{"as_of":"2026-08-14T17:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d9761d3bf563df841c2f34469f01f516290c01dfeb73e8005495b303d514aa67","coverage":[{"denominator":87,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":87,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:42:58.268186Z","state":"measured"},{"denominator":87,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":87,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2608.08490/citation-record","integrity":"/paper/2608.08490/integrity","json":"/paper/2608.08490/citation-record.json","paper":"/paper/2608.08490"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:42:57.842316Z","title":"Brans and R","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.842316Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:a723b654d67d323ace20051be128bd5496ddad9ff15859b8dc906749460e6f96","observation_id":"cea8568c-5117-4115-868b-3af132a27484","resolution":{"observed_at":"2026-08-14T04:42:57.842316Z","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":"2026-08-14T04:42:57.847686Z","title":"Damour and G","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.847686Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:888b2b6eb1829c42939665bdab147cb0ff68df58ddbd23b9f868501cb0da87e0","observation_id":"f807e2ff-d71c-4033-ac9b-d234d769e7e4","resolution":{"observed_at":"2026-08-14T04:42:57.847686Z","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":"2026-08-14T04:42:57.852703Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.852703Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:dd216620c88bdc8e7e50b09f321bb97368e959ecfd19e94ed2427600b2ad8094","observation_id":"a18e6fd5-b091-4737-9e85-04f80400f2e8","resolution":{"observed_at":"2026-08-14T04:42:57.852703Z","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":"2026-08-14T04:42:57.857807Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.857807Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:0c14351a5488b9b3d1d30d7911a135e14eed347d758d49df7acd531ace1a8a9d","observation_id":"1a5eb764-3c59-4122-a06b-1aba24a7c448","resolution":{"observed_at":"2026-08-14T04:42:57.857807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0007031","last_updated":"2001-06-02T01:29:20Z","snapshot_observed_at":"2026-08-06T06:48:17.122588Z","submitted_at":"2000-07-14T18:56:24Z","title":"Gravity with a dynamical preferred frame","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0007031","snapshot_observed_at":"2026-08-14T04:42:57.862353Z","title":"Jacobson and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.862353Z"},"links":{"cited_paper":"/paper/gr-qc/0007031","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:b995a151576cba4c4ece11217fe2f0979127f7f7f6671642ed966bae7d0e2ff0","observation_id":"fdcb7ede-2b09-4839-9d35-a22ffae9214b","resolution":{"observed_at":"2026-08-14T04:42:57.862353Z","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":"2026-08-14T04:42:57.867435Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.867435Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:382a5e766663f768965e891b0cac85fa9ca8add0aa44898f969cdb54f46e07e2","observation_id":"f86c3e7e-eb1a-4bcf-8a3d-7f0bb1ec0a19","resolution":{"observed_at":"2026-08-14T04:42:57.867435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.01899","last_updated":"2018-05-13T02:41:02Z","snapshot_observed_at":"2026-07-06T05:36:49.981924Z","submitted_at":"2017-04-06T15:53:29Z","title":"Polarizations of Gravitational Waves in Horndeski Theory","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.01899","snapshot_observed_at":"2026-08-14T04:42:57.872742Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.872742Z"},"links":{"cited_paper":"/paper/1704.01899","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:89b52b612d6a5f984366c130c53260db20b4ebe3c12d76cb1dc835c36bce381c","observation_id":"57e9cc8a-d0b1-4a2f-944a-71aa0751395f","resolution":{"observed_at":"2026-08-14T04:42:57.872742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.05998","last_updated":"2017-05-14T03:09:29Z","snapshot_observed_at":"2026-07-06T05:27:00.857087Z","submitted_at":"2017-01-21T08:49:58Z","title":"Polarizations of gravitational waves in $f(R)$ gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.05998","snapshot_observed_at":"2026-08-14T04:42:57.877763Z","title":"Liang, Y","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.877763Z"},"links":{"cited_paper":"/paper/1701.05998","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:680952a8d427691055bb04d9852e2faba93e9718355f22cc3648be5cf6db2581","observation_id":"624f09f0-53fb-490f-864a-f3c619d758b5","resolution":{"observed_at":"2026-08-14T04:42:57.877763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.03382","last_updated":"2018-04-15T13:21:49Z","snapshot_observed_at":"2026-07-06T06:18:02.744267Z","submitted_at":"2018-01-10T14:08:36Z","title":"Gravitational waves in Einstein-{\\ae}ther and generalized TeVeS theory after GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.03382","snapshot_observed_at":"2026-08-14T04:42:57.882495Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.882495Z"},"links":{"cited_paper":"/paper/1801.03382","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:9c0f2f17195d5a1676a4751c0eea5aebbc13d44d14320c47aa8200a628e23f57","observation_id":"3ad00b08-5710-4db0-a449-4461158c96f3","resolution":{"observed_at":"2026-08-14T04:42:57.882495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.11336","last_updated":"2024-02-20T10:40:44Z","snapshot_observed_at":"2026-08-13T05:47:31.905763Z","submitted_at":"2023-10-17T15:14:36Z","title":"Polarization modes of gravitational waves in general modified gravity: General metric theory and general scalar-tensor theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.11336","snapshot_observed_at":"2026-08-14T04:42:57.887256Z","title":"Dong, Y.-Q","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.887256Z"},"links":{"cited_paper":"/paper/2310.11336","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:d833ee332c424bebb44a469163dfaf28611621b72d019087379332eec2ffd26b","observation_id":"3baa25f3-b948-4366-bdd9-b7e87e6b41bf","resolution":{"observed_at":"2026-08-14T04:42:57.887256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.20577","last_updated":"2025-01-03T02:47:34Z","snapshot_observed_at":"2026-08-13T12:27:23.674697Z","submitted_at":"2024-05-31T02:10:28Z","title":"Polarization modes of gravitational waves in general Einstein-vector theory","version":2},"cited_work":{"arxiv_id":"2405.20577","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.20577","snapshot_observed_at":"2026-08-14T04:42:59.786923Z","title":"Polarization modes of gravitational waves in general Einstein-vector theory","venue":"gr-qc","work_id":"603e2cdd-696e-4725-95d8-e26710bbb939","year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.891876Z"},"links":{"cited_paper":"/paper/2405.20577","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:e0c77b202ec3e5ac78552041a812bd7bade23f584ef8c4b87dd748f1939e2b39","observation_id":"d3c642ee-77af-4b6c-967d-9c2cfd62ae72","resolution":{"observed_at":"2026-08-14T04:42:59.792172Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:42:57.896605Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.896605Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4f5e250abf24b5d81c8b59351c1b26916bf42cc8a48478bfd9e9dbce0f9f6d4a","observation_id":"4c69a105-b74f-4aef-b6bc-a3c1a70d7694","resolution":{"observed_at":"2026-08-14T04:42:57.896605Z","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":"2026-08-14T04:42:57.900815Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.900815Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:334776ab944a7b6f82ba423c0d9988ab4196cedd8bdf42a871cf8cfa834678f7","observation_id":"de0e970d-41b7-45b5-90ba-2009c8693418","resolution":{"observed_at":"2026-08-14T04:42:57.900815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.7377","last_updated":"2014-03-28T14:04:31Z","snapshot_observed_at":"2026-08-12T13:37:17.409976Z","submitted_at":"2014-03-28T14:04:31Z","title":"The