{"as_of":"2026-08-16T08:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2097dbef9d107b6d5f1183cdf3dd413c70584becaf9dc6a3217f49d36677e84c","coverage":[{"denominator":44,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":44,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:26:02.162586Z","state":"measured"},{"denominator":45,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":45,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T15:19:16.841735Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.09110","snapshot_observed_at":"2026-08-15T15:19:16.841735Z","title":", keywords =","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"2608.00968","last_updated":"2026-08-02T03:47:11Z","snapshot_observed_at":"2026-08-15T15:11:51.522640Z","submitted_at":"2026-08-02T03:47:11Z","title":"First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir","version":1},"reference_index":118,"source":"arxiv_source","source_observed_at":"2026-08-15T15:19:16.841735Z"},"links":{"cited_paper":"/paper/1908.09110","citing_paper":"/paper/2608.00968"},"observation_digest":"sha256:b1b0c918a1f138da9414193881836352abe28263d68d799ac691edffde680226","observation_id":"1acc562a-ccf5-4627-baaa-35d7858cb55b","resolution":{"observed_at":"2026-08-15T15:19:16.841735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.09110/citation-record","integrity":"/paper/1908.09110/integrity","json":"/paper/1908.09110/citation-record.json","paper":"/paper/1908.09110"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.484749Z","title":"D., Stine, P","venue":null,"work_id":"00b1fee0-2f43-4f8d-be9b-2d98b438fae2","year":1988},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.048431Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:ba42de9d679e2a0366b8c2092a2747497e0e8eefcfcbc0ff496425c575662f70","observation_id":"186411c8-d503-441b-93d3-efa25e6a67db","resolution":{"observed_at":"2026-08-14T11:26:02.487385Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.477314Z","title":"A., Sundqvist, J","venue":null,"work_id":"456ef297-dfb3-4566-9331-12148af4b86d","year":2015},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.052164Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:5effc780b2ba9c2b1f5ec7f81eff9702c705a7f50554c34b737e0f22bd2c592d","observation_id":"29438ba5-c983-49f7-a4cf-6504565d5b7c","resolution":{"observed_at":"2026-08-14T11:26:02.480001Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.470294Z","title":null,"venue":null,"work_id":"54114bf6-2896-48cd-8f1f-871ecb2040d5","year":1971},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.055008Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:5d902ced4a1a752a72a6e10e7a66713bfaf20cd252333e9f7e627f927a4ce9f8","observation_id":"666886dc-2ad7-4341-8357-8cea90e51400","resolution":{"observed_at":"2026-08-14T11:26:02.472743Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.462411Z","title":null,"venue":null,"work_id":"7b22f556-c297-4961-8020-f91d789cc716","year":2018},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.058302Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:82584d5fce8c5f24d89205d1282258ffcfef70d8ecad14a39d7709d461ccd3f9","observation_id":"8303405d-5130-4890-a070-1dc2df3f1c26","resolution":{"observed_at":"2026-08-14T11:26:02.465359Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.454623Z","title":"E., et al","venue":null,"work_id":"7a319b6a-1ca5-4577-9e3c-72fcda32bb95","year":2019},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.061395Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:ce1c0f644f5e409764f212f6d87e2e9386d87e9dac87c352c05706cf52b1ce14","observation_id":"c9dc5743-51eb-4b1f-8dbd-7db63bdc7e3c","resolution":{"observed_at":"2026-08-14T11:26:02.457349Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.447132Z","title":"A., Abbott, D","venue":null,"work_id":"ab86c327-2153-49d1-bf90-c31f4ac7e945","year":1987},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.064357Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:b9cc501d2756d1aee458e6625bac683880bebf96a5288c876123d80a37313efc","observation_id":"52a6e8fa-b21b-466a-9c85-abb1641d25db","resolution":{"observed_at":"2026-08-14T11:26:02.449755Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.439615Z","title":null,"venue":null,"work_id":"e4c1af5b-6aa5-4ab9-8fc5-0e32d2e6fb8e","year":2019},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.067450Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:15b1b8d2a801a53691695d93bc54ba29948bcc013c591e7b574d68833ed4962a","observation_id":"898a3f4a-a767-499b-af45-b9783bb6aa97","resolution":{"observed_at":"2026-08-14T11:26:02.442346Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.431872Z","title":"G., et