b31af0f7e0ba593760dfe7cede2f53ee9cdd37736146a9e4ceb978d6a52939a","observation_id":"de4c24d6-6a5f-4514-bbaf-6c8a58b3ce0a","resolution":{"observed_at":"2026-08-15T20:02:43.226553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16912","last_updated":"2023-07-05T07:13:46Z","snapshot_observed_at":"2026-08-13T11:06:46.844126Z","submitted_at":"2023-06-29T13:04:58Z","title":"Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16912","snapshot_observed_at":"2026-08-15T20:02:43.241153Z","title":"Vagnozzi, JHEAp 39, 81 (2023), arXiv:2306.16912 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.241153Z"},"links":{"cited_paper":"/paper/2306.16912","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:bac792480a79518994f8c326a549341853a9871667a02cca1c41f74e03c2786e","observation_id":"64188841-4136-4b26-aeb1-bb7e82bf95df","resolution":{"observed_at":"2026-08-15T20:02:43.241153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17834","last_updated":"2024-02-27T03:49:39Z","snapshot_observed_at":"2026-08-14T21:28:00.459119Z","submitted_at":"2023-06-30T17:54:19Z","title":"The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17834","snapshot_observed_at":"2026-08-15T20:02:43.247784Z","title":"Inomata, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.247784Z"},"links":{"cited_paper":"/paper/2306.17834","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:13aa58215aa1d3d8194021d6a40382a9359d18a6f76f0330d86e402c73f213e5","observation_id":"2abdf6df-daec-4503-8aff-8ee8d5edf626","resolution":{"observed_at":"2026-08-15T20:02:43.247784Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17822","last_updated":"2023-12-20T04:49:43Z","snapshot_observed_at":"2026-08-13T11:04:58.125858Z","submitted_at":"2023-06-30T17:40:08Z","title":"Limits on scalar-induced gravitational waves from the stochastic background by pulsar timing array observations","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17822","snapshot_observed_at":"2026-08-15T20:02:43.255580Z","title":"Cai, X.-C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.255580Z"},"links":{"cited_paper":"/paper/2306.17822","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:491689d06288179a4a09b37a3f69a93061ad62500ce3a75e2c752d0c1e92231f","observation_id":"0e521564-3061-4793-83e3-f3ee02d5e8d0","resolution":{"observed_at":"2026-08-15T20:02:43.255580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01102","last_updated":"2024-01-18T09:28:31Z","snapshot_observed_at":"2026-08-14T15:07:54.609737Z","submitted_at":"2023-07-03T15:27:23Z","title":"Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01102","snapshot_observed_at":"2026-08-15T20:02:43.264012Z","title":"Liu, Z.-C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.264012Z"},"links":{"cited_paper":"/paper/2307.01102","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:39e57ca7910991ddc19fd80f060ddd753d9f7b7e2e0d08ef68e290f53a585452","observation_id":"d1d34330-d6ec-4486-a7e9-ddd8d5301254","resolution":{"observed_at":"2026-08-15T20:02:43.264012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.01653","last_updated":"2023-12-05T05:32:30Z","snapshot_observed_at":"2026-08-13T11:03:04.404758Z","submitted_at":"2023-07-04T11:19:54Z","title":"Translating nano-Hertz gravitational wave background into primordial perturbations taking account of the cosmological QCD phase transition","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.01653","snapshot_observed_at":"2026-08-15T20:02:43.271903Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.271903Z"},"links":{"cited_paper":"/paper/2307.01653","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:3fcec42afceafbd14b616af1c29f3389a9cc774bb3e8655f6e4bdd34c1c8d27a","observation_id":"21f36aed-d6f6-4936-9dbb-150b7b29af6f","resolution":{"observed_at":"2026-08-15T20:02:43.271903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.02467","last_updated":"2023-11-16T15:00:14Z","snapshot_observed_at":"2026-08-13T11:02:09.127413Z","submitted_at":"2023-07-05T17:41:35Z","title":"Scalar induced gravitational waves in light of Pulsar Timing Array data","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02467","snapshot_observed_at":"2026-08-15T20:02:43.278021Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.278021Z"},"links":{"cited_paper":"/paper/2307.02467","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:60674ec57a9e1a698f5e6b2581ada65de20dfaf098227ff82b676f4d30d35ab6","observation_id":"ef6ccec1-1725-4f89-96de-d9e2629e22da","resolution":{"observed_at":"2026-08-15T20:02:43.278021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03164","last_updated":"2023-10-08T13:04:41Z","snapshot_observed_at":"2026-08-13T11:00:44.463223Z","submitted_at":"2023-07-06T17:46:58Z","title":"Induced Gravitational Waves from Ultra Slow-Roll Inflation and Pulsar Timing Arrays Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03164","snapshot_observed_at":"2026-08-15T20:02:43.284343Z","title":"Firouzjahi and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.284343Z"},"links":{"cited_paper":"/paper/2307.03164","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:6f59ac3a1a22af124e92c15d083f13d96b86a67af6aed82bf8d0e1fc8c79d911","observation_id":"1f10f2e5-0698-45e9-bf14-411a5078262e","resolution":{"observed_at":"2026-08-15T20:02:43.284343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04694","last_updated":"2024-03-22T07:40:03Z","snapshot_observed_at":"2026-08-16T01:42:28.789038Z","submitted_at":"2023-07-10T16:46:46Z","title":"Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04694","snapshot_observed_at":"2026-08-15T20:02:43.298878Z","title":"Salvio, JCAP 