{"as_of":"2026-08-17T15:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5d6ff45b967533b299dabc15aadaa1e085254fae101efba87c15205a04c2c75d","coverage":[{"denominator":37,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":37,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T16:35:05.487708Z","state":"measured"},{"denominator":37,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":37,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+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/2412.09986/citation-record","integrity":"/paper/2412.09986/integrity","json":"/paper/2412.09986/citation-record.json","paper":"/paper/2412.09986"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.295860Z","title":"2021, Reviews of Modern Physics, 93, 015001, doi: 10.1103/RevModPhys.93.015001","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.295860Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:76632e3cce80de7472aea961dc3438bfb362de6a61ad1b8d5498b58570025138","observation_id":"4a23ec42-0595-4399-bc02-a1632b8a86d1","resolution":{"observed_at":"2026-08-11T16:35:05.295860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:06.095985Z","title":null,"venue":null,"work_id":"e57cf7b3-333a-497c-8ddd-bed7eb7ccddf","year":2010},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.302665Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:2caee49811093b8fe921ca23e43ef89efa10347998bb703ded0f530dee868994","observation_id":"b1e46a30-4a98-496d-9a3e-770993d18118","resolution":{"observed_at":"2026-08-11T16:35:06.101364Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-11T16:35:05.308190Z","title":"2003, Science, 300, 1926, doi: 10.1126/science.1084993","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.308190Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:2eceb9b7e7a4dae4407092da0b00e30689511e34ec610266862fbd23ff98b3ef","observation_id":"0c2bb246-09f6-4e52-8673-053b61442871","resolution":{"observed_at":"2026-08-11T16:35:05.308190Z","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":"2026-08-11T16:35:05.314782Z","title":"C., Brun, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.314782Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:5c2f2bb7ef512eac0a581196eb96595692140ec64fb0384f9dec971ee8df81f5","observation_id":"4f3d26a0-4e40-4633-89bd-50c918c4ad98","resolution":{"observed_at":"2026-08-11T16:35:05.314782Z","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":"2026-08-11T16:35:05.320726Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.320726Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:2fd9c53d48787331a2d901b5f03b8ec3ffee4d26c2a8e6cb4df6eed7914a598a","observation_id":"0921c408-8be4-4248-8aee-42713d8db8f7","resolution":{"observed_at":"2026-08-11T16:35:05.320726Z","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":"10.1051/0004-6361/201321779","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.878582Z","title":"I., & MiMeS Collaboration","venue":null,"work_id":"0dad8f4d-1460-4ea0-8f93-ca5d7f88b5f4","year":2013},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.324994Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:71778c7bb4cb2eb9914de4ab6714b02ac62161b231855b0ef16466c61b0afddf","observation_id":"57ce0e23-37bb-4e02-88fe-1b18c782d07b","resolution":{"observed_at":"2026-08-11T16:35:05.883999Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.972975Z","title":"2012, MNRAS, 427, 483, doi: 10.1111/j.1365-2966.2012.21933.x","venue":null,"work_id":"6264c0b2-ae85-431b-9777-ca3735e248e5","year":2012},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.329860Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:01f5638a1ce5b33021b233c8774791ca88a5ed3d272c614efe75ce768061c6c9","observation_id":"54cbc8d1-f470-42a0-ad59-528eed557a4f","resolution":{"observed_at":"2026-08-11T16:35:05.977519Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-11T16:35:05.338601Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.338601Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:590a76393ba03dc3692aa6286459250dfca59540f7307402a3cd906b0aa46bd4","observation_id":"3ffa80a4-26e3-4eef-9383-b370383a2156","resolution":{"observed_at":"2026-08-11T16:35:05.338601Z","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":"2026-08-11T16:35:05.343012Z","title":"S., Browning, M","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.343012Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:5997e58e0eb0b0373fd135