al","venue":null,"work_id":"82b4601c-89bd-4dc2-8bbf-50952f25e074","year":2006},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.070141Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:af5251fd2594b89eed92348815439e88143b4c4c5977fdaf7decc8061d28516a","observation_id":"c34b6cf5-aa3d-4df4-9c6a-f7b41fbf41a9","resolution":{"observed_at":"2026-08-14T11:26:02.434726Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.424485Z","title":"2007, ApJ, 663, L25","venue":null,"work_id":"a1037fc3-fb94-4f40-8379-ff52a6e1fe16","year":2007},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.072526Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:5b0a1368e14b5a9ac7e72096e90aa7fb76097fe3be2fc4c21d40fe4e6bbecf53","observation_id":"127926ca-eb6b-4e52-8281-86fb23117001","resolution":{"observed_at":"2026-08-14T11:26:02.427104Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.075195Z","title":"G., et al","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.075195Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:7604c6b0a6ea83094fbc68d82e57ef7f2b4c9bbddb74145132969a645231bdd8","observation_id":"a1d80212-b30c-48a1-a670-47ff612bbc49","resolution":{"observed_at":"2026-08-14T11:26:02.075195Z","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":"2026-08-14T11:26:02.077861Z","title":"P., Cotter, G., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.077861Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:95fc3c8a045d3bc61c9685fb67bcc067acf92a160fbef43a6c365d6c2fce66bb","observation_id":"df5c6146-c52d-4f45-9a70-6f82193d37bf","resolution":{"observed_at":"2026-08-14T11:26:02.077861Z","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":"2026-08-14T11:26:02.080570Z","title":"M., Hallinan, G., Pineda, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.080570Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:9d6fd2868dbeea7cff7c7fa54869609bb9e91c01cfc1dcb62d705dc31b8d9f76","observation_id":"76de9527-5e43-46e8-999d-12e60c609a86","resolution":{"observed_at":"2026-08-14T11:26:02.080570Z","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":"2026-08-14T11:26:02.405090Z","title":"2006, A&A, 450, 763","venue":null,"work_id":"70e1c7d6-4ac3-43c6-8212-c199a4cdc7b2","year":2006},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.083195Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:fc6f59065974da4758d44691216ce963e85fbd4ee3436afc25669bc4ac97f729","observation_id":"48fcfb72-2a75-416e-b256-64cb15dab981","resolution":{"observed_at":"2026-08-14T11:26:02.407936Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.396996Z","title":null,"venue":null,"work_id":"0f27eebd-3486-48f7-a4de-7ec9fc84dd7f","year":2014},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.085879Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:db06b37fe0486083289aa986da6e5c97840d64bae2db045cfe3a76aaf49272f7","observation_id":"077bc877-b61c-4403-b7e6-ca23f53b09cf","resolution":{"observed_at":"2026-08-14T11:26:02.399980Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.389546Z","title":"D., et al","venue":null,"work_id":"76e8b09c-97f3-4a54-a54b-37f91980b41f","year":2017},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.088433Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:f30df2cacb1da0f6225af7820856699f22d934373e46c5f706c28c73a0d79734","observation_id":"4663d934-b159-42e7-a53b-5eafa6bce926","resolution":{"observed_at":"2026-08-14T11:26:02.392311Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.381792Z","title":"D., Bagnulo, S., Andretta, V., et al","venue":null,"work_id":"6a7b86fc-556b-4731-96cb-581b527414d5","year":2007},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.091362Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:0a99f0e43e52d8bba4fd0dfd49839ce806575c295692c53513d6843bfacd5df3","observation_id":"1fab68ae-6680-4202-a29b-c683ce0c3104","resolution":{"observed_at":"2026-08-14T11:26:02.384703Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.374534Z","title":"R., Kaplan, D","venue":null,"work_id":"2bb0f1e9-20aa-422c-861d-e408291bc5e7","year":2018},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.093900Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:93da459718de013d0deccec0eccd63b2599ccd8546451d6e3393c458132ff9ce","observation_id":"c2b6fa7b-2657-44c0-8bdc-0a84b093924f","resolution":{"observed_at":"2026-08-14T11:26:02.377188Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.367278Z","title":"2004, A&A, 