{"as_of":"2026-08-19T13:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c9757eaf9fbf89b4ecb6e414e2863a18df92dc2833b231ae3f470158473b7771","coverage":[{"denominator":78,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":78,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T12:59:24.234088Z","state":"measured"},{"denominator":78,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":78,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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/2607.29141/citation-record","integrity":"/paper/2607.29141/integrity","json":"/paper/2607.29141/citation-record.json","paper":"/paper/2607.29141"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T12:59:14.625414Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:14.625414Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:7c6a9dd4a97bc1ecd90ab8f32c2e47a09a11da4236c5a6783b668a63db0c229e","observation_id":"7be5a396-3774-49bf-9c65-9bad3c08cda0","resolution":{"observed_at":"2026-08-03T12:59:14.625414Z","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":"2026-08-03T12:59:14.763492Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:14.763492Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:57cd34a4850c15b8ab44ea2f5aaa435a0af836c35c97d9179de15a3d7ddaeeff","observation_id":"ec40745c-b820-4acf-9fd7-45365bd0fd70","resolution":{"observed_at":"2026-08-03T12:59:14.763492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.06268","last_updated":"2016-03-20T21:00:06Z","snapshot_observed_at":"2026-08-14T22:05:15.088153Z","submitted_at":"2016-03-20T21:00:06Z","title":"Effect of the rotation and tidal dissipation history of stars on the evolution of close-in planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.06268","snapshot_observed_at":"2026-08-03T12:59:14.897214Z","title":"Celestial Mechanics and Dynamical Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:14.897214Z"},"links":{"cited_paper":"/paper/1603.06268","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:f583dacf2ad45ffa530d473555a46c676b06e12e93f13a2cc1a00bb5c6158fb0","observation_id":"f18c1325-42ff-4814-b2be-30ece9aef3c8","resolution":{"observed_at":"2026-08-03T12:59:14.897214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.03262","last_updated":"2020-08-07T16:45:36Z","snapshot_observed_at":"2026-08-09T00:46:59.576821Z","submitted_at":"2020-08-07T16:45:36Z","title":"Tidal dissipation in evolving low-mass and solar-type stars with predictions for planetary orbital decay","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.03262","snapshot_observed_at":"2026-08-03T12:59:15.032940Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:15.032940Z"},"links":{"cited_paper":"/paper/2008.03262","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:21b011713f00e33c2315d7e2325469a207f017f61b0f0acb6b21335fbf2471f7","observation_id":"ef51ec7d-2bf8-409b-9482-a161e0d72ca3","resolution":{"observed_at":"2026-08-03T12:59:15.032940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.08805","last_updated":"2017-02-28T14:43:57Z","snapshot_observed_at":"2026-08-14T21:14:19.070801Z","submitted_at":"2017-02-28T14:43:57Z","title":"Tidal interactions in spin-orbit misaligned systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.08805","snapshot_observed_at":"2026-08-03T12:59:15.198150Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:15.198150Z"},"links":{"cited_paper":"/paper/1702.08805","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:fb0b394ec732696691e1c6aa1ff74ef9e612bf0bb1ec58e1901e5a009d1bfe4c","observation_id":"0b16cac5-e983-4f68-96ba-c1a805120934","resolution":{"observed_at":"2026-08-03T12:59:15.198150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702492","last_updated":"2007-02-19T18:40:10Z","snapshot_observed_at":"2026-08-15T10:47:22.510915Z","submitted_at":"2007-02-19T18:40:10Z","title":"Tidal dissipation in rotating solar-type stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702492","snapshot_observed_at":"2026-08-03T12:59:15.416374Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:15.416374Z"},"links":{"cited_paper":"/paper/astro-ph/0702492","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:ec0e2208d7e16c013314609032ba3ddab6b18b6e8f4f1e45ef637b8203791bed","observation_id":"bc3b3b3e-cec1-4699-9c93-385036d05721","resolution":{"observed_at":"2026-08-03T12:59:15.416374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04442","last_updated":"2022-03-08T23:28:48Z","snapshot_observed_at":"2026-08-16T17:16:00.861352Z","submitted_at":"2022-03-08T23:28:48Z","title":"Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04442","snapshot_observed_at":"2026-08-03T12:59:15.612354Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:15.612354Z"},"links":{"cited_paper":"/paper/2203.04442","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:1b1726d0746dd9e76588d22b0b0da153a7d5d5149b4e1144f920c759f8be3c0d","observation_id":"97251018-b1d1-45fe-a655-2748f2b2d833","resolution":{"observed_at":"2026-08-03T12:59:15.612354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.12624","last_updated":"2020-07-24T16:24:34Z","snapshot_observed_at":"2026-08-13T22:02:20.954756Z","submitted_at":"2020-07-24T16:24:34Z","title":"Convective turbulent viscosity acting on equilibrium tidal flows: new frequency scaling of the effective