Confrontation between General Relativity and Experiment","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.7377","snapshot_observed_at":"2026-08-14T04:42:57.905125Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.905125Z"},"links":{"cited_paper":"/paper/1403.7377","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:625e0474ab009fd3b06ab7cf16db18e09c90a86ace009661c23e0b3810e6d104","observation_id":"b40bc7d6-9e52-41da-b691-41770f364845","resolution":{"observed_at":"2026-08-14T04:42:57.905125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.08373","last_updated":"2017-10-18T17:22:09Z","snapshot_observed_at":"2026-08-05T11:57:55.500725Z","submitted_at":"2017-04-26T22:55:16Z","title":"Polarization-based Tests of Gravity with the Stochastic Gravitational-Wave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.08373","snapshot_observed_at":"2026-08-14T04:42:57.909856Z","title":"Callister, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.909856Z"},"links":{"cited_paper":"/paper/1704.08373","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:e8dd50902c2d9317ba0f40e6bce1110902837a68c6d4cfa8fb59f8cc80e148c9","observation_id":"1634a4a3-e99f-4862-9340-6216c8b653dc","resolution":{"observed_at":"2026-08-14T04:42:57.909856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.0528","last_updated":"2009-04-17T10:26:06Z","snapshot_observed_at":"2026-08-10T08:55:02.912703Z","submitted_at":"2009-03-03T13:25:10Z","title":"Probing non-tensorial polarizations of stochastic gravitational-wave backgrounds with ground-based laser interferometers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0903.0528","snapshot_observed_at":"2026-08-14T04:42:57.915022Z","title":"Nishizawa, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.915022Z"},"links":{"cited_paper":"/paper/0903.0528","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:dd032d6b593464b0f0a23c997d3e32c5ac02bfc56a859c2b84dfd5e85b302b6b","observation_id":"d6706a39-e7f4-4745-9020-4622eea36c1b","resolution":{"observed_at":"2026-08-14T04:42:57.915022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.10194","last_updated":"2019-10-02T16:30:52Z","snapshot_observed_at":"2026-08-02T08:19:59.341964Z","submitted_at":"2018-02-27T22:38:21Z","title":"A Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.10194","snapshot_observed_at":"2026-08-14T04:42:57.919778Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.919778Z"},"links":{"cited_paper":"/paper/1802.10194","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:bd4810ef6994c873388d1929be19d0478a352c5b9a98af1d90417d15dc672917","observation_id":"22d0dc12-27a3-4995-94f1-c0708ee65fc8","resolution":{"observed_at":"2026-08-14T04:42:57.919778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.02886","last_updated":"2019-09-06T13:09:31Z","snapshot_observed_at":"2026-08-14T17:05:57.456599Z","submitted_at":"2019-03-07T12:53:00Z","title":"Search for the isotropic stochastic background using data from Advanced LIGO's second observing run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.02886","snapshot_observed_at":"2026-08-14T04:42:57.924885Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.924885Z"},"links":{"cited_paper":"/paper/1903.02886","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:f420a879fd06cdb180f70e743863d0118a2b83cda8a53941af08840acdb396bc","observation_id":"e0a2eb13-624a-42d1-b394-9ef554003549","resolution":{"observed_at":"2026-08-14T04:42:57.924885Z","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":"2026-08-14T04:42:57.929795Z","title":"Abbottet al.(LIGO Scientific, Virgo, KAGRA), Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run, (2021), arXiv:2101.12248 [gr-qc]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.929795Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:f0a80d11d31d6d408f38ea38e87d533c9b5b053b51bb1578c997e86e497e78d3","observation_id":"b76e72fd-c060-43a5-8584-b6932a996ae7","resolution":{"observed_at":"2026-08-14T04:42:57.929795Z","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":"2026-08-14T04:42:57.934449Z","title":"Abbottet al.(KAGRA, Virgo, LIGO Scientific), Upper limits on the isotropic gravitational-wave back- ground from Advanced LIGO and Advanced Virgo’s third observing run, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.934449Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:579980cf9fd6a9db395dedeca0b5b5ead677682b1c7beaf511ab33f903eb5a0e","observation_id":"ba2617d4-b2d5-400b-b700-373ffdb0af50","resolution":{"observed_at":"2026-08-14T04:42:57.934449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.20721","last_updated":"2025-08-28T12:44:13Z","snapshot_observed_at":"2026-08-07T10:34:29.047427Z","submitted_at":"2025-08-28T12:44:13Z","title":"Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2508.20721","snapshot_observed_at":"2026-08-14T04:42:57.939160Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.939160Z"},"links":{"cited_paper":"/paper/2508.20721","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:59e0a0e5e4e739cfc35dc202297722ea75f62123e79db7036edc4a5c9b83713d","observation_id":"4fd03767-0ecc-468c-9ba5-df33ae99b89a","resolution":{"observed_at":"2026-08-14T04:42:57.939160Z","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":"2026-08-14T04:42:57.943982Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.943982Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:555454da77ad1bfbdf1c3ef224d0ed5f50feada019986efdd6b85ccab630bd5f","observation_id":"95e969b4-c44d-4383-bdab-ad849bb6c2a9","resolution":{"observed_at":"2026-08-14T04:42:57.943982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09660","last_updated":"2017-10-13T09:37:56Z","snapshot_observed_at":"2026-08-14T14:22:38.692929Z","submitted_at":"2017-09-27T19:11:34Z","title":"GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09660","snapshot_observed_at":"2026-08-14T04:42:57.949107Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.949107Z"},"links":{"cited_paper":"/paper/1709.09660","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:44f0fc695f8539f4578f87e4f4c2f51467cf50bacb91040398df74a39f860370","observation_id":"072ea154-ce62-42eb-98ba-186e7d3d1e21","resolution":{"observed_at":"2026-08-14T04:42:57.949107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02182","last_updated":"2018-06-04T18:00:17Z","snapshot_observed_at":"2026-08-14T08:09:13.736937Z","submitted_at":"2018-06-04T18:00:17Z","title":"Polarization test of gravitational waves from compact binary coalescences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02182","snapshot_observed_at":"2026-08-14T04:42:57.954537Z","title":"Takeda, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.954537Z"},"links":{"cited_paper":"/paper/1806.02182","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:53cce7a2ac24de5e87300cd5d78050faa69028f662d675f4645c69307440de51","observation_id":"98307718-f512-4eb6-9886-f90087f8e4b4","resolution":{"observed_at":"2026-08-14T04:42:57.954537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06861","last_updated":"2025-11-17T15:05:31Z","snapshot_observed_at":"2026-08-13T03:46:51.301529Z","submitted_at":"2021-12-13T18:19:04Z","title":"Tests of General Relativity with GWTC-3","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06861","snapshot_observed_at":"2026-08-14T04:42:57.959441Z","title":"Abbottet al.