12, 046 (2023), arXiv:2307.04694 [hep- ph]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.298878Z"},"links":{"cited_paper":"/paper/2307.04694","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:6b2e474c1bd758294e0db63d3c3e59103b35f463502526c55b60be3a8ca7ac69","observation_id":"0aee89c4-80b8-4b49-9ad7-a4137b935910","resolution":{"observed_at":"2026-08-15T20:02:43.298878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04419","last_updated":"2023-10-30T14:16:11Z","snapshot_observed_at":"2026-08-15T12:49:12.743202Z","submitted_at":"2023-07-10T08:51:04Z","title":"Constraints on primordial curvature power spectrum with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04419","snapshot_observed_at":"2026-08-15T20:02:43.305849Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.305849Z"},"links":{"cited_paper":"/paper/2307.04419","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2f44c7487621a555678365007082a7707be4455ff13d491cc3d3152fd9942bcc","observation_id":"3a81440e-7f7f-4be1-95a5-afebf3328ebe","resolution":{"observed_at":"2026-08-15T20:02:43.305849Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.05455","last_updated":"2024-02-22T16:16:49Z","snapshot_observed_at":"2026-08-13T10:58:03.071133Z","submitted_at":"2023-07-11T17:43:04Z","title":"Can the gravitational wave background feel wiggles in spacetime?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.05455","snapshot_observed_at":"2026-08-15T20:02:43.313716Z","title":"Ye and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.313716Z"},"links":{"cited_paper":"/paper/2307.05455","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:d7be5b4071abee32d7d4a73362513ba1bb55ea9303a66dc949d8cbb010064a2f","observation_id":"5c5a4acb-8cbb-493f-a9ca-71bc5b2ab550","resolution":{"observed_at":"2026-08-15T20:02:43.313716Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.06757","last_updated":"2023-08-17T09:16:43Z","snapshot_observed_at":"2026-08-16T03:51:45.388457Z","submitted_at":"2023-07-13T13:53:15Z","title":"PBHs and GWs from $\\mathbb{T}^2$-inflation and NANOGrav 15-year data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.06757","snapshot_observed_at":"2026-08-15T20:02:43.322905Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.322905Z"},"links":{"cited_paper":"/paper/2307.06757","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:803b8e06c27f3d904830833170bbb03287390ce7bbf9fcf9ba5a93c550662e1f","observation_id":"df045ffb-24f4-44ba-ac9d-75031be62125","resolution":{"observed_at":"2026-08-15T20:02:43.322905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08552","last_updated":"2023-07-17T15:14:47Z","snapshot_observed_at":"2026-08-13T10:54:09.154083Z","submitted_at":"2023-07-17T15:14:47Z","title":"Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08552","snapshot_observed_at":"2026-08-15T20:02:43.330379Z","title":"Balaji, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.330379Z"},"links":{"cited_paper":"/paper/2307.08552","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:70907fd8d7f91ce3d91f7a79c1a7097dfbf67cc495717f70a10279f639452777","observation_id":"3d5deb63-2cb5-48f1-aef4-bfdea60b7137","resolution":{"observed_at":"2026-08-15T20:02:43.330379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.08687","last_updated":"2023-09-07T14:40:47Z","snapshot_observed_at":"2026-08-13T10:54:01.104909Z","submitted_at":"2023-07-17T17:48:03Z","title":"Confronting sound speed resonance with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.08687","snapshot_observed_at":"2026-08-15T20:02:43.338621Z","title":"Jin, Z.-C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.338621Z"},"links":{"cited_paper":"/paper/2307.08687","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:04941e45cbec7054c4788bb9998ea7eb2847cb17010932c15c17ed7660bbb8d6","observation_id":"37c9c4c7-8a66-4f90-b4a6-2576692093d4","resolution":{"observed_at":"2026-08-15T20:02:43.338621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.12913","last_updated":"2023-11-08T17:50:57Z","snapshot_observed_at":"2026-08-13T10:48:59.273508Z","submitted_at":"2023-07-24T16:12:38Z","title":"Gravitational wave background from quintessential inflation and NANOGrav data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.12913","snapshot_observed_at":"2026-08-15T20:02:43.350466Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.350466Z"},"links":{"cited_paper":"/paper/2307.12913","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:a4a97e72828c9d88021a38ff99b0a2bfdfcd2b946d1e9be0f6fb94655a0089c6","observation_id":"1a4d49db-2a50-4556-b39a-0bde5fa9d0be","resolution":{"observed_at":"2026-08-15T20:02:43.350466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15123","last_updated":"2023-10-05T17:37:48Z","snapshot_observed_at":"2026-08-13T10:45:58.283001Z","submitted_at":"2023-07-27T18:00:07Z","title":"Probing The Early Universe Cosmology With NANOGrav: Possibilities and Limitations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15123","snapshot_observed_at":"2026-08-15T20:02:43.360074Z","title":"Ben-Dayan, U","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.360074Z"},"links":{"cited_paper":"/paper/2307.15123","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f9df6244a835cb41fdb22e7d3755f8378dae691e715c592ddf738cefe8c82d27","observation_id":"ac732a4b-2a7c-4eee-a24c-064dd052c1a7","resolution":{"observed_at":"2026-08-15T20:02:43.360074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.14911","last_updated":"2023-10-30T13:36:32Z","snapshot_observed_at":"2026-08-14T07:29:36.537758Z","submitted_at":"2023-07-27T14:55:08Z","title":"Probing the equation of state of the early Universe with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.14911","snapshot_observed_at":"2026-08-15T20:02:43.367776Z","title":"Liu, Z.