{"as_of":"2026-08-20T12:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0d592c24b7a87e3aafcc28ce13a40ac17a960c4fec666bf1b50020011118b7b1","coverage":[{"denominator":25,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":25,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T23:02:03.678018Z","state":"measured"},{"denominator":26,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":26,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T15:42:25.167784Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-07T15:42:25.765258Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"cited_work":{"arxiv_id":"2505.05962","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.05962","snapshot_observed_at":"2026-08-07T15:42:25.765258Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","venue":"astro-ph.SR","work_id":"edcbfb68-fd5d-46f2-8083-80f88c2fedd5","year":2025},"citing_paper":{"arxiv_id":"2505.14084","last_updated":"2025-05-20T08:45:31Z","snapshot_observed_at":"2026-08-11T01:23:45.156709Z","submitted_at":"2025-05-20T08:45:31Z","title":"Coronal Magnetometry with EUV Permitted Lines","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-07T15:42:25.167784Z"},"links":{"cited_paper":"/paper/2505.05962","citing_paper":"/paper/2505.14084"},"observation_digest":"sha256:b2fd6864b0a348e24e69e2cace5358e8cb5c439b93f59ff129de6d1138e50c31","observation_id":"431e35eb-b282-427e-8d89-bd054548a116","resolution":{"observed_at":"2026-08-07T15:42:25.832708Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2505.05962/citation-record","integrity":"/paper/2505.05962/integrity","json":"/paper/2505.05962/citation-record.json","paper":"/paper/2505.05962"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2409.01197","last_updated":"2024-10-13T22:21:53Z","snapshot_observed_at":"2026-08-19T09:16:25.309419Z","submitted_at":"2024-09-02T12:12:29Z","title":"A unifying polarization formalism for electric- and magnetic-multipole interactions","version":2},"cited_work":{"arxiv_id":"2409.01197","doi":"10.48550/arxiv.2409.01197","metadata_source":"pith","pith_arxiv_id":"2409.01197","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"A unifying polarization formalism for electric- and magnetic-multipole interactions","venue":"physics.atom-ph","work_id":"4aad8648-0512-4168-ab35-dfb570652874","year":2024},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.561223Z"},"links":{"cited_paper":"/paper/2409.01197","citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:0e4bcce09327acff57254d67bb53e7bbb48914bbf21f559a334b6ceeef3b4573","observation_id":"0c653971-4bba-4b6a-87a4-fe2418ba2920","resolution":{"observed_at":"2026-08-15T23:02:03.994087Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-15T23:02:03.567003Z","title":"M., & Judge, P","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.567003Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:41ae4da5db9eb74b844a08d635e18cee5e5dc1475771cf03f45782de6c104f6c","observation_id":"59ae753c-6d99-4b0c-865b-226e962b0096","resolution":{"observed_at":"2026-08-15T23:02:03.567003Z","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":"2026-08-15T23:02:04.163299Z","title":"F., Rimmele, T., Casini, R., et al","venue":null,"work_id":"71d3255d-6ee4-403b-b43d-3c27255159a2","year":2014},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.571929Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:01e6933538a30c1a07c2291e5d1ea8df69cbf51e79df94e4f8408c547ed67a13","observation_id":"5b35f648-5701-4e11-a114-534a13e7868e","resolution":{"observed_at":"2026-08-15T23:02:04.169311Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-15T23:02:03.576994Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.576994Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:2a27ac5075f6455b355beb6cec48809f72abcf25e2f606c1808c228ab85959cf","observation_id":"3ad2266c-36eb-4592-9bba-4edbeaa1ec00","resolution":{"observed_at":"2026-08-15T23:02:03.576994Z","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":"2026-08-15T23:02:03.582116Z","title":"R., Schad, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.582116Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:434c0d3757fab82ac021f0dc3ae9fac03a0cf2e33b3c77764eb644c65d48c9e0","observation_id":"31e625ee-7f37-4cbb-bd38-78d63b39c700","resolution":{"observed_at":"2026-08-15T23:02:03.582116Z","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":"2026-08-15T23:02:03.587130Z","title":"P., Ignace, R., Erba, C., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.587130Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:2577bfb3350d3c0be6e50679c1086fe20fd38c21ba8e2b6cd99b8af6583b1709","observation_id":"ee386bfb-77aa-4431-89b3-996162fb7f03","resolution":{"observed_at":"2026-08-15T23:02:03.587130Z","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":"2026-08-15T23:02:03.592523Z","title":"2016, Frontiers in Astronomy and Space Sciences, 3, 8, doi: 