423, 1095","venue":null,"work_id":"b028fd61-ec21-450c-8591-438047ee5ab2","year":2004},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.096380Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:2e4a3b8f63f00687fe3e653482f3415068b28a303b1769668968c3cae5532ba6","observation_id":"4c002475-45d3-47f7-a0b6-39de31de8791","resolution":{"observed_at":"2026-08-14T11:26:02.369834Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.098969Z","title":"S., Umana, G., & Leone, F","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.098969Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:2fba5e9fe14fce50730bdb2f76f4eccef970a6db32bf5cb3c000b59541b3da52","observation_id":"f6f57db5-99f1-4622-afb7-9ed26e71e607","resolution":{"observed_at":"2026-08-14T11:26:02.098969Z","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":"2026-08-14T11:26:02.356036Z","title":"S., Leone, F., & Umana, G","venue":null,"work_id":"854146f6-7162-45bf-9d3e-543b291546f0","year":2012},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.101657Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:bee2b2ff304a2d012f8e4812cabedde4042a679c138b7c058f5100bb8b589734","observation_id":"c77e2d8c-f36e-4c6c-9235-29baf86f5192","resolution":{"observed_at":"2026-08-14T11:26:02.358786Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.349194Z","title":"S., et al","venue":null,"work_id":"077b7580-c981-4da5-a09c-df38d5a31913","year":2016},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.104201Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:b85ddc5fb25c0fcbd668c5695b7d911faad38c9e4a9db218a840fc85d42d43ca","observation_id":"dc4b5b1c-76ba-4897-ac19-f01a44de1a3b","resolution":{"observed_at":"2026-08-14T11:26:02.351748Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.341692Z","title":"2017, MNRAS, 467, 2820","venue":null,"work_id":"eea6a498-2472-4c3d-ba6e-0cd749902957","year":2017},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.106757Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:6e305a6958605b863bcab029ce639f7b4feefcdfca9649b9178afbea79b630d9","observation_id":"a1525abb-127d-429c-ad6a-b6bdf3cebb6e","resolution":{"observed_at":"2026-08-14T11:26:02.344174Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.334542Z","title":"M., et al","venue":null,"work_id":"0a93b909-5171-40f8-ba07-bc6438678d80","year":2018},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.109384Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:a40477eeeac026974da6eef57a3f47882bccb94edc7a08de827ce0d7604eb729","observation_id":"274fe2e4-515e-4b63-bda3-3f9bba5e98fc","resolution":{"observed_at":"2026-08-14T11:26:02.337195Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.327285Z","title":"M., et al","venue":null,"work_id":"c0ac6d7d-dce6-47f2-b811-a78ea418a8e5","year":2019},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.111988Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:cbf370df5e12421e17fdf4819afffe87a7488c891f71c1b920f61457e8e47f18","observation_id":"9154ecc8-3e54-4be9-b53a-178017d9819c","resolution":{"observed_at":"2026-08-14T11:26:02.330057Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.320402Z","title":"L., Drake, S","venue":null,"work_id":"5f39a775-452d-456a-80ba-332d87614088","year":1992},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.114526Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:d7c7cae8b20f011c6bc709b04d26ef7bdd9c3528374715b24089f9dd2ecab324","observation_id":"1161f29a-3d99-4d6c-ac23-776d5d201436","resolution":{"observed_at":"2026-08-14T11:26:02.323011Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.312776Z","title":"K., Bray, J","venue":null,"work_id":"5931f143-1088-4c06-a6cb-acb866eb1e16","year":2012},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.117138Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:63b3b03185f68ae4355ba69349f51c675dcd71078c1418effb1a08ddd619b70d","observation_id":"9939feca-9385-4f1f-910e-199c9ac04c84","resolution":{"observed_at":"2026-08-14T11:26:02.315546Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.304760Z","title":"P., Waters, B., Schiebel, D., Young, W., & Golap, K","venue":null,"work_id":"333d36de-f86d-4cfc-a3cf-d2ba44f0eba6","year":2007},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.119694Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:3edc05c1a334e28ca5f8ce1c75d3b7eb4aac5381bb851c0afcbec45ffc06ae22","observation_id":"697b9aad-7058-41fa-84bc-29c2e119121b","resolution":{"observed_at":"2026-08-14T11:26:02.307980Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.297243Z","title":"B., & Dulk, G","venue":null,"work_id":"3cc2e86d-19e8-42ae-acf2-3ac2541ee83f","year":1982},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.122243Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:cefa8db83e902fb677195c6c82f67a2b1dd81af3bf6c4ae2ab4db05142f476de","observation_id":"766c1b15-2744-490b-aeba-7e7c6988091c","resolution":{"observed_at":"2026-08-14T11:26:02.300140Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.290020Z","title":"B., Hewitt, R","venue":null,"work_id":"00d34c4d-c276-4897-8833-3677d2715ca2","year":1984},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.124898Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:8a1b5e721f216bbe44d817ff86ecf848e08984f37872db38e58acd94ac3ec0f7","observation_id":"62dfc8b1-03ee-4182-a3fb-8a2ec4c93e2b","resolution":{"observed_at":"2026-08-14T11:26:02.292647Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.281328Z","title":"2003, ApJ, 583, 451","venue":null,"work_id":"182b1ed9-31e8-4edc-a942-26201ec840dc","year":2003},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.127484Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:d96b7bbadeb47b2b2d2d1c5205acd50395073474bc2fa48286f40ed15199ce3d","observation_id":"8982bdf3-01d5-458d-9d8c-c101947418bf","resolution":{"observed_at":"2026-08-14T11:26:02.284569Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.273390Z","title":"P., Wade, G","venue":null,"work_id":"3879c2d7-92ea-4058-b5ed-6918bb974c4c","year":2013},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.130050Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:11ab16552f96ecc8fd52c5d9f05539c56bcec15a15fb0aa4fe20dca7f887eb03","observation_id":"9aa643ca-633d-4525-969f-ea00454e5397","resolution":{"observed_at":"2026-08-14T11:26:02.276263Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.265870Z","title":"2002, A&A, 381, 736","venue":null,"work_id":"737bf370-fae6-4ded-a831-2214b86c6ee8","year":2002},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.132642Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:af86cbb15506fa58591968c58306b1e540f0692726186650ea699f9bc37c8048","observation_id":"74437778-f66f-4619-b64d-12fe7c2851cf","resolution":{"observed_at":"2026-08-14T11:26:02.268478Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.258469Z","title":"2010, MNRAS, 408, L99","venue":null,"work_id":"923d7bf4-875f-4166-879b-8e2b3aefdcdc","year":2010},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.134911Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:e1f5aaaefde082b93346921271b41df589edb7ce1125ac084be6f6f33f222234","observation_id":"3a009489-6c73-498d-8de7-5aa22cc487f1","resolution":{"observed_at":"2026-08-14T11:26:02.261144Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.250976Z","title":"2006, A&A, 448, 293","venue":null,"work_id":"1c810b0b-ed72-498a-a444-9614c935541f","year":2006},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.137424Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:37fe9a5ad139d911ed2c242f3c882b3ca228363a6054b0d0191470411e29df52","observation_id":"77551e74-f325-439b-bb85-f5eefcba3066","resolution":{"observed_at":"2026-08-14T11:26:02.253682Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.243363Z","title":"R., Vlahos, L., & Papadopoulos, K","venue":null,"work_id":"996c48be-db12-4f86-bee7-1bfe431c4f87","year":1982},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.139893Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:bb870a7e9fe527641f8fbbd6ce9f60cd079587af6df95b33bf8d121685fd1844","observation_id":"af5b80cc-6f44-4961-bf8e-bf31b682fd10","resolution":{"observed_at":"2026-08-14T11:26:02.246100Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.235789Z","title":"R., & Vlahos, L","venue":null,"work_id":"4317244e-8a91-4472-9309-52a20e1ad152","year":1984},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.142297Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:d19bc72f811f827c9a8