-C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.367776Z"},"links":{"cited_paper":"/paper/2307.14911","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:d5cafc6860449dfe84727d48ef4e9e74436f965d89abd3bb8e58e150201eac61","observation_id":"7da03f32-ab2c-4d73-810b-c183eb6beaf1","resolution":{"observed_at":"2026-08-15T20:02:43.367776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.05632","last_updated":"2024-02-01T08:28:12Z","snapshot_observed_at":"2026-08-13T10:37:10.676773Z","submitted_at":"2023-08-10T15:19:46Z","title":"Model-independent reconstruction of the primordial curvature power spectrum from PTA data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.05632","snapshot_observed_at":"2026-08-15T20:02:43.374592Z","title":"Yi, Z.-Q","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.374592Z"},"links":{"cited_paper":"/paper/2308.05632","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:8b4c51f0f7ca4dae9d04710e4624c013f1ac8a83a2ffd46aff0657fcad52a89e","observation_id":"959272a6-5bbf-4077-b0fc-94abaf3bfd45","resolution":{"observed_at":"2026-08-15T20:02:43.374592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06915","last_updated":"2023-08-17T10:32:32Z","snapshot_observed_at":"2026-08-13T10:35:11.507815Z","submitted_at":"2023-08-14T03:21:06Z","title":"On the inflationary interpretation of the nHz gravitational-wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06915","snapshot_observed_at":"2026-08-15T20:02:43.387015Z","title":"Frosina and A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.387015Z"},"links":{"cited_paper":"/paper/2308.06915","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:15bbcc3dc72a916bf4186f09dc314261ee9e225bb6c7e93a3535d38b4220fc19","observation_id":"94860a74-b3b6-4d91-b303-ddf2622f546f","resolution":{"observed_at":"2026-08-15T20:02:43.387015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.07912","last_updated":"2023-12-01T11:23:48Z","snapshot_observed_at":"2026-08-13T10:34:07.419269Z","submitted_at":"2023-08-15T17:53:34Z","title":"Ultra-low mass PBHs in the early universe can explain the PTA signal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.07912","snapshot_observed_at":"2026-08-15T20:02:43.402740Z","title":"Bhaumik, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.402740Z"},"links":{"cited_paper":"/paper/2308.07912","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:4fc5f931ed807012215080faddc98b42a3da99007087bf44352b2676be10ed40","observation_id":"0c7adab9-fa88-406d-a20f-aef3af51c135","resolution":{"observed_at":"2026-08-15T20:02:43.402740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.07155","last_updated":"2024-02-18T01:26:50Z","snapshot_observed_at":"2026-08-13T10:34:54.129042Z","submitted_at":"2023-08-14T14:09:12Z","title":"Full analysis of the scalar-induced gravitational waves for the curvature perturbation with local-type non-Gaussianities","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.07155","snapshot_observed_at":"2026-08-15T20:02:43.418784Z","title":"Yuan, D.-S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.418784Z"},"links":{"cited_paper":"/paper/2308.07155","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:6dab847ed2b8f2a154c5a79dc69856b29fbedfa91d13ead7d3a9de24692c3941","observation_id":"daa49899-27ad-4e4b-b913-cebc16135d61","resolution":{"observed_at":"2026-08-15T20:02:43.418784Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.13109","last_updated":"2023-10-03T12:51:03Z","snapshot_observed_at":"2026-08-13T10:48:46.669242Z","submitted_at":"2023-07-24T19:58:25Z","title":"Extra-tensor-induced origin for the PTA signal: No primordial black hole production","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.13109","snapshot_observed_at":"2026-08-15T20:02:43.431216Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.431216Z"},"links":{"cited_paper":"/paper/2307.13109","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:87e810de6b5dbcac38e671d0d096d3f7d89cf43bb8a49229bccc917f0fcb71b8","observation_id":"a3b73561-e12b-412c-b418-bec324b374a6","resolution":{"observed_at":"2026-08-15T20:02:43.431216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16219","last_updated":"2023-06-28T13:51:07Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-06-28T13:51:07Z","title":"The NANOGrav 15-year Data Set: Search for Signals from New Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16219","snapshot_observed_at":"2026-08-15T20:02:43.441420Z","title":"Afzal et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.441420Z"},"links":{"cited_paper":"/paper/2306.16219","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:9f7b1108b70e3817b5082273a22f2d98986f0969e9dfe674b7d7f9d22ccbeb36","observation_id":"30d8eb61-8171-4c05-b4f5-45bacc438cf0","resolution":{"observed_at":"2026-08-15T20:02:43.441420Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.08546","last_updated":"2023-10-09T13:07:48Z","snapshot_observed_at":"2026-08-13T10:33:29.075755Z","submitted_at":"2023-08-16T17:59:15Z","title":"What is the source of the PTA GW signal?