(LIGO Scientific, VIRGO, KAGRA), Tests of General Relativity with GWTC-3, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.959441Z"},"links":{"cited_paper":"/paper/2112.06861","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:85de53b5dbd4d6b2a12749a119719e6fd83eaafb71e0c5cb837df8bf45b106c3","observation_id":"63d7253b-a5ce-4185-a0b0-334e8bff4146","resolution":{"observed_at":"2026-08-14T04:42:57.959441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.19019","last_updated":"2026-03-19T15:22:26Z","snapshot_observed_at":"2026-07-06T22:49:42.664225Z","submitted_at":"2026-03-19T15:22:26Z","title":"GWTC-4.0: Tests of General Relativity. I. Overview and General Tests","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.19019","snapshot_observed_at":"2026-08-14T04:42:57.964515Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.964515Z"},"links":{"cited_paper":"/paper/2603.19019","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:ed7d2d6eaa2dfcfc9aed38c69ebb487a75b2888a72547e49862e9309aeec56dd","observation_id":"9840719f-49c9-4176-bc06-3e50c92b6960","resolution":{"observed_at":"2026-08-14T04:42:57.964515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.19020","last_updated":"2026-07-20T22:42:43Z","snapshot_observed_at":"2026-08-13T00:04:52.074572Z","submitted_at":"2026-03-19T15:22:27Z","title":"GWTC-4.0: Tests of General Relativity. II. Parameterized Tests","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.19020","snapshot_observed_at":"2026-08-14T04:42:57.969803Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.969803Z"},"links":{"cited_paper":"/paper/2603.19020","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:8fe0d75b3218f60416e6b7ef972945487c598ed9a144049b4d65d916e0c6132d","observation_id":"1934de09-7b30-4d31-a626-6e549d672cb9","resolution":{"observed_at":"2026-08-14T04:42:57.969803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.11128","last_updated":"2020-03-24T22:00:39Z","snapshot_observed_at":"2026-07-06T09:07:06.825963Z","submitted_at":"2020-03-24T22:00:39Z","title":"Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background","version":1},"cited_work":{"arxiv_id":"2003.11128","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.11128","snapshot_observed_at":"2026-08-14T04:42:59.403620Z","title":"Parameter Estimation for Tests of General Relativity with the Astrophysical Stochastic Gravitational Wave Background","venue":"gr-qc","work_id":"42072dd7-6287-4cb0-ad4b-e0ae87c9d0fa","year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.974281Z"},"links":{"cited_paper":"/paper/2003.11128","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4098bc7ced328d3f6bb7734b0d390b725e139c67838b084e19a55154acebac95","observation_id":"7b409c84-cb2d-4aa5-85b8-9b796ca9c8c6","resolution":{"observed_at":"2026-08-14T04:42:59.408679Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12138","last_updated":"2023-10-18T17:49:33Z","snapshot_observed_at":"2026-08-14T15:47:16.745127Z","submitted_at":"2023-10-18T17:49:33Z","title":"The NANOGrav 15-year data set: Search for Transverse Polarization Modes in the Gravitational-Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.12138","snapshot_observed_at":"2026-08-14T04:42:57.979138Z","title":"Agazieet al.(NANOGrav), The NANOGrav 15 yr Data Set: Search for Transverse Polarization Modes in the Gravitational-wave Background, Astrophys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.979138Z"},"links":{"cited_paper":"/paper/2310.12138","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:9a1e954effe6dff90a45e2ebfabb063ee52c7047d9b61b4e90a0f90412438af6","observation_id":"d535a055-6727-4e2c-948b-e515dd3e78df","resolution":{"observed_at":"2026-08-14T04:42:57.979138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.06869","last_updated":"2021-10-04T11:58:04Z","snapshot_observed_at":"2026-08-13T20:29:21.016744Z","submitted_at":"2021-01-18T04:44:09Z","title":"Non-tensorial Gravitational Wave Background in NANOGrav 12.5-Year Data Set","version":2},"cited_work":{"arxiv_id":"2101.06869","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.06869","snapshot_observed_at":"2026-08-14T04:42:59.367053Z","title":"Non-tensorial Gravitational Wave Background in NANOGrav 12.5-Year Data Set","venue":"astro-ph.CO","work_id":"3e37c319-042f-4eb6-b9c4-b5e909037ca2","year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.983839Z"},"links":{"cited_paper":"/paper/2101.06869","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:84a6bf719aeaaf102657b1d1d4f0f6615d50f1377d395ad7862eb2ee5f827aff","observation_id":"6a201a0d-868c-44d9-a922-6f25f54acae5","resolution":{"observed_at":"2026-08-14T04:42:59.372120Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.11238","last_updated":"2024-05-06T13:50:12Z","snapshot_observed_at":"2026-08-13T05:47:37.946893Z","submitted_at":"2023-10-17T13:08:21Z","title":"Search for Non-Tensorial Gravitational-Wave Backgrounds in the NANOGrav 15-Year Data Set","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.11238","snapshot_observed_at":"2026-08-14T04:42:57.988790Z","title":"Chen, Y.-M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.988790Z"},"links":{"cited_paper":"/paper/2310.11238","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:322a6d41e21386208185b84bd94581602f01099a884cfa52c2b5ba68d9d14a88","observation_id":"c45ce06b-f24b-4454-8e8f-61b4785c2fc2","resolution":{"observed_at":"2026-08-14T04:42:57.988790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00786","last_updated":"2017-02-23T05:33:01Z","snapshot_observed_at":"2026-08-11T09:09:15.127132Z","submitted_at":"2017-02-02T07:06:53Z","title":"Laser Interferometer Space Antenna","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00786","snapshot_observed_at":"2026-08-14T04:42:57.993909Z","title":"Amaro-Seoaneet al.(LISA), Laser Interferometer Space Antenna, (2017), arXiv:1702.00786 [astro-ph.IM]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.993909Z"},"links":{"cited_paper":"/paper/1702.00786","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:1737dd01d9474f57bbd8d8786b008a2424b06233f3cbe2e0e97bc438d0231f0b","observation_id":"2f0edba1-cc97-4c7a-9552-9cc59aab3789","resolution":{"observed_at":"2026-08-14T04:42:57.993909Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07571","last_updated":"2024-02-12T11:06:12Z","snapshot_observed_at":"2026-08-02T13:54:50.876049Z","submitted_at":"2024-02-12T11:06:12Z","title":"LISA Definition Study Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07571","snapshot_observed_at":"2026-08-14T04:42:57.999193Z","title":"Colpiet al.