b05800d197af9b94e71f401df6813610635b927f02","observation_id":"61e40749-2dc4-472c-8f6c-a144beaa12c2","resolution":{"observed_at":"2026-08-11T16:35:05.343012Z","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":"2026-08-11T16:35:05.348246Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.348246Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:ce61d53a7ad53fc4826ad4dfc0bb25457a92b009c3f304df6eda97ab070d8eb3","observation_id":"0c9d9e75-ebc4-4478-b005-d44f1aa8f738","resolution":{"observed_at":"2026-08-11T16:35:05.348246Z","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":"2026-08-11T16:35:05.352442Z","title":"M., Michielsen, M., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.352442Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:ccee74732de4e9f6713e9114c3059be637bd43e5010feeafe5f3528cae72fee4","observation_id":"b00368f3-f9a0-4dc7-b15e-b1a27a87b4f2","resolution":{"observed_at":"2026-08-11T16:35:05.352442Z","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":"2026-08-11T16:35:05.356837Z","title":"M., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.356837Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:4119000a4ad579d292f1963c798b6b16f534fd5e29111cc89bc58f1006a3f28d","observation_id":"4fde177a-6f0a-436f-a767-4bb9c02eac73","resolution":{"observed_at":"2026-08-11T16:35:05.356837Z","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":"10.1051/0004-6361/201731012","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.804350Z","title":"2017, A&A, 605, A104, doi: 10.1051/0004-6361/201731012","venue":null,"work_id":"c26f41b2-1100-4c46-b2dd-a371d54e09fc","year":2017},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.361715Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:817feea26359e877ea90f656b49d48aa3989f10aedb096928d26401f707a7274","observation_id":"d090ba53-0415-4eff-b4d5-6ed71092946f","resolution":{"observed_at":"2026-08-11T16:35:05.808330Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-11T16:35:05.368300Z","title":"2023, SSRv, 219, 35, doi: 10.1007/s11214-023-00980-0","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.368300Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:045f583051cce438661761efffb7d26531dc532dade4e781a72f5d5d4e7a1297","observation_id":"866bac9c-e0ff-4b2c-b514-93bc32f69a7e","resolution":{"observed_at":"2026-08-11T16:35:05.368300Z","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":"2026-08-11T16:35:05.374788Z","title":"2016, The Astrophysical Journal, 818, 32, doi: http://doi.org/10.3847/0004-637X/818/1/32","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.374788Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:0929a3ec4b7507668a6685a7c1f1f41d717a38989f1c35523d06734bc515c2b6","observation_id":"dfa1a972-5ce4-4cde-8f4a-9c38005e48a6","resolution":{"observed_at":"2026-08-11T16:35:05.374788Z","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":"2026-08-11T16:35:05.380297Z","title":"2009, ApJ, 705, 1000, doi: 10.1088/0004-637X/705/1/1000","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.380297Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:9eced7870e5bf6dfb3fd18c802efb606812fb1c88bddeb8b6e1e18a93af234ea","observation_id":"1905dc27-6875-4fe7-ad5b-c61c30ac35a2","resolution":{"observed_at":"2026-08-11T16:35:05.380297Z","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":"10.1088/1742-6596/271/1/012068","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.751600Z","title":"2011, in Journal of Physics Conference Series, Vol","venue":null,"work_id":"37dd4a08-1e74-4f04-b694-adad3be81cb2","year":2011},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.384313Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:681e1c93c9910e815d983b1bca6b5bdade6d93f8cff9d6b4327efc6ffb430f01","observation_id":"5a6f5d83-e38b-4bed-9e58-4d1d432387c1","resolution":{"observed_at":"2026-08-11T16:35:05.757618Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.6522806","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:05.728567Z","title":"A., Edelmann, P","venue":null,"work_id":"fd58642f-c403-42bc-8233-3d4373a00ffe","year":2022},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.389149Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:1fdc1045cfcd73c54a35fb983149192fe11c57c4bb2060fa5f1887a0c299bd37","observation_id":"c73866a6-8c8b-4f7a-889b-a638c0482af9","resolution":{"observed_at":"2026-08-11T16:35:05.735969Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-11T16:35:05.394728Z","title":"M., & Van