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.08546","snapshot_observed_at":"2026-08-15T20:02:43.454694Z","title":"Ellis, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.454694Z"},"links":{"cited_paper":"/paper/2308.08546","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:a5fc4834bfd075cf9b5f0a0fd52be549019439abd7bf270713be211c8dfca43a","observation_id":"02e510e4-0a21-4b4e-b113-819789baa156","resolution":{"observed_at":"2026-08-15T20:02:43.454694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.09637","last_updated":"2020-10-14T19:23:03Z","snapshot_observed_at":"2026-08-13T19:01:25.084256Z","submitted_at":"2019-10-21T20:26:45Z","title":"Probing Primordial Stochastic Gravitational Wave Background with Multi-band Astrophysical Foreground Cleaning","version":4},"cited_work":{"arxiv_id":"1910.09637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.09637","snapshot_observed_at":"2026-08-15T20:02:45.955805Z","title":"Probing Primordial Stochastic Gravitational Wave Background with Multi-band Astrophysical Foreground Cleaning","venue":"astro-ph.CO","work_id":"928511c3-96a9-4d43-a8df-75aec82b8bb8","year":2019},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.478729Z"},"links":{"cited_paper":"/paper/1910.09637","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:9e1aaaf0e8ce21ca59ddf4067e872d30542c8b6e201c082cf9b9ae727625f44a","observation_id":"4b0cb3c9-76be-4290-a65e-5aa7984c494a","resolution":{"observed_at":"2026-08-15T20:02:45.971668Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"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":"2026-08-15T20:02:43.490063Z","title":"Biscoveanu, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.490063Z"},"links":{"cited_paper":"/paper/2009.04418","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f44b486b21850ffaee08547db7ea55a9f161eadd0fad964bfbba5f8c2579a6ac","observation_id":"7b1dd7b0-ebff-4330-a715-8e0b818a4333","resolution":{"observed_at":"2026-08-15T20:02:43.490063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.16116","last_updated":"2020-06-29T15:25:24Z","snapshot_observed_at":"2026-08-09T17:31:03.581161Z","submitted_at":"2020-06-29T15:25:24Z","title":"Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.16116","snapshot_observed_at":"2026-08-15T20:02:43.498922Z","title":"Sharma and J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.498922Z"},"links":{"cited_paper":"/paper/2006.16116","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:34d9dedc5ce9f8e76ae8111d2061cd5e088c6f25dd7d5595a275b866e1141a3f","observation_id":"53bb82e9-ad6a-4adc-a2ab-f7cf0b9a0441","resolution":{"observed_at":"2026-08-15T20:02:43.498922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.01846","last_updated":"2025-01-07T14:25:05Z","snapshot_observed_at":"2026-08-14T16:29:29.295361Z","submitted_at":"2024-03-04T08:54:03Z","title":"Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds. II. Subthreshold binary neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.01846","snapshot_observed_at":"2026-08-15T20:02:43.506818Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.506818Z"},"links":{"cited_paper":"/paper/2403.01846","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:a40045ede32468325e3d8288775029faed6cc3ba6474e7b8855730e4591b0fcb","observation_id":"1b810e55-19ec-4625-86af-36e824d05175","resolution":{"observed_at":"2026-08-15T20:02:43.506818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.04529","last_updated":"2023-07-11T13:31:01Z","snapshot_observed_at":"2026-08-13T13:05:53.374854Z","submitted_at":"2023-01-11T15:47:05Z","title":"Improving the detection sensitivity to primordial stochastic gravitational waves with reduced astrophysical foregrounds","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.04529","snapshot_observed_at":"2026-08-15T20:02:43.518267Z","title":"Pan and H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.518267Z"},"links":{"cited_paper":"/paper/2301.04529","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:cf5a8e075946ccf03fac4a99434340a317756e2e7da766304afee09d5f0fa5ac","observation_id":"dfdceb5d-4801-4d2e-8850-0798170a4770","resolution":{"observed_at":"2026-08-15T20:02:43.518267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.05847","last_updated":"2023-02-22T16:16:34Z","snapshot_observed_at":"2026-08-13T17:35:57.724745Z","submitted_at":"2021-11-10T18:56:00Z","title":"Impact of LIGO-Virgo black hole binaries on gravitational wave background searches","version":2},"cited_work":{"arxiv_id":"2111.05847","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.05847","snapshot_observed_at":"2026-08-15T20:02:45.763022Z","title":"Impact of LIGO-Virgo black hole binaries on gravitational wave background searches","venue":"astro-ph.CO","work_id":"e35fe87d-2f09-43e2-b3eb-07ec09292132","year":2021},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.527997Z"},"links":{"cited_paper":"/paper/2111.05847","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:83473e0fb8b5400b871a4f964d9c76b6a496ca2fb1475595c822c8ccc6751bf3","observation_id":"4e90085d-cb6a-4b3c-b4df-33e922e66e11","resolution":{"observed_at":"2026-08-15T20:02:45.774369Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.03291","last_updated":"2016-01-07T12:36:12Z","snapshot_observed_at":"2026-08-14T22:52:37.215452Z","submitted_at":"2015-04-13T18:45:28Z","title":"Numerical