viscosity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.12624","snapshot_observed_at":"2026-08-03T12:59:15.820787Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:15.820787Z"},"links":{"cited_paper":"/paper/2007.12624","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:409a519d72264ecbfadd8788109b84bd8ce7031fd15f051977d2430471a19c1b","observation_id":"bb0e4ccd-944a-4691-bc65-0bcd14e9c533","resolution":{"observed_at":"2026-08-03T12:59:15.820787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.17622","last_updated":"2023-06-30T12:52:01Z","snapshot_observed_at":"2026-08-16T15:19:45.210575Z","submitted_at":"2023-06-30T12:52:01Z","title":"Tidal dissipation due to the elliptical instability and turbulent viscosity in convection zones in rotating giant planets and stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17622","snapshot_observed_at":"2026-08-03T12:59:16.070726Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.070726Z"},"links":{"cited_paper":"/paper/2306.17622","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b8b8fe2393d23a835387317aceefa344082b1f36b2ee14dc35573e96b4540a5b","observation_id":"5eb20bc3-bfb7-419a-ba96-b6ce2911977a","resolution":{"observed_at":"2026-08-03T12:59:16.070726Z","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":"2026-08-03T12:59:16.211270Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.211270Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:ec38eaa957e6ddc252a9333a6e3f73a8d736cfb11c22cee8c001ef3fa2272a6b","observation_id":"bc93f382-445b-4943-893e-e76edf95ca8e","resolution":{"observed_at":"2026-08-03T12:59:16.211270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.03653","last_updated":"2022-01-10T21:16:49Z","snapshot_observed_at":"2026-08-16T17:29:11.753230Z","submitted_at":"2022-01-10T21:16:49Z","title":"Tidal erasure of stellar obliquities constrains the timing of hot Jupiter formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.03653","snapshot_observed_at":"2026-08-03T12:59:16.353931Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.353931Z"},"links":{"cited_paper":"/paper/2201.03653","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:afa35a7885cbad7080f9e4f6e3e0b760352c3e78989541cf1f5603413e1ff571","observation_id":"470316de-bad0-4c0b-86e4-2580a25e9312","resolution":{"observed_at":"2026-08-03T12:59:16.353931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.09661","last_updated":"2018-03-26T15:29:29Z","snapshot_observed_at":"2026-08-15T15:24:17.060797Z","submitted_at":"2018-03-26T15:29:29Z","title":"Influence of stellar structure, evolution and rotation on the tidal damping of exoplanetary spin-orbit angles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.09661","snapshot_observed_at":"2026-08-03T12:59:16.462053Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.462053Z"},"links":{"cited_paper":"/paper/1803.09661","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:f0a181fdb0f46f35acf3b1faa783a2402f0ca391a3fb5476585569d709d47fcb","observation_id":"eeab7151-01ee-43ef-bdb5-34082a3b9577","resolution":{"observed_at":"2026-08-03T12:59:16.462053Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.03867","last_updated":"2016-05-12T15:54:24Z","snapshot_observed_at":"2026-08-18T08:54:14.856980Z","submitted_at":"2016-05-12T15:54:24Z","title":"On turbulence driven by axial precession and tidal evolution of the spin-orbit angle of close-in giant planets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.03867","snapshot_observed_at":"2026-08-03T12:59:16.534472Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.534472Z"},"links":{"cited_paper":"/paper/1605.03867","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:e642c8bf612ef3a13aaf476659a2ebb8611c1dcfdac5fc9868d567198c3050c5","observation_id":"6b37f2ea-cbd7-4432-b6e3-037e1d6be949","resolution":{"observed_at":"2026-08-03T12:59:16.534472Z","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":"2026-08-03T12:59:16.599379Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.599379Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:a00e485a025d6e03b9c8beb60383519c97540a6c73922375800e4660049a8200","observation_id":"545f3c4e-0454-4029-8029-75b8ca6449b6","resolution":{"observed_at":"2026-08-03T12:59:16.599379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.01004","last_updated":"2021-04-16T08:52:41Z","snapshot_observed_at":"2026-08-16T18:34:15.073916Z","submitted_at":"2021-04-02T12:13:52Z","title":"Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.01004","snapshot_observed_at":"2026-08-03T12:59:16.698699Z","title":"Influence of secular evolution on their population","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.698699Z"},"links":{"cited_paper":"/paper/2104.01004","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:bb47b06a3b4a8b503ae2ca646096a501434830d8b474fdfbd23bbc6a756beda0","observation_id":"b5abeb2e-c68a-4857-8a77-888570f7a42a","resolution":{"observed_at":"2026-08-03T12:59:16.698699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09257","last_updated":"2021-12-12T22:40:06Z","snapshot_observed_at":"2026-08-16T17:55:33.413076Z","submitted_at":"2021-09-20T01:09:57Z","title":"Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.09257","snapshot_observed_at":"2026-08-03T12:59:16.782198Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.782198Z"},"links":{"cited_paper":"/paper/2109.09257","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:64520da0db85ace9fee086662debff3dcc08101da7b49b2e87444be4cdc473de","observation_id":"b2408767-00fc-4de2-b102-fec4edee27fc","resolution":{"observed_at":"2026-08-03T12:59:16.782198Z","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":"2026-08-03T12:59:16.881215Z","title":"3D Obliquities of Five Low-Mass Eclipsing