10.3389/fspas.2016.00008","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.592523Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:d297cda68045752dfea63d77324ff9672e8c338cb51ca53947220f3b3596840c","observation_id":"17d95c1e-4581-4e42-ae62-363d49269230","resolution":{"observed_at":"2026-08-15T23:02:03.592523Z","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":"2026-08-15T23:02:04.147642Z","title":"G., & Casini, R","venue":null,"work_id":"d038086e-a720-41eb-8017-d07323a114aa","year":2001},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.598388Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:3afaef86ab3004a1be122575019bc1831b50f3e8554c29b5a53355b3aa5c503b","observation_id":"2126c3d6-0a34-4201-8866-e9c635d6ef95","resolution":{"observed_at":"2026-08-15T23:02:04.152336Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/507982","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.918696Z","title":"G., Low, B","venue":null,"work_id":"70edd4d7-e16d-4748-b580-b7ae0a6c2a0d","year":2006},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.603101Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:db392c7932f2ec6f51716dcdcb6605901fc8b869b8a60e441ffc12afcd08940e","observation_id":"e52e5026-a4a3-464a-bcc5-caba35c11ade","resolution":{"observed_at":"2026-08-15T23:02:03.923548Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201219404","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.901568Z","title":"2012, A&A, 545, A52, doi: 10.1051/0004-6361/201219404","venue":null,"work_id":"3193d291-cdc0-46fb-8412-5c0cea4e977b","year":2012},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.608163Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:4c0a7c32f22d99f4f1e62377527d904542a4bce49d0baae7d3fa83f223cf3a21","observation_id":"9a215847-08ca-401f-9b29-4b9ca55456b9","resolution":{"observed_at":"2026-08-15T23:02:03.906493Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201015551","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.886518Z","title":"2011, A&A, 529, A12, doi: 10.1051/0004-6361/201015551","venue":null,"work_id":"bc523d67-ef64-4e1e-9357-5c30d57fcfe7","year":2011},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.612953Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:7e5a4a652426655d2221c77253228a7c6e871f03623812a4d94ae69f91b96a7b","observation_id":"057b9900-811c-4ee0-b0ea-d4466e6e7867","resolution":{"observed_at":"2026-08-15T23:02:03.891434Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201219164","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.870589Z","title":"2012, A&A, 543, A158, doi: 10.1051/0004-6361/201219164","venue":null,"work_id":"cf8814d6-3861-4592-9c85-c30524157fb4","year":2012},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.617563Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:f48ed39497da39d9b4fd45a9a0d797c68abd9c06bd44f7824d3ec49a2f70ca63","observation_id":"d121d3b3-4e75-4622-86f3-edabd9e5fd4e","resolution":{"observed_at":"2026-08-15T23:02:03.875795Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-15T23:02:03.622334Z","title":"R., & Tomczyk, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.622334Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:4fb03989274432e715d1d4e7d24a4c4d22503a284ff74e9140cc0e9aaf22b79a","observation_id":"56f032f1-4d73-4d84-b0d0-479d5fcd79b1","resolution":{"observed_at":"2026-08-15T23:02:03.622334Z","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":"10.3847/1538-4357/aa6625","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.845223Z","title":"2017, ApJ, 838, 69, doi: 10.3847/1538-4357/aa6625 Manso Sainz, R., & Trujillo Bueno, J","venue":null,"work_id":"c9097f0f-4852-437a-92ac-1b0742ff87c5","year":2017},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.626663Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:6610c8e9f973d6f5cd277d552500eef7dec96a1997bd96e5302db9fc2d169f78","observation_id":"a853ddd4-28ae-49f9-bdbe-ebb473145f54","resolution":{"observed_at":"2026-08-15T23:02:03.850053Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-15T23:02:03.631190Z","title":"E., & Casini, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.631190Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:f3764baccf4fb6cc30e61ff9ea91fc322eeeecab3167e8ef501f07a220a4cb35","observation_id":"eb7cc02f-58af-42b0-8796-7d452f2727b8","resolution":{"observed_at":"2026-08-15T23:02:03.631190Z","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":"2026-08-15T23:02:03.635756Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.635756Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:169bacba0f9acfbda7392cc65135e6ec860c588315c821207ba1eaebff825c71","observation_id":"204ed64d-7e43-432e-8b89-c55d7fc3b853","resolution":{"observed_at":"2026-08-15T23:02:03.635756Z","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":"2026-08-15T23:02:03.640226Z","title":"2017, ApJ, 834, 10, doi: 