simulations of acoustically generated gravitational waves at a first order phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.03291","snapshot_observed_at":"2026-08-15T20:02:43.535243Z","title":"Hindmarsh, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.535243Z"},"links":{"cited_paper":"/paper/1504.03291","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:1a6727c0c89c544b91ccd41967042205e9350318b48c6c90a4f6583f4ceecc87","observation_id":"2fb39d25-2fcb-43bb-a8cd-7fbfe007313a","resolution":{"observed_at":"2026-08-15T20:02:43.535243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.05712","last_updated":"2018-06-13T18:56:26Z","snapshot_observed_at":"2026-08-14T19:45:31.270868Z","submitted_at":"2018-02-15T15:41:14Z","title":"Gravitational waves from vacuum first-order phase transitions: from the envelope to the lattice","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.05712","snapshot_observed_at":"2026-08-15T20:02:43.544818Z","title":"Cutting, M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.544818Z"},"links":{"cited_paper":"/paper/1802.05712","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:18c96a6902f75e75bd0e52bd79289494dd0b9afef3a1ac6bd21c80ef64724ee8","observation_id":"75f8d65e-ac0a-4cff-8b09-d834e16c43a0","resolution":{"observed_at":"2026-08-15T20:02:43.544818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.15625","last_updated":"2021-08-22T09:03:10Z","snapshot_observed_at":"2026-08-15T15:37:03.938830Z","submitted_at":"2020-12-31T14:27:46Z","title":"Magnetic field and gravitational waves from the first-order Phase Transition","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.15625","snapshot_observed_at":"2026-08-15T20:02:43.559532Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.559532Z"},"links":{"cited_paper":"/paper/2012.15625","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:d8d304c430d9f3946987b18060eb5043616ce87a1e03044c2ed398b78ff18e2c","observation_id":"db8b43f5-e5ab-4d75-bf26-7849d59f3842","resolution":{"observed_at":"2026-08-15T20:02:43.559532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.5001","last_updated":"2014-02-20T09:53:13Z","snapshot_observed_at":"2026-08-15T00:02:34.425298Z","submitted_at":"2013-09-19T14:40:21Z","title":"On the estimation of gravitational wave spectrum from cosmic domain walls","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.5001","snapshot_observed_at":"2026-08-15T20:02:43.570000Z","title":"Hiramatsu, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.570000Z"},"links":{"cited_paper":"/paper/1309.5001","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:d5d06accf4f2aeff8519ee71c20b7883ddc646fde14fd2a3ec8be70217b7420e","observation_id":"243f1f69-a755-47cd-b712-2e16676a9287","resolution":{"observed_at":"2026-08-15T20:02:43.570000Z","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":"2026-08-15T20:02:43.582024Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.582024Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:4d78c71f7fb9d14929db92996b8edf95bf0a8fcee947e1f2527b7fcd6ca0a335","observation_id":"b8e5a6d3-a3d4-4a4f-90b3-2ca1f0dd096a","resolution":{"observed_at":"2026-08-15T20:02:43.582024Z","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":"2026-08-15T20:02:43.587333Z","title":"Liu, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.587333Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:25c30c54c2111abcb27160c5266230c671575a504101fbe620ecba3a3f839caf","observation_id":"93ebdde0-e8eb-4a04-8d15-d95822019e42","resolution":{"observed_at":"2026-08-15T20:02:43.587333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.03857","last_updated":"2025-03-05T19:38:22Z","snapshot_observed_at":"2026-08-12T07:06:10.645304Z","submitted_at":"2025-03-05T19:38:22Z","title":"WIMPs and new physics interpretations of the PTA signal are incompatible","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.03857","snapshot_observed_at":"2026-08-15T20:02:43.602969Z","title":"Gouttenoire, (2025), arXiv:2503.03857 [hep-ph]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.602969Z"},"links":{"cited_paper":"/paper/2503.03857","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:5d1d6fb5d26c4806a6ccab142359daaafab91895ff5a617e9ba93afb237279b5","observation_id":"1ab87c78-5b9b-4872-8453-e162ac11d8a1","resolution":{"observed_at":"2026-08-15T20:02:43.602969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05421","last_updated":"2018-03-05T19:00:00Z","snapshot_observed_at":"2026-08-14T20:03:31.326148Z","submitted_at":"2017-12-14T19:16:44Z","title":"Are ultracompact minihalos really ultracompact?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.05421","snapshot_observed_at":"2026-08-15T20:02:43.614052Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.614052Z"},"links":{"cited_paper":"/paper/1712.05421","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:608083148f4857d51fddaa0b34c558c5726905121e674011c476596efc6a7242","observation_id":"f59491dd-a8b5-40eb-a636-e16d5f859574","resolution":{"observed_at":"2026-08-15T20:02:43.614052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.07389","last_updated":"2018-09-27T18:02:19Z","snapshot_observed_at":"2026-08-15T13:43:46.822387Z","submitted_at":"2018-06-19T18:00:00Z","title":"Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.07389","snapshot_observed_at":"2026-08-15T20:02:43.622128Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.622128Z"},"links":{"cited_paper":"/paper/1806.07389","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:4a06a3d031b9d6428bb8e1f8c1e8f26358d6dcc20235b8832d4614c523a7e6b4","observation_id":"6f3816ce-6717-4087-8680-9debe73c4692","resolution":{"observed_at":"2026-08-15T20:02:43.622128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.2484","last_updated":"2013-02-17T23:41:48Z","snapshot_observed_at":"2026-08-15T04:32:32.808677Z","submitted_at":"2011-10-11T20:00:00Z","title":"Improved constraints on the primordial power spectrum at small scales from ultracompact minihalos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.2484","snapshot_observed_at":"2026-08-15T20:02:43.639101Z","title":"Bringmann, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.639101Z"},"links":{"cited_paper":"/paper/1110.2484","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:9996d5a03f477c8802c9f3062e7bbb513126afb10b0655aa93f124c2c6940a89","observation_id":"3bdc67f4-7042-4f03-8e68-0248beca7c1e","resolution":{"observed_at":"2026-08-15T20:02:43.639101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.04803","last_updated":"2015-06-22T13:00:29Z","snapshot_observed_at":"2026-08-15T08:13:53.847976Z","submitted_at":"2015-03-16T20:00:12Z","title":"Expected properties of the first gravitational wave signal detected with pulsar timing arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.04803","snapshot_observed_at":"2026-08-15T20:02:43.649878Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.649878Z"},"links":{"cited_paper":"/paper/1503.04803","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:61100e35a75a311029ecac0bd4eac7cde33be12728c32bae3197d412849be02e","observation_id":"cc6a5029-1e94-41bb-87b0-194f9ad6766f","resolution":{"observed_at":"2026-08-15T20:02:43.649878Z","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":"2026-08-15T20:02:43.664135Z","title":"Punturo et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.664135Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:b1f117a7632562d69f35c13decab3dc40fa405c2314fb0efda4e7731ae8d22b7","observation_id":"a69e6aab-db91-4485-bf21-5ab9d0164780","resolution":{"observed_at":"2026-08-15T20:02:43.664135Z","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":"2026-08-15T20:02:43.679533Z","title":"Reitze et al., Bull","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.679533Z"},"links":{"cited_paper":"/paper/1907.04833","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2bff2ff80a160eb580e2bc6826d7928ca622164fb635f3a8c66110994e0b4996","observation_id":"ef1eb53a-b2a6-4c81-b7bb-6b852ad67181","resolution":{"observed_at":"2026-08-15T20:02:43.679533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.06239","last_updated":"2016-04-01T10:50:20Z","snapshot_observed_at":"2026-08-14T22:17:47.472294Z","submitted_at":"2015-12-19T12:44:06Z","title":"Science with the space-based interferometer eLISA. II: Gravitational waves from cosmological phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.06239","snapshot_observed_at":"2026-08-15T20:02:43.695234Z","title":"Caprini et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.695234Z"},"links":{"cited_paper":"/paper/1512.06239","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:61c7a7d18cfb0d57fde440654700c1126a87eefd3abddbb656b3f853cd16af44","observation_id":"8aa8dda4-c04a-4f68-925f-b6b63cfe4b58","resolution":{"observed_at":"2026-08-15T20:02:43.695234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13125","last_updated":"2021-01-12T09:42:19Z","snapshot_observed_at":"2026-08-12T20:16:12.772883Z","submitted_at":"2019-10-29T07:58:57Z","title":"Detecting gravitational waves from cosmological phase transitions with LISA: an update","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13125","snapshot_observed_at":"2026-08-15T20:02:43.703087Z","title":"Caprini et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.703087Z"},"links":{"cited_paper":"/paper/1910.13125","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:d73a7c0ee9fdef8f02946c719705179910ff8b692f9fb15a62a612f5ba015230","observation_id":"832f6e44-95bf-4295-b953-e2446b6a1769","resolution":{"observed_at":"2026-08-15T20:02:43.703087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01783","last_updated":"2023-07-27T15:10:31Z","snapshot_observed_at":"2026-08-15T22:10:05.320037Z","submitted_at":"2017-05-04T10:30:07Z","title":"Gravitational waves from a first order electroweak phase transition: a brief review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.01783","snapshot_observed_at":"2026-08-15T20:02:43.713666Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.713666Z"},"links":{"cited_paper":"/paper/1705.01783","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:1575c6bb5752ac2a38d281161de23c0caa08159b798fdc1495ffa66eb20fde12","observation_id":"5c8a2ea0-f85e-4071-8155-00db787cacb8","resolution":{"observed_at":"2026-08-15T20:02:43.713666Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.01948","last_updated":"2019-12-18T20:09:18Z","snapshot_observed_at":"2026-08-15T17:37:55.592148Z","submitted_at":"2018-11-05T19:00:00Z","title":"Cosmic phase transitions: their applications and experimental signatures","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.01948","snapshot_observed_at":"2026-08-15T20:02:43.719663Z","title":"Mazumdar