(LISA), LISA Definition Study Report, (2024), arXiv:2402.07571 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:57.999193Z"},"links":{"cited_paper":"/paper/2402.07571","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:26f8bd9763f79bbd880099978239b66a2e3696a851c0b85d10a682ec6a0f36e9","observation_id":"dc39f21a-ed3f-4332-8ff0-8dd87b21e5e7","resolution":{"observed_at":"2026-08-14T04:42:57.999193Z","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":"2026-08-14T04:42:58.004114Z","title":"Hu and Y.-L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.004114Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:f639e39e2d958b03523664f519766547d3f463c826b2c33ba632d4acd61a43ce","observation_id":"c7446e11-7fc9-4643-8ff4-03fe869f6c26","resolution":{"observed_at":"2026-08-14T04:42:58.004114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.02076","last_updated":"2015-12-07T14:57:50Z","snapshot_observed_at":"2026-08-05T11:59:29.671184Z","submitted_at":"2015-12-07T14:57:50Z","title":"TianQin: a space-borne gravitational wave detector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.02076","snapshot_observed_at":"2026-08-14T04:42:58.008845Z","title":"Luoet al.(TianQin), TianQin: a space-borne gravi- tational wave detector, Class","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.008845Z"},"links":{"cited_paper":"/paper/1512.02076","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:d8c7e55d6416a2bff0e16511be1e1a6317fb31def72abadb9c86b5f95be2669c","observation_id":"58ab452a-6010-4b0a-bc4d-8e494c3cb201","resolution":{"observed_at":"2026-08-14T04:42:58.008845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.03603","last_updated":"2020-02-10T08:43:08Z","snapshot_observed_at":"2026-08-13T08:03:21.030900Z","submitted_at":"2020-02-10T08:43:08Z","title":"The LISA-Taiji network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.03603","snapshot_observed_at":"2026-08-14T04:42:58.014066Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.014066Z"},"links":{"cited_paper":"/paper/2002.03603","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4fde6620ba0ec8781fa8db29c95e344257b821286b121f2f6891a2aa0bb5542e","observation_id":"ffd9e00f-8117-4e92-afe7-6bbc3713ea83","resolution":{"observed_at":"2026-08-14T04:42:58.014066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.12628","last_updated":"2020-07-10T05:33:08Z","snapshot_observed_at":"2026-08-08T10:40:17.414932Z","submitted_at":"2020-02-28T10:12:58Z","title":"Numerical simulation of sky localization for LISA-TAIJI joint observation","version":2},"cited_work":{"arxiv_id":"2002.12628","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.12628","snapshot_observed_at":"2026-08-14T04:42:59.271555Z","title":"Numerical simulation of sky localization for LISA-TAIJI joint observation","venue":"gr-qc","work_id":"be7fd562-e016-4864-8a20-fa2854a284d4","year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.019565Z"},"links":{"cited_paper":"/paper/2002.12628","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:3c7b8253b1c3eb348343a072706440cd53eaac5a19ebf490325cce4bea2e897b","observation_id":"ca59eb1a-06e0-45a9-814d-c5f9d645c488","resolution":{"observed_at":"2026-08-14T04:42:59.276598Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.01991","last_updated":"2021-02-16T02:59:33Z","snapshot_observed_at":"2026-08-05T04:34:26.392803Z","submitted_at":"2021-01-06T12:28:46Z","title":"Observing gravitational wave polarizations with LISA-TAIJI network","version":2},"cited_work":{"arxiv_id":"2101.01991","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.01991","snapshot_observed_at":"2026-08-14T04:42:59.250757Z","title":"Observing gravitational wave polarizations with LISA-TAIJI network","venue":"gr-qc","work_id":"3e271b9c-ef8d-4628-9a6b-18c7b2c6cffe","year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.025520Z"},"links":{"cited_paper":"/paper/2101.01991","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:eea0ce4aecca115d79c802ebcdc03063be7aeb9ca194743b2effcfe9062abd00","observation_id":"56331d09-f805-4747-afdf-adefb56461c9","resolution":{"observed_at":"2026-08-14T04:42:59.256195Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.02943","last_updated":"2021-05-17T16:16:28Z","snapshot_observed_at":"2026-08-13T19:27:28.522221Z","submitted_at":"2021-05-06T20:41:56Z","title":"Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks","version":2},"cited_work":{"arxiv_id":"2105.02943","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.02943","snapshot_observed_at":"2026-08-14T04:42:59.229037Z","title":"Massive Black Hole Binaries and Where to Find Them with Dual Detector Networks","venue":"gr-qc","work_id":"a9d9a564-ea65-42e4-b446-4d0fab619975","year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.031867Z"},"links":{"cited_paper":"/paper/2105.02943","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:f3d1424ee8dd2849929dad2b1f2a302875f43e8e66d7f60fda3722e4ec92ef4a","observation_id":"200a8a74-ea55-448f-be25-8e4c6850e4b9","resolution":{"observed_at":"2026-08-14T04:42:59.234194Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.00771","last_updated":"2020-10-02T04:20:59Z","snapshot_observed_at":"2026-08-09T17:06:20.607845Z","submitted_at":"2020-10-02T04:20:59Z","title":"Searching anomalous polarization modes of stochastic gravitational wave background with LISA and Taiji","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.00771","snapshot_observed_at":"2026-08-14T04:42:58.037015Z","title":"Omiya and N","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.037015Z"},"links":{"cited_paper":"/paper/2010.00771","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:57339fe49c2999d16357944ca25a1341f182f8a14581a3cbd928636df997493f","observation_id":"ac4d85b5-a622-45ce-be0c-ea3d5e9dc34d","resolution":{"observed_at":"2026-08-14T04:42:58.037015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.06877","last_updated":"2020-11-25T04:47:22Z","snapshot_observed_at":"2026-08-05T11:24:59.893990Z","submitted_at":"2020-10-14T08:41:22Z","title":"Gravitational Wave Background Search by Correlating Multiple Triangular Detectors in the mHz Band","version":2},"cited_work":{"arxiv_id":"2010.06877","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.06877","snapshot_observed_at":"2026-08-14T04:42:59.191379Z","title":"Gravitational Wave Background Search by Correlating Multiple Triangular Detectors in the mHz Band","venue":"gr-qc","work_id":"eba4d87e-dc95-4a5e-b023-30e44d2eb403","year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.042115Z"},"links":{"cited_paper":"/paper/2010.06877","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:cc764b47ad0a9a8d99c6ed268a39925979fe95b9ccc9f5baa37a1f55e3045b43","observation_id":"73e69258-c81f-415b-89a3-8f537e47b675","resolution":{"observed_at":"2026-08-14T04:42:59.196584Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.07059","last_updated":"2021-04-01T09:37:08Z","snapshot_observed_at":"2026-08-07T21:01:32.434295Z","submitted_at":"2020-11-13T18:56:09Z","title":"Measuring Parity Violation in the Stochastic Gravitational Wave Background with the LISA-Taiji network","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.07059","snapshot_observed_at":"2026-08-14T04:42:58.047089Z","title":"Orlando, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.047089Z"},"links":{"cited_paper":"/paper/2011.07059","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:f60d811663b9d23d75392dc8370dd357e45bc3f2c5afdf36421037225c04cb78","observation_id":"0568e370-1943-40f5-9be6-4bd4f826a34e","resolution":{"observed_at":"2026-08-14T04:42:58.047089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.05356","last_updated":"2022-04-05T00:11:01Z","snapshot_observed_at":"2026-08-13T18:47:43.935512Z","submitted_at":"2021-07-12T12:24:23Z","title":"Polarization