e1c449f80742120aa9cd019ac1939b0247e5e910b5ad6","observation_id":"1e036c6d-869b-4ca5-affe-ce9687d8424b","resolution":{"observed_at":"2026-08-14T11:26:02.238500Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.144689Z","title":"E., Wade, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.144689Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:cda64fe331911d04da79b56ffc822dd17264ff0f0ce60a52619e6a02db4df802","observation_id":"9e63e98c-b746-4ca3-92ce-1e76fb7daeb2","resolution":{"observed_at":"2026-08-14T11:26:02.144689Z","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":"2026-08-14T11:26:02.223871Z","title":"E., Wade, G","venue":null,"work_id":"be0f5798-a0f2-4e33-806f-4f265ec4ab86","year":2019},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.147595Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:a772c2dba43e55067076c799e46dd6bd43ae8c397b7a48129e59dbf0e035dc1d","observation_id":"2e28471d-ee41-48bd-921a-15bc2f9a36af","resolution":{"observed_at":"2026-08-14T11:26:02.226677Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.216261Z","title":null,"venue":null,"work_id":"b76b50c8-d055-4f28-bb30-93b914b88a72","year":2006},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.150225Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:c2b683187f4d787bc19c3a567a8b7531a5b9d96eb2e26bca5fefd4fced8bf438","observation_id":"497c0f96-1d82-43da-bf08-7016ce35c2ce","resolution":{"observed_at":"2026-08-14T11:26:02.219109Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.152821Z","title":"2000, A&A, 362, 281","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.152821Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:dc07f55e9769ad7ec9e69aee4d97e65a3285ea870bea6020c537ea50882287d3","observation_id":"0e021465-a56b-4723-a799-2e84e07cad3d","resolution":{"observed_at":"2026-08-14T11:26:02.152821Z","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":"2026-08-14T11:26:02.204134Z","title":"2004, A&A, 418, 593","venue":null,"work_id":"3b539d43-9617-4f22-9a63-5ecb09c695d4","year":2004},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.155137Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:6803d0ef351b4f0398104cf8cb241f4803591367a969a4d04ce77f61ce89d0ba","observation_id":"f83ec075-ba2c-4a98-b185-fa5bc905d8e0","resolution":{"observed_at":"2026-08-14T11:26:02.206834Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.196423Z","title":"2008, MNRAS, 384, 1437","venue":null,"work_id":"47b7c767-e269-420c-a3ca-1651346ae52d","year":2008},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.157561Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:4564ec5f09a570015c908b18eb6fdb25f456f8f52e619a790fd3eeba305e809f","observation_id":"7bae8f0d-bdff-4706-a06a-bcd131961955","resolution":{"observed_at":"2026-08-14T11:26:02.199347Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.188981Z","title":"2011, ApJ, 739, L10","venue":null,"work_id":"e2b43093-e1cc-468c-aba8-a22a2da7ac4f","year":2011},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.160145Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:4fd8b15d73dc3b4b6953be9fc4177320a1f3b7b59d23d42a7b7a51c5693eed5f","observation_id":"375f5ca8-7c88-4393-af01-3902e0f58d4d","resolution":{"observed_at":"2026-08-14T11:26:02.191787Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:26:02.180085Z","title":null,"venue":null,"work_id":"d884abcc-641f-4198-a435-d4f2bdc6fe08","year":2019},"citing_paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T11:26:02.162586Z"},"links":{"citing_paper":"/paper/1908.09110"},"observation_digest":"sha256:8152ccf591105c6142153aa95caaade2fe2dc385c042ba7a2859c795f3676030","observation_id":"82cb32c6-3282-4424-8db1-9788ad25b214","resolution":{"observed_at":"2026-08-14T11:26:02.183827Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.09110","last_updated":"2019-08-24T09:11:39Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-15T17:09:56.915322Z","submitted_at":"2019-08-24T09:11:39Z","title":"The fifth main sequence magnetic B-type star showing coherent radio emission: is this really a rare phenomenon?"},"reference_resolution":{"displayed":44,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":12,"verified_exact":0,"verified_fuzzy":32},"total_outbound_references":44},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 44 of 44 outbound references and 1 inbound Pith citation observation for arXiv:1908.09110."}