and G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.719663Z"},"links":{"cited_paper":"/paper/1811.01948","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:323b086d7bef15514d24a744ef90b1c0a385cda32a86b22e7997849be0759fe8","observation_id":"a04d5b68-6eef-4962-a497-ad60d093fce8","resolution":{"observed_at":"2026-08-15T20:02:43.719663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14086","last_updated":"2022-08-30T09:06:52Z","snapshot_observed_at":"2026-08-13T14:36:51.457443Z","submitted_at":"2022-08-30T09:06:52Z","title":"Constraining first-order phase transitions with curvature perturbations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14086","snapshot_observed_at":"2026-08-15T20:02:43.733314Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.733314Z"},"links":{"cited_paper":"/paper/2208.14086","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:6ce6ad5decf1ef978c40352572969c974c3c8b86821ec0df574e76064447ae96","observation_id":"7c65f7d1-811d-4f3e-b454-8f1ac0af7b5d","resolution":{"observed_at":"2026-08-15T20:02:43.733314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.03639","last_updated":"2018-08-10T14:17:14Z","snapshot_observed_at":"2026-08-14T19:17:04.748774Z","submitted_at":"2018-05-09T17:59:53Z","title":"Primordial Black Holes from Sound Speed Resonance during Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.03639","snapshot_observed_at":"2026-08-15T20:02:43.744668Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.744668Z"},"links":{"cited_paper":"/paper/1805.03639","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:bb8687ba82f61d6cae5f53be40bed38c0542dd689263b0bf2487da3b163aacb4","observation_id":"f44d7c63-4725-44a2-abeb-ab4bb4a57951","resolution":{"observed_at":"2026-08-15T20:02:43.744668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.10437","last_updated":"2020-06-05T15:49:06Z","snapshot_observed_at":"2026-08-15T17:18:50.200107Z","submitted_at":"2019-12-22T12:49:12Z","title":"Primordial black holes and gravitational waves from parametric amplification of curvature perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.10437","snapshot_observed_at":"2026-08-15T20:02:43.755794Z","title":"Cai, Z.-K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.755794Z"},"links":{"cited_paper":"/paper/1912.10437","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:e7aa1bb1abb3b0cb3b28bd00c1e4fcdf904d227cdcad76c82540856d8da61fdf","observation_id":"b1275a01-08b3-4e19-9d70-6b93a6d3963e","resolution":{"observed_at":"2026-08-15T20:02:43.755794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02576","last_updated":"2017-05-06T16:26:20Z","snapshot_observed_at":"2026-08-14T21:13:00.935202Z","submitted_at":"2017-03-07T20:19:39Z","title":"A review of gravitational waves from cosmic domain walls","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02576","snapshot_observed_at":"2026-08-15T20:02:43.773141Z","title":"Saikawa, Universe 3, 40 (2017), arXiv:1703.02576 [hep-ph]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.773141Z"},"links":{"cited_paper":"/paper/1703.02576","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:6ff41528ab872039b678a9ee20b093661b2715f0bbff9d811af42f861aaa7e2e","observation_id":"3a551cab-6db8-4864-9b27-3db8be0ef541","resolution":{"observed_at":"2026-08-15T20:02:43.773141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.4476","last_updated":"2008-07-04T17:45:41Z","snapshot_observed_at":"2026-08-15T10:16:40.957234Z","submitted_at":"2008-04-28T20:05:44Z","title":"The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.4476","snapshot_observed_at":"2026-08-15T20:02:43.786156Z","title":"Sesana, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.786156Z"},"links":{"cited_paper":"/paper/0804.4476","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:2e5938849eab542c5f2b9b5a3690831cfb36364585f8a7d4dde6f345763611ac","observation_id":"1197ff30-c193-4f5f-b086-d14dd875c926","resolution":{"observed_at":"2026-08-15T20:02:43.786156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.00127","last_updated":"2014-12-31T12:53:40Z","snapshot_observed_at":"2026-08-14T23:05:36.005846Z","submitted_at":"2014-12-31T12:53:40Z","title":"Gravitational wave astronomy with the SKA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.00127","snapshot_observed_at":"2026-08-15T20:02:43.792752Z","title":"Janssen et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.792752Z"},"links":{"cited_paper":"/paper/1501.00127","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:437ed9ddd647d2c4a53242d93fb10b51430a13d3cdc46d91d7a9f73e2ec23acb","observation_id":"0cda139f-421e-4f95-8992-ccbd535b2bf5","resolution":{"observed_at":"2026-08-15T20:02:43.792752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.03600","last_updated":"2023-05-08T20:30:48Z","snapshot_observed_at":"2026-08-14T09:24:44.014319Z","submitted_at":"2023-01-09T19:00:00Z","title":"Inflation and Primordial Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.03600","snapshot_observed_at":"2026-08-15T20:02:43.800884Z","title":"¨Ozsoy and