Binaries","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.881215Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:fd918eb09b4a3383ab6f0853bd453cae9dee693a0ab12e1ab15371fd5d8a3cc3","observation_id":"205bc049-c2a0-4017-9379-0e38927e4033","resolution":{"observed_at":"2026-08-03T12:59:16.881215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06324","last_updated":"2023-08-11T18:00:46Z","snapshot_observed_at":"2026-08-18T06:48:24.743653Z","submitted_at":"2023-08-11T18:00:46Z","title":"Measuring Tidal Dissipation in Giant Planets from Tidal Circularization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06324","snapshot_observed_at":"2026-08-03T12:59:16.989469Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:16.989469Z"},"links":{"cited_paper":"/paper/2308.06324","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:72f59ffb3c42248da6c24ca571311db5772f0c703070b44d829dc8d0d3cc225d","observation_id":"1e7f07c6-6690-4e9f-86f9-4eb3bffb825b","resolution":{"observed_at":"2026-08-03T12:59:16.989469Z","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":"10.1051/0004-6361:20021671","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Axisymmetric shear Alfv \\'e n modes of a spherical shell in a dipolar magnetic field","venue":"Astronomy and Astrophysics","work_id":"c21a2dee-5d2a-42e5-aaef-949a27f549e3","year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:17.106428Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:3603caf535f2ee4df0c76dcd234a38dbc522942d091f0e718eb4b8661531ba0f","observation_id":"b20fa83a-4456-4b4a-8d79-5e147b4418d5","resolution":{"observed_at":"2026-08-03T13:03:27.587705Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-03T12:59:17.300141Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:17.300141Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:20b7e063c9e7f687f005847f1555d3111ab31b3e674d76c8e5d4b266897ea054","observation_id":"ef35e7b3-af99-4ef9-b6bc-30fec05f03c5","resolution":{"observed_at":"2026-08-03T12:59:17.300141Z","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":"10.1103/physrevlett.99.194501","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"自由と正義","work_id":"8c94a8cf-72a8-4a11-bf23-b5beec6a24dd","year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:17.544085Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:c901faf9427fdba61ecca357adfa9ad80cedce193456a5e49bab23940d16bfad","observation_id":"18abefa5-5637-42ed-80de-bdfc64adf1b5","resolution":{"observed_at":"2026-08-03T13:03:27.577724Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.08109","last_updated":"2022-09-22T20:54:25Z","snapshot_observed_at":"2026-08-16T16:31:56.422362Z","submitted_at":"2022-09-16T18:00:11Z","title":"Comprehensive Bayesian Modeling of Tidal Circularization in Open Cluster Binaries part I: M 35, NGC 6819, NGC 188","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.08109","snapshot_observed_at":"2026-08-03T12:59:17.756709Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:17.756709Z"},"links":{"cited_paper":"/paper/2209.08109","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:51c0151bee903e16aacfa9b8e49ffa490609c87c2b812ed028adf480ca40a07b","observation_id":"f26a3fc9-4acc-47db-aca1-95bf0aeb7dc4","resolution":{"observed_at":"2026-08-03T12:59:17.756709Z","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":"2026-08-03T12:59:17.931100Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:17.931100Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:38410148e2d04e429266795dc5f4395c31e4becc4dc49b7e7b2e695d6cd5b61f","observation_id":"de8a2d09-22ea-43a9-9c5f-a99a15d5e7a5","resolution":{"observed_at":"2026-08-03T12:59:17.931100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.1938","last_updated":"2009-04-13T10:14:24Z","snapshot_observed_at":"2026-08-18T13:47:44.124193Z","submitted_at":"2009-04-13T10:14:24Z","title":"Magnetic fields of non-degenerate stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.1938","snapshot_observed_at":"2026-08-03T12:59:18.031200Z","title":", keywords =","venue":null,"work_id":null,"year":1938},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.031200Z"},"links":{"cited_paper":"/paper/0904.1938","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:db3dc1f02e976adc657d8d72ed2107d62690fb7340d31e0838d85f9fdac49411","observation_id":"5a747bc6-fede-4777-9efe-becb59c147fc","resolution":{"observed_at":"2026-08-03T12:59:18.031200Z","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":"10.1146/annurev-fluid-122109-160727","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Annual Review of Fluid Mechanics , year = 2011, month = jan, volume =","venue":"Annual Review of Fluid Mechanics","work_id":"83955338-29d9-4be3-a234-756c4596ba7c","year":2011},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.253972Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:0ab415f0730f0883a88490e886086b2e5bcbcbefe312e5074c3220af6178d61f","observation_id":"7aa57e08-f66e-41dc-8729-c175a0002be3","resolution":{"observed_at":"2026-08-03T13:03:27.566137Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-03T12:59:18.405673Z","title":"The Astrophysical Journal Letters , volume=","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.405673Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:fd7aadb6650f6250bd10dc2644dfa9ab516ec76e53dd5ed33f6666bde8079eed","observation_id":"52f5a18f-6620-42ee-9028-1be5b0aafe10","resolution":{"observed_at":"2026-08-03T12:59:18.405673Z","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":"2026-08-03T12:59:18.532773Z","title":"Monthly Notices of the Royal Astronomical Society , pages=","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.532773Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:d63388e16ecb4efb367dbe7ca6654cafd74861b90b7be99fbbcbdf5ea626a33c","observation_id":"4f63193a-baf7-4bce-9bc5-58213fd0eb38","resolution":{"observed_at":"2026-08-03T12:59:18.532773Z","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":"2026-08-03T12:59:18.625645Z","title":"Annual Review of Astronomy and Astrophysics , volume=","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.625645Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b00975ee3b26d79f11da2cb01b2e74f889f9322600f7a0dd98a3c183b4676c45","observation_id":"14a26fb0-b6d1-4f12-a81b-f1d304a2c146","resolution":{"observed_at":"2026-08-03T12:59:18.625645Z","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":"2026-08-03T12:59:18.767609Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.767609Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:16fac6f0a49b0567033022a6673e89a97adad0a3cf749f2fb73691dcae84f649","observation_id":"edd70f24-9166-46a9-8f48-171cc611d660","resolution":{"observed_at":"2026-08-03T12:59:18.767609Z","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":"2026-08-03T12:59:18.914267Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:18.914267Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b1b8b3f63505599afb28c8c5f786d81eb732f3dbd676746b29f0ce4a936c3769","observation_id":"ade0ed57-4652-4cd6-aa18-5f89fa14b5bf","resolution":{"observed_at":"2026-08-03T12:59:18.914267Z","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":"2026-08-03T12:59:19.056815Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.056815Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:c408ab845ee7580d1c74165b2b933c3931a2a9ff6f87bcd6c7563d44f8c0790c","observation_id":"a071ea92-7bc6-4bbb-a5dc-56302d331770","resolution":{"observed_at":"2026-08-03T12:59:19.056815Z","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":"2026-08-03T12:59:19.189037Z","title":"Physics of the Earth and Planetary Interiors , volume=","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.189037Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:8fa23c667552287e3951f965db642114e04b0706c09742cc48f90c119c6f3c42","observation_id":"d01a5844-27d6-4dfe-b13f-de6ee2efe54f","resolution":{"observed_at":"2026-08-03T12:59:19.189037Z","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":"2026-08-03T12:59:19.340146Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.340146Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:2647323544ef2da300665127313deabc29a125e5da5b9b0c07f5ba2a5b6a24ea","observation_id":"a9bae223-d755-412a-bdc5-3ddfe7a1c77c","resolution":{"observed_at":"2026-08-03T12:59:19.340146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601461","last_updated":"2006-01-19T22:58:44Z","snapshot_observed_at":"2026-07-07T00:57:45.936590Z","submitted_at":"2006-01-19T22:58:44Z","title":"Evolutionary state of magnetic chemically peculiar stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601461","snapshot_observed_at":"2026-08-03T12:59:19.535076Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.535076Z"},"links":{"cited_paper":"/paper/astro-ph/0601461","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:a9ca9142f2a8b9311c33917b73cdab8b04bd6ff07dd8712486d1509e73d23876","observation_id":"5a030e80-df9d-4e90-b2ef-5b294f82c4a1","resolution":{"observed_at":"2026-08-03T12:59:19.535076Z","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":"2026-08-03T12:59:19.674586Z","title":"Physical Review Research , volume=","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.674586Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:2168413fd69119e92236772b147c8d3dd2e1ead92ff77ebd8d367272666f0ac8","observation_id":"a68f91ed-18b7-4d3a-a02d-195487187387","resolution":{"observed_at":"2026-08-03T12:59:19.674586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.05552","last_updated":"2018-01-19T05:05:51Z","snapshot_observed_at":"2026-08-14T19:54:29.987187Z","submitted_at":"2018-01-17T05:10:37Z","title":"Magnetic effect on dynamical tide in rapidly rotating astronomical objects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.05552","snapshot_observed_at":"2026-08-03T12:59:19.760210Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.760210Z"},"links":{"cited_paper":"/paper/1801.05552","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:16cf7395e0ef9752bd4f16a79a3b87b4702d9b628ccd3b9e1b47e1ccaf9df4d4","observation_id":"ae115b10-4034-458e-9d6e-09818c2c1643","resolution":{"observed_at":"2026-08-03T12:59:19.760210Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.10490","last_updated":"2019-09-23T17:17:35Z","snapshot_observed_at":"2026-08-15T14:12:59.911753Z","submitted_at":"2019-09-23T17:17:35Z","title":"Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.10490","snapshot_observed_at":"2026-08-03T12:59:19.877555Z","title":", keywords =","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.877555Z"},"links":{"cited_paper":"/paper/1909.10490","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:9565d6f8023e30265f40ceaa2303950add1f790d6173849c2ed6313870b06ac1","observation_id":"8980eea8-e5d7-478d-b298-ed11c6d5e6d7","resolution":{"observed_at":"2026-08-03T12:59:19.877555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.15815","last_updated":"2023-11-27T13:40:38Z","snapshot_observed_at":"2026-08-19T09:02:37.729910Z","submitted_at":"2023-11-27T13:40:38Z","title":"Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.15815","snapshot_observed_at":"2026-08-03T12:59:19.984006Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:19.984006Z"},"links":{"cited_paper":"/paper/2311.15815","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:0a29be6ce37a05227cc968b47a894e5aca91abd2228c81f82d8fd7ec5efdd4f9","observation_id":"7b0d742e-404e-4020-9cbe-06f1784ca226","resolution":{"observed_at":"2026-08-03T12:59:19.984006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.03950","last_updated":"2022-03-08T09:24:05Z","snapshot_observed_at":"2026-08-16T17:16:13.468543Z","submitted_at":"2022-03-08T09:24:05Z","title":"Tidal