Reeth, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.394728Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:a0a298d3debcb7092e353c536f9a21516aeaaab823fff03605bb6de02643ca1e","observation_id":"67e1a048-8c55-464b-8978-335ce2b801ff","resolution":{"observed_at":"2026-08-11T16:35:05.394728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T16:35:06.080175Z","title":null,"venue":null,"work_id":"24552449-6031-4ef2-9f54-e90f24bf05a7","year":2016},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.400853Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:f78c9fa86be1a73e7a20e80996de5deb48aedee9c4b60f6b7566f29fb36c3394","observation_id":"07abecaf-1961-4718-aa0c-e0df18a43354","resolution":{"observed_at":"2026-08-11T16:35:06.083854Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-11T16:35:05.405649Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.405649Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:e074449cdb5184e9fcae594a99594773d06ccabf893242b0dc245470caefad32","observation_id":"267f8467-f0d6-423c-a5ea-5b24bbe2479d","resolution":{"observed_at":"2026-08-11T16:35:05.405649Z","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":"2026-08-11T16:35:05.412244Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.412244Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:5bf76c2f56051b3d6a7b9eeb4b1f25e2d535f96f75ae68b0e0a9bcfc83ee697e","observation_id":"3b7db824-0b06-4219-a23e-962aab9b9757","resolution":{"observed_at":"2026-08-11T16:35:05.412244Z","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":"2026-08-11T16:35:05.419238Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.419238Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:c05cc06f5576cf3a5ecba0c83fea3f3e381a0756a8c0cb1f7fb3ede0ea27ca4d","observation_id":"aa274870-d106-4675-9f0e-1c7d8f6d70ff","resolution":{"observed_at":"2026-08-11T16:35:05.419238Z","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":"2026-08-11T16:35:05.422581Z","title":"2015, A&A, 580, A27, doi: 10.1051/0004-6361/201425290","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.422581Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:aff4e23cdbdd310809d0691f3d893b5caa79ba67e5f37db73d766b39d8777742","observation_id":"9da3a2f4-3cbb-4dd6-9756-3919e759800a","resolution":{"observed_at":"2026-08-11T16:35:05.422581Z","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":"2026-08-11T16:35:05.425967Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.425967Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:d52b743349db2377ba9242a77e8d3418f43e3a3267699cfb7a1508fd73b023a9","observation_id":"edd9e56a-0217-4131-a2dd-07014be81f7f","resolution":{"observed_at":"2026-08-11T16:35:05.425967Z","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":"2026-08-11T16:35:05.429713Z","title":"2011, ApJS, 192, 3, doi: 10.1088/0067-0049/192/1/3","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.429713Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:32caf537c55a89acec00d55767950c907885e92b9c9dfc0b80021aebccbf9687","observation_id":"4f530bb7-96d5-4efb-a2b4-7713d9321575","resolution":{"observed_at":"2026-08-11T16:35:05.429713Z","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":"2026-08-11T16:35:05.436396Z","title":"2013, ApJS, 208, 4, doi: 10.1088/0067-0049/208/1/4","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.436396Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:1bbdb672e73b286970ec97b56bffb9aa347d9a3096bd4ceb79cf7a7120f4d278","observation_id":"5c27020e-4fb2-442f-9267-b773e0d45072","resolution":{"observed_at":"2026-08-11T16:35:05.436396Z","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":"2026-08-11T16:35:05.444116Z","title":"2015, ApJS, 220, 15, doi: 10.1088/0067-0049/220/1/15","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.444116Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:15e658a38c558df33cc0f0ea2a4455de741c8da4228b99397e677c2a34b4601b","observation_id":"7a39a8bc-87f1-4421-a9e9-4cfff87794a6","resolution":{"observed_at":"2026-08-11T16:35:05.444116Z","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":"2026-08-11T16:35:05.450215Z","title":"B., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.450215Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:d17a6786d1bd7a3c064a92c136e715dcdd2dac782399cd22f61e3db781e960fa","observation_id":"51161b39-27cf-420e-b00b-001acf1b8961","resolution":{"observed_at":"2026-08-11T16:35:05.450215Z","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":"2026-08-11T16:35:05.455248Z","title":"2019, ApJS, 