of gravitational waves from helical MHD turbulent sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.05356","snapshot_observed_at":"2026-08-14T04:42:58.051872Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.051872Z"},"links":{"cited_paper":"/paper/2107.05356","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:84f47066c2af6e18ac7fd098e95dd623cfb35b37043329fc59e5faf0a5751927","observation_id":"96b51945-a95d-43da-b668-b467c93366ba","resolution":{"observed_at":"2026-08-14T04:42:58.051872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.09380","last_updated":"2024-09-13T08:03:39Z","snapshot_observed_at":"2026-08-12T23:23:18.419597Z","submitted_at":"2024-07-12T15:59:55Z","title":"Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.09380","snapshot_observed_at":"2026-08-14T04:42:58.056522Z","title":"Zhao and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.056522Z"},"links":{"cited_paper":"/paper/2407.09380","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:8a31e9bda71aabeeab59d41d736b2339d85ddde584a740318019fd8916cbeb3b","observation_id":"6f75cfae-47e9-42d9-9e73-e06c007b022e","resolution":{"observed_at":"2026-08-14T04:42:58.056522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11882","last_updated":"2021-06-17T09:07:20Z","snapshot_observed_at":"2026-08-13T04:52:43.917323Z","submitted_at":"2021-01-28T09:22:53Z","title":"Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11882","snapshot_observed_at":"2026-08-14T04:42:58.061153Z","title":"Wang, S.-J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.061153Z"},"links":{"cited_paper":"/paper/2101.11882","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4e168dbc5cbd1a4992c3d33abb97f0ba9ab406f44aa3ee2e9600830c63c2b934","observation_id":"cbc449d0-9ce5-4852-a38c-635e4572c79a","resolution":{"observed_at":"2026-08-14T04:42:58.061153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14732","last_updated":"2021-06-01T01:11:13Z","snapshot_observed_at":"2026-08-11T09:27:17.847438Z","submitted_at":"2020-10-28T03:47:39Z","title":"Hubble parameter estimation via dark sirens with the LISA-Taiji network","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14732","snapshot_observed_at":"2026-08-14T04:42:58.065991Z","title":"Wang, W.-H","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.065991Z"},"links":{"cited_paper":"/paper/2010.14732","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:e3a5aaeb5c18bede8ba4a06f728a995d27c1490abd25587f419586fef506132d","observation_id":"100e1f02-ed91-449d-9aaa-53e4e0f4538a","resolution":{"observed_at":"2026-08-14T04:42:58.065991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.00746","last_updated":"2021-05-11T11:05:44Z","snapshot_observed_at":"2026-07-06T11:05:42.032726Z","submitted_at":"2021-05-03T10:46:33Z","title":"Alternative LISA-TAIJI networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.00746","snapshot_observed_at":"2026-08-14T04:42:58.070690Z","title":"Wang, W.-T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.070690Z"},"links":{"cited_paper":"/paper/2105.00746","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:37af9a377b70435afcc1d5a58c5b38a7381430c6b96ad6a549428936a7867ff0","observation_id":"8472245c-cfa2-4a6b-b119-1e9589837235","resolution":{"observed_at":"2026-08-14T04:42:58.070690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.11151","last_updated":"2021-11-08T13:32:05Z","snapshot_observed_at":"2026-07-06T11:41:22.176602Z","submitted_at":"2021-08-25T10:13:03Z","title":"Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.11151","snapshot_observed_at":"2026-08-14T04:42:58.075795Z","title":"Wang and W.-B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.075795Z"},"links":{"cited_paper":"/paper/2108.11151","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:95e170c59d2ee7a50ee50a751af459b8c60b5defc2a612d0817087dd185d82d5","observation_id":"e14194c3-ab05-4486-9da6-eae0bcbcd651","resolution":{"observed_at":"2026-08-14T04:42:58.075795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.18420","last_updated":"2025-04-25T11:43:48Z","snapshot_observed_at":"2026-08-14T15:14:13.075918Z","submitted_at":"2024-12-24T13:24:13Z","title":"Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.18420","snapshot_observed_at":"2026-08-14T04:42:58.080371Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.080371Z"},"links":{"cited_paper":"/paper/2412.18420","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:2234029a39dea79576bceaa5a8c5f264dda881849b9d72401bff1e682d9a4334","observation_id":"befd8463-e910-47f9-bfcc-59efdef536ec","resolution":{"observed_at":"2026-08-14T04:42:58.080371Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.09238","last_updated":"2026-06-08T09:14:53Z","snapshot_observed_at":"2026-08-11T16:14:10.013118Z","submitted_at":"2026-06-08T09:14:53Z","title":"Detectability to extreme mass ratio inspirals with alternative space-based detector networks","version":1},"cited_work":{"arxiv_id":"2606.09238","doi":null,"metadata_source":"pith","pith_arxiv_id":"2606.09238","snapshot_observed_at":"2026-08-14T04:42:59.047233Z","title":"Detectability to extreme mass ratio inspirals with alternative space-based detector networks","venue":"gr-qc","work_id":"0442dfb5-5a09-4504-b1f2-65a7ebba7411","year":2026},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.085070Z"},"links":{"cited_paper":"/paper/2606.09238","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:559c677c76aaa80126ae899c7b24d66353e411243250f429f806fa8fa9a7b554","observation_id":"44e27dab-4f3b-49ff-9388-82c0371f1561","resolution":{"observed_at":"2026-08-14T04:42:59.052465Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3684","last_updated":"2012-09-12T20:35:14Z","snapshot_observed_at":"2026-08-06T03:33:30.927132Z","submitted_at":"2012-01-18T02:24:43Z","title":"Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3684","snapshot_observed_at":"2026-08-14T04:42:58.090076Z","title":"Vallisneri and C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.090076Z"},"links":{"cited_paper":"/paper/1201.3684","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:e4c4a8f7d0fd5fdfb9ce18fbd3f6854517be48dde887668e92ff3fbe735eff19","observation_id":"3b3b2794-6061-4069-acea-4c6f74fb9bc0","resolution":{"observed_at":"2026-08-14T04:42:58.090076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.06633","last_updated":"2022-09-01T07:54:11Z","snapshot_observed_at":"2026-08-13T16:02:44.635336Z","submitted_at":"2022-04-13T20:53:00Z","title":"Assessing the data-analysis impact of LISA orbit approximations using a GPU-accelerated response model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.06633","snapshot_observed_at":"2026-08-14T04:42:58.095529Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.095529Z"},"links":{"cited_paper":"/paper/2204.06633","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4b99c1c4860f54d42d4676c4164f76fad9cc55740042113aa932b069cb3f4fa0","observation_id":"f869962d-1344-474a-8c64-58374aa153d9","resolution":{"observed_at":"2026-08-14T04:42:58.095529Z","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":"2603.22377","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:42:58.982471Z","title":"Baghiet al., LISA science ground segment conven- tions, (2026), arXiv:2603.22377 [astro-ph.IM]","venue":null,"work_id":"0fb2f817-0c69-4ca6-b9ff-4b1f9555fe4d","year":2026},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.100713Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:2bfbd7778c2122697cfb98e419c3182b867951491dbfda04ba2221eb0e33b2fa","observation_id":"7f9b89c8-d996-4004-a330-978973a57dbc","resolution":{"observed_at":"2026-08-14T04:42:58.994344Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.18397","last_updated":"2026-06-05T05:49:36Z","snapshot_observed_at":"2026-08-09T20:43:47.638606Z","submitted_at":"2025-07-24T13:28:44Z","title":"Correlation and Data-Analysis Distinctiveness of Time-Delay Interferometry Configurations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.18397","snapshot_observed_at":"2026-08-14T04:42:58.105801Z","title":"Wang, Correlation and Data-Analysis Distinctiveness of Time-Delay Interferometry Configurations, (2025), arXiv:2507.18397 [gr-qc]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.105801Z"},"links":{"cited_paper":"/paper/2507.18397","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:7341d8d73e608da21d6ca418ff313986e1d48117335ffd4fb37d24b0cc2c19b6","observation_id":"69e994ff-031a-43ed-812a-c606759d03c9","resolution":{"observed_at":"2026-08-14T04:42:58.105801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.14173","last_updated":"2024-06-20T10:26:39Z","snapshot_observed_at":"2026-08-13T05:09:15.145990Z","submitted_at":"2024-06-20T10:26:39Z","title":"Time-Delay Interferometry for ASTROD-GW","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.14173","snapshot_observed_at":"2026-08-14T04:42:58.111116Z","title":"Wang, Time-Delay Interferometry for ASTROD-GW (2011), arXiv:2406.14173 [gr-qc]","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.111116Z"},"links":{"cited_paper":"/paper/2406.14173","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:15c85733570cfa761fc1b2826215d9df799d2e1d1abf9f4811b982ef8c80e411","observation_id":"8967f683-1069-45af-86b4-c638bf6a3d86","resolution":{"observed_at":"2026-08-14T04:42:58.111116Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0504145","last_updated":"2005-06-28T19:27:51Z","snapshot_observed_at":"2026-07-07T03:20:53.471754Z","submitted_at":"2005-04-29T19:08:15Z","title":"Geometric Time Delay Interferometry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0504145","snapshot_observed_at":"2026-08-14T04:42:58.116947Z","title":"Vallisneri, Geometric time delay interferometry, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.116947Z"},"links":{"cited_paper":"/paper/gr-qc/0504145","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:cd0fcf401b45a615dfbac3e7d625ed46acb6734ab44742b1e5e91d02ed83f70d","observation_id":"d408658e-9a9a-43c4-bf83-f64a14fd48b5","resolution":{"observed_at":"2026-08-14T04:42:58.116947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:43:00.039199Z","title":null,"venue":null,"work_id":"e8ca79f8-d147-4cc9-bf4e-1463625eefad","year":1975},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.122312Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:56908524bb9e2e0a561e685f0fc709d4b162e9452ed49196c204ef58f49a4cb8","observation_id":"cfe9a60c-6550-4e47-9e28-bda70f834c2a","resolution":{"observed_at":"2026-08-14T04:43:00.044645Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:42:58.127031Z","title":"Wahlquist, The Doppler response to gravitational waves from a binary star source., General Relativity and Gravitation19, 1101 (1987)","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.127031Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:c57fc445262a84f01697f07c606f254f35dd6c9c31271712991fd2ca59bbb68e","observation_id":"83848404-528e-40c2-baf3-ff50a4d49e40","resolution":{"observed_at":"2026-08-14T04:42:58.127031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.4369","last_updated":"2008-03-04T17:00:56Z","snapshot_observed_at":"2026-08-11T10:07:17.564054Z","submitted_at":"2007-10-24T01:29:46Z","title":"Sensitivity and parameter-estimation precision for alternate LISA configurations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.4369","snapshot_observed_at":"2026-08-14T04:42:58.132483Z","title":"Vallisneri, J","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.132483Z"},"links":{"cited_paper":"/paper/0710.4369","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4b9be4901e795eac92b18395f43ee7d607af3b4d0b8b8d2b3ba24d4e83dfefe5","observation_id":"816a2b64-a75d-41db-af7b-0170e0749548","resolution":{"observed_at":"2026-08-14T04:42:58.132483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.1302","last_updated":"2010-10-06T23:33:59Z","snapshot_observed_at":"2026-08-07T11:16:00.612809Z","submitted_at":"2010-10-06T23:33:59Z","title":"LISA Sensitivities to Gravitational Waves from Relativistic Metric Theories of Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.1302","snapshot_observed_at":"2026-08-14T04:42:58.138372Z","title":"Tinto and M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.138372Z"},"links":{"cited_paper":"/paper/1010.1302","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:90b7bc739d0d00ffa6822f650a69ff352a07d1c80614fd1f24e5e810327325a6","observation_id":"3aa7e3c6-6f3f-456b-9a87-6589ca426d12","resolution":{"observed_at":"2026-08-14T04:42:58.138372Z","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":"2026-08-14T04:42:58.143383Z","title":"Wang, Time delay interferometry with minimal null frequencies and shortened time span, Sci","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.143383Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:2542faf03f3ee1a3542985e7f7f0a4bf8e0590c4f0abb19cc3ba2d714ad5e98c","observation_id":"9970e5dd-d268-4ea0-a08b-6b7cb01c9f69","resolution":{"observed_at":"2026-08-14T04:42:58.143383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0209039","last_updated":"2003-06-04T05:04:15Z","snapshot_observed_at":"2026-07-07T03:16:22.102309Z","submitted_at":"2002-09-12T06:45:36Z","title":"The LISA Optimal Sensitivity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0209039","snapshot_observed_at":"2026-08-14T04:42:58.147825Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.147825Z"},"links":{"cited_paper":"/paper/gr-qc/0209039","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:a9667e79f192540c87ddee4672e3f2d137e24d2a6200cb26c8c3dde95b3a8895","observation_id":"8c96a769-2671-4c94-bc4f-9101256fbb7a","resolution":{"observed_at":"2026-08-14T04:42:58.147825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.06889","last_updated":"2017-04-07T16:55:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2016-08-24T16:28:38Z","title":"Detection methods for stochastic gravitational-wave backgrounds: a unified treatment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.06889","snapshot_observed_at":"2026-08-14T04:42:58.152637Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.152637Z"},"links":{"cited_paper":"/paper/1608.06889","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:3d6f3525262cff91c0ea0ea6eb05113a646809f881f70c23b05b75176abd252c","observation_id":"6b5f7c19-1f73-4700-9b35-b4da94721621","resolution":{"observed_at":"2026-08-14T04:42:58.152637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:43:00.008767Z","title":null,"venue":null,"work_id":"93498760-3251-4a51-908b-cdd6602f32e7","year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.157466Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:c3dbd6da1151deae6e4075ce1a3560f302de7e243ffb82283a0c6699587b26ae","observation_id":"6343a05a-892c-4a2a-9ac3-9d6b162b3fb5","resolution":{"observed_at":"2026-08-14T04:43:00.014432Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.05812","last_updated":"2022-08-02T13:36:10Z","snapshot_observed_at":"2026-08-09T23:09:29.819892Z","submitted_at":"2020-08-13T10:56:39Z","title":"Revisiting time delay interferometry for unequal-arm LISA and TAIJI","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.05812","snapshot_observed_at":"2026-08-14T04:42:58.161812Z","title":"Wang and W.