dissipation due to inertial waves can explain the circularization periods of solar-type binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.03950","snapshot_observed_at":"2026-08-03T12:59:20.081045Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.081045Z"},"links":{"cited_paper":"/paper/2203.03950","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:535304bf4487cbb07bbee631b3f33bdf191918effd8191feff931e9dbde701bc","observation_id":"bdfd9db6-d723-49e4-b252-c9093bad4559","resolution":{"observed_at":"2026-08-03T12:59:20.081045Z","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":"10.1016/b978-0-443-21439-4.00075-4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Encyclopedia of Astrophysics , year = 2026, volume =","venue":"Elsevier eBooks","work_id":"2ef06549-a70c-4086-9b75-21027a8b15a9","year":2026},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.191100Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:eca6c24de612df43b3d9721c6fb0b78c46c4e84afd5f6a7218e44044d6b006e9","observation_id":"8f948c4b-4c7b-4512-a902-b98add4c8fba","resolution":{"observed_at":"2026-08-03T13:03:27.554918Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06960","last_updated":"2015-10-23T14:59:16Z","snapshot_observed_at":"2026-08-15T11:44:50.781712Z","submitted_at":"2015-10-23T14:59:16Z","title":"Asteroseismology Can Reveal Strong Internal Magnetic Fields in Red Giant Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06960","snapshot_observed_at":"2026-08-03T12:59:20.293585Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.293585Z"},"links":{"cited_paper":"/paper/1510.06960","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:2b7e7a0638e9f74d1bc08a12f00d7b1f2c7a73bfbce3bda10d62bd5f4d1d2988","observation_id":"f9a16161-fe92-41c0-abc8-b88a3a1e3b0b","resolution":{"observed_at":"2026-08-03T12:59:20.293585Z","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":"2026-08-03T12:59:20.405037Z","title":"Physics of Fluids , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.405037Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:2bdc6bdc8abca11551f867be29b9e86536cd6d3c52436107424c082d59da758f","observation_id":"7fdd4705-4695-4f0d-9d36-b889c652eb78","resolution":{"observed_at":"2026-08-03T12:59:20.405037Z","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":"2026-08-03T12:59:20.502294Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.502294Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:6b5f589b338588adc8672bc12c087f493906fbe18ec54520de99eb5fc7e17dfe","observation_id":"5ab4bca1-d5ce-445b-96ad-aa190b85aa9b","resolution":{"observed_at":"2026-08-03T12:59:20.502294Z","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":"2026-08-03T12:59:20.611210Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.611210Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:2a47a825bb0ff5b77c14f25669c9247d57141b44f7fa126232eda0c34e9e16de","observation_id":"166767a7-decb-4773-a833-4d697e4ebc89","resolution":{"observed_at":"2026-08-03T12:59:20.611210Z","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":"2026-08-03T12:59:20.716049Z","title":"The Solar Tachocline , year = 2007, editor =","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.716049Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:7b39e475db6362a46570a9f9a84840f9d06f28e6f47da021f9514354e72f7091","observation_id":"b53e0301-2cc5-4743-8448-b3c307f309ae","resolution":{"observed_at":"2026-08-03T12:59:20.716049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00225","last_updated":"2019-03-30T14:22:41Z","snapshot_observed_at":"2026-08-17T14:04:31.766132Z","submitted_at":"2019-03-30T14:22:41Z","title":"Rossby and Magnetic Prandtl Number Scaling of Stellar Dynamos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00225","snapshot_observed_at":"2026-08-03T12:59:20.873157Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.873157Z"},"links":{"cited_paper":"/paper/1904.00225","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:95fc888a9c40e9d626595d8f8ac49670397212999c418585fddf87ca7e6b2a24","observation_id":"3e8f1c65-7862-4bf3-ab84-6efa0a180b98","resolution":{"observed_at":"2026-08-03T12:59:20.873157Z","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":"2026-08-03T12:59:20.952823Z","title":"Science , year = 1996, month = may, volume =","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:20.952823Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:026927a603dff7c69ee09dc2481224995ddca556287dfba007e4597e28d620e6","observation_id":"965add81-db57-4f12-8cf1-c9088220834e","resolution":{"observed_at":"2026-08-03T12:59:20.952823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.00004","last_updated":"2016-01-06T02:20:01Z","snapshot_observed_at":"2026-08-14T22:16:18.881604Z","submitted_at":"2015-12-31T21:00:03Z","title":"A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.00004","snapshot_observed_at":"2026-08-03T12:59:21.123864Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.123864Z"},"links":{"cited_paper":"/paper/1601.00004","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:076fd79e6903ea969e76359479c732de2a1eed99d4a7d0e09a805420f2a230f8","observation_id":"5a08858f-7710-43b7-a14e-0d02f62dd1d6","resolution":{"observed_at":"2026-08-03T12:59:21.123864Z","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":"2026-08-03T12:59:21.249033Z","title":"Earth