10.3847/1538-4357/834/1/10","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.640226Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:c3473e4f56f4c77055a3a2bd670fb623918f3fcaa8068fcb2bf3e23b96bcf6f6","observation_id":"07c76d46-b980-4d94-98be-176d65d11282","resolution":{"observed_at":"2026-08-15T23:02:03.640226Z","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":"2026-08-15T23:02:03.644781Z","title":"R., Warner, M., Keil, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.644781Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:b22633ee77747a98a607360386b93b1137daa06a5904523423f33ae3af748224","observation_id":"b21a16a2-8b90-40d5-8aca-c7cee0c38a23","resolution":{"observed_at":"2026-08-15T23:02:03.644781Z","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":"2026-08-15T23:02:03.649383Z","title":"2020, SoPh, 295, 98, doi: 10.1007/s11207-020-01669-1 —","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.649383Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:c1679471a8b32f4c8d6bd74d8f1bb711094a0884bd774c2ae41bbf78f66d2301","observation_id":"5583b2d1-0b0e-4862-aea0-e7cdca9fc9d5","resolution":{"observed_at":"2026-08-15T23:02:03.649383Z","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":"2026-08-15T23:02:03.654239Z","title":"A., Petrie, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.654239Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:4005ab7f075f82c2094cc3aceaadf6550e6f9b4cab947face50a4f5f3587928a","observation_id":"ab86d33c-00bd-4b37-82c4-f9446e134596","resolution":{"observed_at":"2026-08-15T23:02:03.654239Z","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":"2026-08-15T23:02:03.659473Z","title":"T., Reames, D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.659473Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:a7826ec30daf2a7d7c3cf4a27ca2b8debc2e638e3c5556147c56393b56ac8d2c","observation_id":"897092d4-dbae-469f-8f5a-2e0e3a67f34e","resolution":{"observed_at":"2026-08-15T23:02:03.659473Z","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":"10.5281/zenodo.15195460","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.768473Z","title":"2025, P-CORONA, Zenodo, doi: 10.5281/zenodo.15195460","venue":null,"work_id":"a47b341a-0000-44e7-a34e-a220e6181976","year":2025},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.663997Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:5196c20c97df5f833555628cfea75b6a248779399b6dde0290431c07d6487e4c","observation_id":"c79863c8-e19b-4868-971f-84c9c6eb1a4b","resolution":{"observed_at":"2026-08-15T23:02:03.773241Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac1068","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.752037Z","title":"D., Trujillo Bueno, J., de Vicente, ´A., & del Pino Alem´ an, T","venue":null,"work_id":"b0149d0f-0b4a-4526-9865-d7aa28f3beb1","year":2021},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.668369Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:14b9385cda7acc6444812a9adc922a500b52e96a66b9c26ed31f5a8bd18bcabe","observation_id":"7879f7ba-5eda-4c2d-9806-e73ae3f8b5e4","resolution":{"observed_at":"2026-08-15T23:02:03.757268Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202328","last_updated":"2002-02-18T12:22:14Z","snapshot_observed_at":"2026-08-08T04:23:32.849729Z","submitted_at":"2002-02-18T12:22:14Z","title":"Atomic Polarization and the Hanle Effect","version":1},"cited_work":{"arxiv_id":"astro-ph/0202328","doi":"10.48550/arxiv.astro-ph/0202328","metadata_source":"pith","pith_arxiv_id":"astro-ph/0202328","snapshot_observed_at":"2026-08-16T12:16:17.039197Z","title":"Atomic Polarization and the Hanle Effect","venue":"astro-ph","work_id":"bdc2fbbb-38d1-422a-9055-24b0b0c2599b","year":2002},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.673021Z"},"links":{"cited_paper":"/paper/astro-ph/0202328","citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:ceeb8c5eb55e08727c9d5be31b061cab80ddd28c2d7af53587de602cb0706132","observation_id":"fa3bfae7-9d06-497d-bf80-0ea0ec82dcb2","resolution":{"observed_at":"2026-08-15T23:02:03.741504Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/415403a","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:02:03.711654Z","title":"2002, Nature, 415, 403, doi: 10.1038/415403a","venue":null,"work_id":"d3640e12-46c3-47ed-92b4-5815455d500a","year":2002},"citing_paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T23:02:03.678018Z"},"links":{"citing_paper":"/paper/2505.05962"},"observation_digest":"sha256:b2a2a151d201ddca0b948264869e30ddb956421d145b1f4761fe1c2aaf18886b","observation_id":"f8568015-8e56-494d-bc42-f5a7df8b30cc","resolution":{"observed_at":"2026-08-15T23:02:03.718217Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2505.05962","last_updated":"2025-05-09T11:22:50Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-19T21:00:37.792160Z","submitted_at":"2025-05-09T11:22:50Z","title":"P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona"},"reference_resolution":{"displayed":25,"state_counts":{"malformed_identifier":0,"metadata_mismatch":2,"parse_uncertain":0,"unresolved":13,"verified_exact":8,"verified_fuzzy":2},"total_outbound_references":25},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 25 of 25 outbound references and 1 inbound Pith citation observation for arXiv:2505.05962."}