-T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.161812Z"},"links":{"cited_paper":"/paper/2008.05812","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:5ff60c6cdec1aa548e073769087862a0008511c2dec8a2005f536c13645e5320","observation_id":"cdea39eb-fcab-43fe-8b82-ace99fc48014","resolution":{"observed_at":"2026-08-14T04:42:58.161812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15544","last_updated":"2021-06-03T13:13:07Z","snapshot_observed_at":"2026-08-06T12:10:28.336878Z","submitted_at":"2020-10-29T13:24:04Z","title":"Algorithm for TDI numerical simulation and sensitivity investigation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15544","snapshot_observed_at":"2026-08-14T04:42:58.166823Z","title":"Wang, W.-T","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.166823Z"},"links":{"cited_paper":"/paper/2010.15544","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:d8c5ae079cd8e51c861b8bbb79c4d3e89cda6bafa1bb02076a9860b461e25aff","observation_id":"68f04172-6cfc-439a-983c-91047f863fe3","resolution":{"observed_at":"2026-08-14T04:42:58.166823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9604033","last_updated":"1996-09-30T22:23:11Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1996-04-16T18:47:08Z","title":"The stochastic gravity-wave background: sources and detection","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9604033","snapshot_observed_at":"2026-08-14T04:42:58.171352Z","title":"Allen, The Stochastic gravity wave background: Sources and detection, inLes Houches School of Physics: Astrophysical Sources of Gravitational Radiation(1996) arXiv:gr-qc/9604033","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.171352Z"},"links":{"cited_paper":"/paper/gr-qc/9604033","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:c4619391f5dcfe99e47443ea15be2ae08cdf138bfacd812f83d4e98809588339","observation_id":"624cbc7e-4c65-44a0-a0c0-7f2176fa33fa","resolution":{"observed_at":"2026-08-14T04:42:58.171352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9710117","last_updated":"1997-10-27T21:41:31Z","snapshot_observed_at":"2026-07-07T03:28:08.861130Z","submitted_at":"1997-10-27T21:41:31Z","title":"Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9710117","snapshot_observed_at":"2026-08-14T04:42:58.176027Z","title":"Allen and J","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.176027Z"},"links":{"cited_paper":"/paper/gr-qc/9710117","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:fdc7153e5cee3df8c00848233ddd30765985e852497713d6fd9dcf28e9e56094","observation_id":"cfb721ae-d4dc-4986-bcf1-c197f5c69d79","resolution":{"observed_at":"2026-08-14T04:42:58.176027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0103075","last_updated":"2001-03-24T23:32:51Z","snapshot_observed_at":"2026-07-07T03:13:57.163820Z","submitted_at":"2001-03-21T09:06:28Z","title":"Space missions to detect the cosmic gravitational-wave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0103075","snapshot_observed_at":"2026-08-14T04:42:58.180922Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.180922Z"},"links":{"cited_paper":"/paper/gr-qc/0103075","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:3542513fd6486743d60dc566af604e91ea8e3432bd0f4cc9afe66d2276a74d02","observation_id":"d0c2071d-2dbb-4308-a379-e80ba9545d31","resolution":{"observed_at":"2026-08-14T04:42:58.180922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.09244","last_updated":"2019-06-21T17:08:48Z","snapshot_observed_at":"2026-08-14T16:12:31.238446Z","submitted_at":"2019-06-21T17:08:48Z","title":"Reconstructing the spectral shape of a stochastic gravitational wave background with LISA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.09244","snapshot_observed_at":"2026-08-14T04:42:58.186121Z","title":"Caprini, D","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.186121Z"},"links":{"cited_paper":"/paper/1906.09244","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:8e8c359e79417a6b1d0675e8a76e9c7e3e848f4e9a65322095f308f237d4bfea","observation_id":"475f0614-336b-4c9c-8bb9-7a1ce70adc72","resolution":{"observed_at":"2026-08-14T04:42:58.186121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-14T04:42:58.190876Z","title":"Aghanimet al.(Planck), Planck 2018 results","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.190876Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:2922814cdb05b882544646bb0bf6edbe2ccdffd8c3d701f14a752ac5f884c627","observation_id":"8fb976d8-2d75-43d6-8ba1-8f785ef226c2","resolution":{"observed_at":"2026-08-14T04:42:58.190876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.5300","last_updated":"2013-11-25T17:13:47Z","snapshot_observed_at":"2026-07-06T03:26:03.309810Z","submitted_at":"2013-10-20T04:08:41Z","title":"Sensitivity curves for searches for gravitational-wave backgrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.5300","snapshot_observed_at":"2026-08-14T04:42:58.195614Z","title":"Thrane and J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.195614Z"},"links":{"cited_paper":"/paper/1310.5300","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:8a742e2d48b58c11e99c98b0807275f6217d6d58f4ffc621323f25b1e6fe26b7","observation_id":"9f9b34ce-969c-44f8-a36e-2212076e23d0","resolution":{"observed_at":"2026-08-14T04:42:58.195614Z","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":"2026-08-14T11:17:30.102515Z","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":"2026-08-14T04:42:58.200399Z","title":"Capriniet al., Science with the space-based interfer- ometer eLISA","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.200399Z"},"links":{"cited_paper":"/paper/1512.06239","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:bf478de6bc9e856b4797701d6c43bd0321f3985cdde78171747c78c7f3b62cd4","observation_id":"679965a6-e773-46ae-bc85-01c2fe15feda","resolution":{"observed_at":"2026-08-14T04:42:58.200399Z","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":"2026-08-14T04:42:58.205558Z","title":"Capriniet al., Detecting gravitational waves from cos- mological phase transitions with LISA: an update, JCAP 03, 024, arXiv:1910.13125 [astro-ph.CO]","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.205558Z"},"links":{"cited_paper":"/paper/1910.13125","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:190f4b2c866311a331ebcacb0de820dc629753e5e6e8eb427dc62254bd879273","observation_id":"f7e303bb-9928-456c-a7a1-b6098ec03b60","resolution":{"observed_at":"2026-08-14T04:42:58.205558Z","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":"2026-08-10T07:12:13.034438Z","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":"2026-08-14T04:42:58.211034Z","title":"Kuroyanagi, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.211034Z"},"links":{"cited_paper":"/paper/1807.00786","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:38f4f9f96a01dd96c8e841a3ad500dc53d63d4f54a643213cbe04590716321a5","observation_id":"f0171bf0-a89f-4296-a635-10f09fe6b0f7","resolution":{"observed_at":"2026-08-14T04:42:58.211034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.11845","last_updated":"2021-02-16T12:14:21Z","snapshot_observed_at":"2026-08-14T06:54:34.145629Z","submitted_at":"2020-09-24T17:48:06Z","title":"Improved