and Planetary Science Letters , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.249033Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b592ae7c858ad87a057dabb17a9eaa09f9ec90d5311e2ffe9c2599a4f263d5b8","observation_id":"599ab0b6-59aa-4326-b507-47584c348ec5","resolution":{"observed_at":"2026-08-03T12:59:21.249033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.09487","last_updated":"2022-08-19T18:00:01Z","snapshot_observed_at":"2026-08-16T16:38:06.326990Z","submitted_at":"2022-08-19T18:00:01Z","title":"30 to 100-kG magnetic fields in the cores of red giant stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.09487","snapshot_observed_at":"2026-08-03T12:59:21.335070Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.335070Z"},"links":{"cited_paper":"/paper/2208.09487","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:e22fdb151d9607eb7af5570cf3ec0ab5b9520009d5747fa336371d0d0a6d827e","observation_id":"2414940f-6e15-4c75-8a2e-380e64df4608","resolution":{"observed_at":"2026-08-03T12:59:21.335070Z","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":"2026-08-03T12:59:21.447334Z","title":"EAS Publications Series , year = 2019, series =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.447334Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:512b9fcb816be29c0a88ed8685fe9df1a398bd3a746ab12d8b058686bbf4e009","observation_id":"19512b4f-6d28-49e1-9bf5-161aa40ed017","resolution":{"observed_at":"2026-08-03T12:59:21.447334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.0643","last_updated":"2014-01-03T13:16:00Z","snapshot_observed_at":"2026-08-14T23:49:39.972405Z","submitted_at":"2014-01-03T13:16:00Z","title":"Nonlinear evolution of tidally forced inertial waves in rotating fluid bodies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.0643","snapshot_observed_at":"2026-08-03T12:59:21.543326Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.543326Z"},"links":{"cited_paper":"/paper/1401.0643","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:c0b06492ceddeacb7594c89ca3915597a4eb2501e61810932e15bc80292527bc","observation_id":"6633b2ed-aa7b-40fc-994d-dd61586a46c2","resolution":{"observed_at":"2026-08-03T12:59:21.543326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.04211","last_updated":"2015-04-30T20:58:38Z","snapshot_observed_at":"2026-08-19T08:34:10.442906Z","submitted_at":"2015-01-17T16:46:30Z","title":"On obliquely magnetized and differentially rotating stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.04211","snapshot_observed_at":"2026-08-03T12:59:21.651751Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.651751Z"},"links":{"cited_paper":"/paper/1501.04211","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:a53bcb66d90c4d4fd1228c5b3ea095e673393ae0bdc8c774c3f802cffb62a620","observation_id":"b2387ebe-d0c8-4498-b327-f0a6d3aa8964","resolution":{"observed_at":"2026-08-03T12:59:21.651751Z","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":"10.1017/s0022112067002447","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Journal of Fluid Mechanics , year = 1967, month = jan, volume =","venue":"Journal of Fluid Mechanics","work_id":"fb96b3ab-7a8c-45bb-99d9-01fadf0f4322","year":1967},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.718423Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:110f3bea63c7e1daedddf12b1b72eaf666f160f9eacafb4a4de2e2a7b7deca28","observation_id":"9bef6b74-47e9-41c3-aa4b-99b583d8491b","resolution":{"observed_at":"2026-08-03T13:03:27.522453Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-03T12:59:21.785805Z","title":"from the pms to the rgb at solar metallicity , author=","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.785805Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:8d8b4d7d373d36974ecfdf0838a5d6ec14eee4612fbb7b5d900f560861688f2b","observation_id":"fe166506-1a76-4d6e-b42a-07c38706e081","resolution":{"observed_at":"2026-08-03T12:59:21.785805Z","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":"2026-08-03T12:59:21.934866Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:21.934866Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b49616d1bd663c786b4917a13f34ba44068bedc1667bec58d0a9f5f816237e7e","observation_id":"18087d91-95ef-4deb-9936-30aaa6e95886","resolution":{"observed_at":"2026-08-03T12:59:21.934866Z","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":"2026-08-03T12:59:22.015781Z","title":"Les houches , volume=","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.015781Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:816a9481fc739238da952e558de26253726fd8931f60343cb440775f75c21287","observation_id":"f87d3cb2-9cc0-4b64-8f65-3b7a1a6406fe","resolution":{"observed_at":"2026-08-03T12:59:22.015781Z","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":"2026-08-03T12:59:22.055102Z","title":"Astronomy & Astrophysics , volume=","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.055102Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:be40b829740954baf1de83a80f74c0ab0b588f86beba401bcd98c1ac88058172","observation_id":"db72e1da-455a-4fe1-a2d6-a5fb3281d2f5","resolution":{"observed_at":"2026-08-03T12:59:22.055102Z","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":"2026-08-03T12:59:22.119032Z","title":"Astronomy & Astrophysics , volume=","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.119032Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:96987970967fa0857b7a7e9085dd31ff068683fecfbd28b64d572d885781d718","observation_id":"50b5890f-7c34-4dbe-aabb-0894d0cb5539","resolution":{"observed_at":"2026-08-03T12:59:22.119032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.03255","last_updated":"2016-05-11T01:35:55Z","snapshot_observed_at":"2026-08-14T21:57:56.133550Z","submitted_at":"2016-05-11T01:35:55Z","title":"The