243, 10, doi: 10.3847/1538-4365/ab2241","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.455248Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:e4a8f4eaf03aa192e4cd98ecb1ac81d4cea2f1a3c25a852b8d915217b2d1ca59","observation_id":"87be1c35-9be5-49c7-a761-9ca559bf7f64","resolution":{"observed_at":"2026-08-11T16:35:05.455248Z","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":"2026-08-11T16:35:05.460229Z","title":"G., Aerts, C., P´ apics, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.460229Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:dee2910d18e364714fb8f88732aadd02446ec9f1026912f43ddcd8c3d044b8b6","observation_id":"17846aa3-e719-41b6-96b6-ccbdbf62cf4b","resolution":{"observed_at":"2026-08-11T16:35:05.460229Z","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":"2026-08-11T16:35:05.465764Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.465764Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:66c853e086f8412fc5bd99cb04aeb64943a683274890da2d950fb26af621325e","observation_id":"18b306fa-5623-46b9-a723-412649e4e380","resolution":{"observed_at":"2026-08-11T16:35:05.465764Z","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":"2026-08-11T16:35:05.469191Z","title":"2019, A&A, 627, A64, doi: 10.1051/0004-6361/201935462 8 Ratnasingam et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.469191Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:450e159a34334256cd2e3e1b3fcff28e19376565800f8b58046215f50e7d5b41","observation_id":"041ea30e-491a-4eee-8ae5-2c02740a03ae","resolution":{"observed_at":"2026-08-11T16:35:05.469191Z","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":"2026-08-11T16:35:05.475200Z","title":"2020, A&A, 636, A100, doi: 10.1051/0004-6361/201937398","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.475200Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:2ee5b8ab4dfdc01be0519ace0f93b51e5501890689eb23b423480217dcdac73c","observation_id":"25eac92d-0d87-4fac-9c96-1fe7a5d9f061","resolution":{"observed_at":"2026-08-11T16:35:05.475200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907138","last_updated":"1999-07-12T10:20:36Z","snapshot_observed_at":"2026-08-11T19:31:48.421086Z","submitted_at":"1999-07-12T10:20:36Z","title":"Differential rotation and magnetic fields in stellar interiors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907138","snapshot_observed_at":"2026-08-11T16:35:05.478946Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.478946Z"},"links":{"cited_paper":"/paper/astro-ph/9907138","citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:662b83b00bceff9fd075c0b53685ec66698ed5cc778325aaa877f6798d30b348","observation_id":"c9665ea9-bdf9-4b37-be3c-4533ef6675c2","resolution":{"observed_at":"2026-08-11T16:35:05.478946Z","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":"2026-08-11T16:35:05.483267Z","title":"2021, MNRAS, 503, 5894, doi: 10.1093/mnras/stab683 Van Beeck, J., Prat, V., Van Reeth, T., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.483267Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:76942da7b2dadb200388a661d2ee6e3c30fe08420ce4dcdecf1478b797d85373","observation_id":"c0051163-6a08-4106-a656-c4885062a525","resolution":{"observed_at":"2026-08-11T16:35:05.483267Z","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":"2026-08-11T16:35:05.487708Z","title":"P., Brun, A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T16:35:05.487708Z"},"links":{"citing_paper":"/paper/2412.09986"},"observation_digest":"sha256:5b187e3718be47d4d96f418c5c3e3214a12d4253780db0c3db3bfba241bafe60","observation_id":"1cc23e2d-53b4-4b1c-b3f2-ae03beb0d6c2","resolution":{"observed_at":"2026-08-11T16:35:05.487708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.09986","last_updated":"2024-12-13T09:11:45Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-17T13:58:26.726482Z","submitted_at":"2024-12-13T09:11:45Z","title":"On the Geometry of the Near-Core Magnetic Field in Massive Stars"},"reference_resolution":{"displayed":37,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":32,"verified_exact":5,"verified_fuzzy":0},"total_outbound_references":37},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 37 of 37 outbound references and 0 inbound Pith citation observations for arXiv:2412.09986."}