G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.800884Z"},"links":{"cited_paper":"/paper/2301.03600","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:355ca105ee312f25d45659dabf6f24dd010ccfa6b9f76ce5dc2a6f7cfb212244","observation_id":"161c21a3-8171-4651-89f2-c545edc68a90","resolution":{"observed_at":"2026-08-15T20:02:43.800884Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-15T20:02:43.808908Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.808908Z"},"links":{"citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:918b262885cb35a2ed81492348cd011274d05dd1759e4d0ade8d5297cca52efd","observation_id":"242c673f-c509-42cc-9fd7-d7397bddf079","resolution":{"observed_at":"2026-08-15T20:02:43.808908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.08577","last_updated":"2018-06-29T02:30:22Z","snapshot_observed_at":"2026-08-14T23:23:47.705346Z","submitted_at":"2018-04-23T17:16:37Z","title":"Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.08577","snapshot_observed_at":"2026-08-15T20:02:43.824285Z","title":"Kohri and T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.824285Z"},"links":{"cited_paper":"/paper/1804.08577","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:a0a1b7fc11cce4e868dac2429c6e93279592a9149269b75a5e74bbe7cbc9aa1a","observation_id":"7423a6c3-b559-410c-a274-9b61dc561164","resolution":{"observed_at":"2026-08-15T20:02:43.824285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.07732","last_updated":"2019-05-23T16:09:36Z","snapshot_observed_at":"2026-08-14T19:23:45.504743Z","submitted_at":"2018-04-20T17:13:45Z","title":"A Cosmological Signature of the SM Higgs Instability: Gravitational Waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.07732","snapshot_observed_at":"2026-08-15T20:02:43.835527Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.835527Z"},"links":{"cited_paper":"/paper/1804.07732","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:0d88bd2087d24ad0688dddeff0c2848768a3cd21180dbf9e388d22c05201b8da","observation_id":"7a0281e0-cd69-4444-a831-843c48607ea0","resolution":{"observed_at":"2026-08-15T20:02:43.835527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.13171","last_updated":"2023-03-27T16:34:49Z","snapshot_observed_at":"2026-08-16T05:54:11.932612Z","submitted_at":"2023-01-30T18:41:30Z","title":"Lensing constraints on ultradense dark matter halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.13171","snapshot_observed_at":"2026-08-15T20:02:43.842318Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.842318Z"},"links":{"cited_paper":"/paper/2301.13171","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:04690e774a286db6097a78d636d0d64b712b68765046de9e2c33f05595124dd3","observation_id":"18eee497-5ed5-43a5-b6ea-655f94637b3d","resolution":{"observed_at":"2026-08-15T20:02:43.842318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.04904","last_updated":"2023-01-31T07:43:17Z","snapshot_observed_at":"2026-08-14T08:25:03.366429Z","submitted_at":"2022-10-10T18:00:00Z","title":"Ultradense dark matter haloes accompany primordial black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.04904","snapshot_observed_at":"2026-08-15T20:02:43.850975Z","title":"Sten Delos and J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.850975Z"},"links":{"cited_paper":"/paper/2210.04904","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:83ece9e03e11d0fc1bd8edc435889ef562baaac89e094561892bdd7290e96dff","observation_id":"edf0a23b-a3b6-43d2-b20b-994fec2b8a96","resolution":{"observed_at":"2026-08-15T20:02:43.850975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.4615","last_updated":"2010-10-21T14:55:44Z","snapshot_observed_at":"2026-08-15T09:04:40.426854Z","submitted_at":"2010-06-23T19:04:29Z","title":"On Features and Nongaussianity from Inflationary Particle Production","version":2},"cited_work":{"arxiv_id":"1006.4615","doi":null,"metadata_source":"pith","pith_arxiv_id":"1006.4615","snapshot_observed_at":"2026-08-15T20:02:44.623669Z","title":"On Features and Nongaussianity from Inflationary Particle Production","venue":"astro-ph.CO","work_id":"cfdb2c99-0b1d-4bca-84b0-831476eb2007","year":2010},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.867098Z"},"links":{"cited_paper":"/paper/1006.4615","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:f528708b2184c5c4439255468b336b7508e737c87639358d640f9ec9ce2db89c","observation_id":"e6ebc178-7491-492c-8c9c-d789936c38ff","resolution":{"observed_at":"2026-08-15T20:02:44.653707Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.03422","last_updated":"2021-10-21T06:52:02Z","snapshot_observed_at":"2026-08-14T19:10:43.815417Z","submitted_at":"2021-08-07T10:52:48Z","title":"Primordial black holes and stochastic gravitational wave background from inflation with a noncanonical spectator field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.03422","snapshot_observed_at":"2026-08-15T20:02:43.877803Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-15T20:02:43.877803Z"},"links":{"cited_paper":"/paper/2108.03422","citing_paper":"/paper/2506.14366"},"observation_digest":"sha256:b04379cdd2322b8924c64a6e0f7ea0b52e8d7981caf37dee8957ca1d26770e5c","observation_id":"e31e6f69-e668-4363-b100-6a385620fbcd","resolution":{"observed_at":"2026-08-15T20:02:43.877803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.14366","last_updated":"2025-06-17T10:07:51Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T00:07:41.417251Z","submitted_at":"2025-06-17T10:07:51Z","title":"The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":96,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":113},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 113 outbound references and 1 inbound Pith citation observation for arXiv:2506.14366."}