magnetic properties of the planet host star Kepler-78","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.03255","snapshot_observed_at":"2026-08-03T12:59:22.199958Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.199958Z"},"links":{"cited_paper":"/paper/1605.03255","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:50f77f5b57607af248819ff96789f73545e1f6340dd45d704f8d899daf5e16e7","observation_id":"c2667dd4-00e9-42b3-9215-24d11a39f062","resolution":{"observed_at":"2026-08-03T12:59:22.199958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01512","last_updated":"2017-01-06T00:20:25Z","snapshot_observed_at":"2026-08-19T07:37:47.452715Z","submitted_at":"2017-01-06T00:20:25Z","title":"A hot Jupiter around the very active weak-line T Tauri star TAP 26","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01512","snapshot_observed_at":"2026-08-03T12:59:22.256481Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.256481Z"},"links":{"cited_paper":"/paper/1701.01512","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:d6145dd729ef88b0fff45977b2fc4a650ad2ae4b0a1a86e86b35d93f292af53d","observation_id":"312fb18e-06c6-4e6c-bbc4-249915cef39c","resolution":{"observed_at":"2026-08-03T12:59:22.256481Z","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":"2026-08-03T12:59:22.388154Z","title":", keywords =","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.388154Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:e0a86dc4c5e470f81d6bb6366956405eaa0e930e6ab4bf1982229d18b929c1ea","observation_id":"05baf854-c9db-4032-9dd4-09eacd2d1bb4","resolution":{"observed_at":"2026-08-03T12:59:22.388154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1883","last_updated":"2010-08-11T10:46:25Z","snapshot_observed_at":"2026-08-15T05:11:42.288546Z","submitted_at":"2010-08-11T10:46:25Z","title":"The magnetic fields of forming solar-like stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1883","snapshot_observed_at":"2026-08-03T12:59:22.487814Z","title":"Reports on Progress in Physics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.487814Z"},"links":{"cited_paper":"/paper/1008.1883","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:4096ed3b812a09f918c9432b56989c6cbfcb79bd7ead194d8f5bb33c13decafa","observation_id":"0546aae3-88bf-4e0f-8703-17ad0d935947","resolution":{"observed_at":"2026-08-03T12:59:22.487814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.5901","last_updated":"2011-10-26T19:57:16Z","snapshot_observed_at":"2026-08-19T01:42:20.894320Z","submitted_at":"2011-10-26T19:57:16Z","title":"Analytic and numerical models of the 3D multipolar magnetospheres of pre-main sequence stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.5901","snapshot_observed_at":"2026-08-03T12:59:22.559579Z","title":"Astronomische Nachrichten , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.559579Z"},"links":{"cited_paper":"/paper/1110.5901","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:31cbce57698140585da31c6e7161fb95be94a1a968dadec6a2f5837203718687","observation_id":"5b7f43a1-1c52-4dcf-bc11-db3953bdc780","resolution":{"observed_at":"2026-08-03T12:59:22.559579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.5238","last_updated":"2012-06-22T19:53:59Z","snapshot_observed_at":"2026-08-15T00:55:42.760568Z","submitted_at":"2012-06-22T19:53:59Z","title":"Can we predict the global magnetic topology of a pre-main sequence star from its position in the Hertzsprung-Russell diagram?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.5238","snapshot_observed_at":"2026-08-03T12:59:22.635771Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.635771Z"},"links":{"cited_paper":"/paper/1206.5238","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:9d0f3389d4d1735654b4f556826036dad60330bc894d6bc73ab284ee8b0686e5","observation_id":"b9b4abeb-35d6-4efc-a852-ef3c80add78a","resolution":{"observed_at":"2026-08-03T12:59:22.635771Z","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":"2026-08-03T12:59:22.743229Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.743229Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:24f7d71d8a278de466fbddbb4b8adb927b777d4942aec4700e0d9df55de22165","observation_id":"811368b3-956f-4468-8125-78b2d32f41ee","resolution":{"observed_at":"2026-08-03T12:59:22.743229Z","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":"2026-08-03T12:59:22.751186Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.751186Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:1343b1220e7fadf1e02402b53a6c22139f0255ea2a1dec32a89c617196a24687","observation_id":"f86ffb14-b27c-4cd5-aea3-f8e067b8a43b","resolution":{"observed_at":"2026-08-03T12:59:22.751186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.5384","last_updated":"2010-09-27T20:02:19Z","snapshot_observed_at":"2026-08-18T15:55:46.249651Z","submitted_at":"2010-09-27T20:02:19Z","title":"On the Stability of Non Force-Free Magnetic Equilibria in Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.5384","snapshot_observed_at":"2026-08-03T12:59:22.872952Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.872952Z"},"links":{"cited_paper":"/paper/1009.5384","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:e011e8852da1c0084ce1c0fcffabdffe333c21b2fce9b1e0dc44d8af2ffe0b13","observation_id":"9a0aec72-8231-4b3e-83b2-5f25bb3404a8","resolution":{"observed_at":"2026-08-03T12:59:22.872952Z","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":"2026-08-03T12:59:22.994252Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:22.994252Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:d83a17eea10f1ece86caacfedbcffa8dff1e0d90c0811960124a14a1d723af39","observation_id":"8a299653-5831-487f-b786-6601194fc2b2","resolution":{"observed_at":"2026-08-03T12:59:22.994252Z","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":"2026-08-03T12:59:23.156109Z","title":", keywords =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.156109Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:5baefba92db83f1794e2b01bae71f951494626831e66734272b57d7969516c11","observation_id":"9fafea7a-2dee-44ac-82d9-e94e582bb418","resolution":{"observed_at":"2026-08-03T12:59:23.156109Z","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":"2026-08-03T12:59:23.322134Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.322134Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:67f2569e3b4893d3ac4ebd8f10d629110713240b1c80ec566eef3424b0627061","observation_id":"b84d90c7-15ea-43e3-bbc4-246963b04679","resolution":{"observed_at":"2026-08-03T12:59:23.322134Z","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":"2026-08-03T12:59:23.434653Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.434653Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:85b360acbd487dba006c2bb0e7eb7ede3dc67e8543aab71ec58927d8b563152f","observation_id":"f92b862d-b2fb-4ef2-a789-090db61c323d","resolution":{"observed_at":"2026-08-03T12:59:23.434653Z","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":"2026-08-03T12:59:23.581563Z","title":"Earth and Planetary Science Letters , keywords =","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.581563Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:3f1dfa2ee2e538e522621a5ed2aa1ef3fbc776d72f069ab472c61ca6b16993e6","observation_id":"6e66b3c8-6936-4f2c-8025-3012d663ec66","resolution":{"observed_at":"2026-08-03T12:59:23.581563Z","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":"10.1088/1742-6596/440/1/012014","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Journal of Physics Conference Series , year = 2013, series =","venue":"Journal of Physics Conference Series","work_id":"9ba6534c-47a6-4f1c-8533-151ce2414451","year":2013},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.673685Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:063337b7780fb9aae3a5ecb0ea45d7424584bc127c1693bba7bc2c47bb18d6a4","observation_id":"9ce66458-743a-4d1c-9d5c-8a37cc3a09f8","resolution":{"observed_at":"2026-08-03T13:03:27.503929Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.14861","last_updated":"2025-07-20T08:07:36Z","snapshot_observed_at":"2026-08-17T20:08:42.494972Z","submitted_at":"2025-07-20T08:07:36Z","title":"Evolving magnetic lives of Sun-like stars. I. Characterisation of the large-scale magnetic field with Zeeman-Doppler imaging","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.14861","snapshot_observed_at":"2026-08-03T12:59:23.857991Z","title":"Characterisation of the large-scale magnetic field with Zeeman-Doppler imaging","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:23.857991Z"},"links":{"cited_paper":"/paper/2507.14861","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:6ee81096cd8adbf7af8795a90da3aa9e530ec00fe341fcf1fac259d58f903040","observation_id":"09282737-dd3d-4435-aa85-be611810ca50","resolution":{"observed_at":"2026-08-03T12:59:23.857991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03388","last_updated":"2016-12-11T08:48:33Z","snapshot_observed_at":"2026-08-14T21:26:08.255302Z","submitted_at":"2016-12-11T08:48:33Z","title":"Surface magnetism of cool stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03388","snapshot_observed_at":"2026-08-03T12:59:24.057829Z","title":"Astronomische Nachrichten , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:24.057829Z"},"links":{"cited_paper":"/paper/1612.03388","citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:b43a8cfc8e8222f70aa00fbd3f5490e04e25208df8a5d537c9602ffe7bb90cad","observation_id":"06991a15-d561-4708-808f-b0d742e7be28","resolution":{"observed_at":"2026-08-03T12:59:24.057829Z","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":"2026-08-03T12:59:24.146734Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:24.146734Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:464acf995a8629d1a643d7923e812c269844552bd091cf01e9af8143680fc1ac","observation_id":"488a1c65-0ea0-484b-b64e-7219bac1343c","resolution":{"observed_at":"2026-08-03T12:59:24.146734Z","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":"2026-08-03T12:59:24.234088Z","title":", keywords =","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-03T12:59:24.234088Z"},"links":{"citing_paper":"/paper/2607.29141"},"observation_digest":"sha256:ea8c411dec81458d93b2abbf265f836533a20b69ccac9d9c54073899457b097c","observation_id":"8ce56215-d367-4314-827d-11456c1d3071","resolution":{"observed_at":"2026-08-03T12:59:24.234088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.29141","last_updated":"2026-07-31T08:11:12Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-18T13:48:06.840184Z","submitted_at":"2026-07-31T08:11:12Z","title":"Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations"},"reference_resolution":{"displayed":78,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":72,"verified_exact":6,"verified_fuzzy":0},"total_outbound_references":78},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 78 of 78 outbound references and 0 inbound Pith citation observations for arXiv:2607.29141."}