reconstruction of a stochastic gravitational wave background with LISA","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.11845","snapshot_observed_at":"2026-08-14T04:42:58.216210Z","title":"Flauger, N","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.216210Z"},"links":{"cited_paper":"/paper/2009.11845","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4f37bc3a9db8fd98bb0090605f53584afd89d49cccf03d99d4df34676e16ee67","observation_id":"3a33b855-1038-4698-abb7-117502f25191","resolution":{"observed_at":"2026-08-14T04:42:58.216210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05697","last_updated":"2020-11-11T11:06:24Z","snapshot_observed_at":"2026-08-12T14:26:20.962497Z","submitted_at":"2020-11-11T11:06:24Z","title":"Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.05697","snapshot_observed_at":"2026-08-14T04:42:58.221073Z","title":"Martinovic, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.221073Z"},"links":{"cited_paper":"/paper/2011.05697","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:5e32fdae9c5e5a669f643258c982423936699d12620eca506ab40b2c5ef640cc","observation_id":"10747884-70cf-4157-a0fb-59e82fb6143c","resolution":{"observed_at":"2026-08-14T04:42:58.221073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14183","last_updated":"2023-06-27T08:47:55Z","snapshot_observed_at":"2026-08-13T14:17:38.371114Z","submitted_at":"2022-09-28T15:58:57Z","title":"Primordial Black Hole Formation in Starobinsky's Linear Potential Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14183","snapshot_observed_at":"2026-08-14T04:42:58.226725Z","title":"Pi and J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.226725Z"},"links":{"cited_paper":"/paper/2209.14183","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:e6c3c372b757b039a1be52e9d25243274c3e1db66606ff03a357a8d4692994a4","observation_id":"0bfd12a4-dfd0-4206-9cc1-07fbda8948be","resolution":{"observed_at":"2026-08-14T04:42:58.226725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T04:42:59.991290Z","title":"LiGong, P","venue":null,"work_id":"f74e1964-9cab-4593-ada7-d5ec6969a3d9","year":2025},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.231636Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:867c929271a502b1c1ece79cdfa6fd0db98002760d42a39e886c1aa9581b07c7","observation_id":"15e13477-491b-4640-a88d-6ac44549573a","resolution":{"observed_at":"2026-08-14T04:42:59.996362Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.05055","last_updated":"2021-10-07T11:21:26Z","snapshot_observed_at":"2026-08-13T21:05:06.804748Z","submitted_at":"2020-11-10T11:40:57Z","title":"Spectral separation of the stochastic gravitational-wave background for LISA: observing both cosmological and astrophysical backgrounds","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.05055","snapshot_observed_at":"2026-08-14T04:42:58.236257Z","title":"Boileau, N","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.236257Z"},"links":{"cited_paper":"/paper/2011.05055","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:31a878077c9639313909ceca086093c252e84e9f83cb37ce77dd4043934cc98a","observation_id":"f5400ee9-bb0e-4511-acaa-8c3426d7b5b2","resolution":{"observed_at":"2026-08-14T04:42:58.236257Z","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":"2026-08-14T04:42:58.240844Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.240844Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4b513249e7aa8dc7fdf6592f09f57aa51c59037e5cb31c787ddab5f4045f440e","observation_id":"62fb6dfb-af78-4a80-89c7-8c699db276a9","resolution":{"observed_at":"2026-08-14T04:42:58.240844Z","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":"2026-08-14T04:42:58.245247Z","title":"Virtanen, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.245247Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:98b03ca3269d6014161bdbbcb4eb59019ef28207e99e58a143c6a31770f4fedf","observation_id":"ed518b8f-04b0-4e5e-9306-585eddb23b8c","resolution":{"observed_at":"2026-08-14T04:42:58.245247Z","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":"2026-08-14T04:42:58.249816Z","title":"pandas development team, pandas-dev/pandas: Pan- das (2020)","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.249816Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:64153cbc73d0986d91d32b59de1691ba2812b003dd9115b1c524d2d73c146081","observation_id":"196668b1-2703-45ed-a84f-4c9619f7bf53","resolution":{"observed_at":"2026-08-14T04:42:58.249816Z","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":"2026-08-14T04:42:58.254261Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.254261Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:4da4510795b181372169e924a545f69f8f47b0fbac1aa2e269251024902ea7cf","observation_id":"ce32a154-d7ce-4833-979b-7e6639575483","resolution":{"observed_at":"2026-08-14T04:42:58.254261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-14T04:42:58.258882Z","title":"Lewis, GetDist: a Python package for analysing Monte Carlo samples, (2019), arXiv:1910.13970 [astro-ph.IM]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.258882Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:432e308b86e0d89d5838a1b32b263f025222629477bd5aad262ddeac894dbfc2","observation_id":"f09f1288-4529-4799-b9b3-586355cf0390","resolution":{"observed_at":"2026-08-14T04:42:58.258882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0409513","last_updated":"2004-09-21T18:00:00Z","snapshot_observed_at":"2026-07-07T00:44:53.460945Z","submitted_at":"2004-09-21T18:00:00Z","title":"HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0409513","snapshot_observed_at":"2026-08-14T04:42:58.263706Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.263706Z"},"links":{"cited_paper":"/paper/astro-ph/0409513","citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:22f461eea345dc1904f6e912de0b43f793c4bb6ca29873f25635760bcb562e25","observation_id":"86c58be0-fd84-4802-bd10-17a83e8e3d22","resolution":{"observed_at":"2026-08-14T04:42:58.263706Z","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":"2026-08-14T04:42:58.268186Z","title":"Zonca, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T04:42:58.268186Z"},"links":{"citing_paper":"/paper/2608.08490"},"observation_digest":"sha256:a899c0c4cfb122f2ec4b81776a0873a37b93cbbe9d88d057d058342ef5894603","observation_id":"facd5c81-0dea-4b59-8e3d-d062545b13e8","resolution":{"observed_at":"2026-08-14T04:42:58.268186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.08490","last_updated":"2026-08-09T05:23:25Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T17:46:59.941353Z","submitted_at":"2026-08-09T05:23:25Z","title":"Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background"},"reference_resolution":{"displayed":87,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":77,"verified_exact":9,"verified_fuzzy":1},"total_outbound_references":87},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 87 of 87 outbound references and 0 inbound Pith citation observations for arXiv:2608.08490."}