{"as_of":"2026-08-18T08:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fac0ead191283a4e6a2c9c9747d0c71f2893ab6e873dc1b606fd5d248624b1ee","coverage":[{"denominator":72,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":72,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T15:13:21.864369Z","state":"measured"},{"denominator":72,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":72,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2411.14540/citation-record","integrity":"/paper/2411.14540/integrity","json":"/paper/2411.14540/citation-record.json","paper":"/paper/2411.14540"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:23.291399Z","title":null,"venue":null,"work_id":"5ab2f2a4-c45b-46fd-a923-38ee553cffa9","year":2015},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.423001Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:869031d05aa38171ca905b266fe47c26a8d8f85c55532a3d792a19c072a6a363","observation_id":"7d087207-908d-4b3f-a6a4-b8d1503027d2","resolution":{"observed_at":"2026-08-12T15:13:23.299260Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.272855Z","title":"(1956) Harvard Announcement Card, 1340","venue":null,"work_id":"6cdb55cd-eb9e-42ce-96ac-6b8c6bc1222e","year":1956},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.429781Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f63e1fb226fd585c07ae487504e07b5a3ca3e2aa7003042f9b03f96a7825d8dd","observation_id":"4e1391bc-6413-44d5-8fd0-bcca6fd327fb","resolution":{"observed_at":"2026-08-12T15:13:23.278493Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.435519Z","title":"K., Armstrong, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.435519Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:37b1d92ee01a1ba19fa32555c0aa16773aa079b669841dda399e11e838c46c84","observation_id":"20f40dc9-6ab0-448e-93a7-f4ae788e3f63","resolution":{"observed_at":"2026-08-12T15:13:21.435519Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T15:13:23.254745Z","title":"R., Davies, B., Smith, N","venue":null,"work_id":"d3a63561-a2f0-4a51-8af5-ad79e35afcf3","year":2019},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.441781Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2db77ae64b7e8c7cf14b31af550f76de22a35252a77134a4d56f1130116e08bf","observation_id":"a897eab0-2e17-4970-b9d1-2c07e9b41584","resolution":{"observed_at":"2026-08-12T15:13:23.260634Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.1467958","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.743436Z","title":"and Ayres, T","venue":null,"work_id":"771bd0ad-5506-4989-897b-72660f76b71a","year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.449782Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:5953a3caa78d07362bcacd5bc1ddd538f372a96df7d5f6cfebe1ad7293c4e7f4","observation_id":"3f95361f-28a4-4dc2-8f05-169f35181ba4","resolution":{"observed_at":"2026-08-12T15:13:22.748692Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.238481Z","title":"D., Brown, A","venue":null,"work_id":"8c059ea9-df43-4f3b-b933-89e9d5ac7611","year":1995},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.455041Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:27f393efd89933b4052f4a63f5c9d07e89c48eab6f534a207368d6e7a8522842","observation_id":"a8784a33-f8dd-4fc4-8862-ada9ccf45e9d","resolution":{"observed_at":"2026-08-12T15:13:23.243469Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.472675Z","title":"E., Cantiello, M., Langer, N., de Koter, A., Evans, C","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.472675Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f611a47421fe58e45fb8733919d68abfaade6b82908aefc9a7545cd933e1cd17","observation_id":"bb509fed-47cd-41e7-a14c-27679f5d0823","resolution":{"observed_at":"2026-08-12T15:13:21.472675Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T15:13:23.221206Z","title":"J., Jaschek, C., Jaschek, M","venue":null,"work_id":"c393e378-dcef-4672-90e9-f62e605a1381","year":1997},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.477494Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:48ff8db48f8390134149686220b0153a0104ecec1134ca2c109f05909a03c172","observation_id":"862451db-dda9-46f5-a294-ec217eb853de","resolution":{"observed_at":"2026-08-12T15:13:23.227115Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.482302Z","title":"M., Nazé, Y ., Smith, N., Spang, A., Smoker, J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.482302Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a6d5d468e64bd0cf7e22fec8c37566c6d7705ee09d89a9c1e9072aba58012e75","observation_id":"bd0fa3a5-51d6-4634-b7bd-c17e67de74f1","resolution":{"observed_at":"2026-08-12T15:13:21.482302Z","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":"10.1086/526337","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.684544Z","title":null,"venue":null,"work_id":"954e1a7a-a12f-4e73-89f1-e12cac3522e9","year":2008},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.487233Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:10761bc31c84cad7d7dcdc86bd226b3dc1891058f887166a1d6edda8a940a797","observation_id":"f8a89819-8b21-47a8-8b45-481a3ef6a032","resolution":{"observed_at":"2026-08-12T15:13:22.690058Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.203545Z","title":null,"venue":null,"work_id":"18bc5fe8-c233-448f-8a29-15878ebebcfc","year":1965},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.493413Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2e6308d7c638915aebd614acd80aec6ac1892ce88efdc13e613931d577f31480","observation_id":"94e395ae-d8b0-45f7-a23c-66866d07ccb7","resolution":{"observed_at":"2026-08-12T15:13:23.208858Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.182754Z","title":null,"venue":null,"work_id":"80d9a3fa-1888-4df2-bf64-754946a0abd8","year":1969},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.505383Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2992abc87aef9b8736d304554b2ce06a3570c23e5c2b10a7ac2c89c7da6acdb3","observation_id":"b4e00950-c321-451f-b4d0-cf13f68da8f4","resolution":{"observed_at":"2026-08-12T15:13:23.188834Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ac5b11","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.646158Z","title":null,"venue":null,"work_id":"f5160ecb-8cc7-450d-b484-ac3d064554c5","year":2022},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.512507Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:1645a11e2478dbdf216f859c3ca7ef0e610480bc4a98fb0b4386898e2549ab74","observation_id":"b7cd5783-9bda-4ec8-b81e-9f3b196476a2","resolution":{"observed_at":"2026-08-12T15:13:22.652551Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnrasl/slad164","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.628038Z","title":null,"venue":null,"work_id":"7055d18d-9c7d-491f-9fd0-1b32bdedfef5","year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.520476Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:15652cc7dad297d9abdc4a1a95a964c17d35116d4689eedebd61b340384a2331","observation_id":"4424dbee-d5ee-4db3-b476-753f2d8986ee","resolution":{"observed_at":"2026-08-12T15:13:22.633891Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.528670Z","title":"and Izzard, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.528670Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:20b36af02ebfe5df85e1e03a60049a7b2802e768c60398e0e45be9ca7cfafa55","observation_id":"62113fa0-9160-4b4e-bc89-7bd9e1e99eb6","resolution":{"observed_at":"2026-08-12T15:13:21.528670Z","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":"2026-08-12T15:13:21.534802Z","title":"E., Langer, N., Izzard, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.534802Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:dfe99ad46a97b7d0f28cf8a4602c8cbe5c89d9077647f8089baf09f34f2cdce6","observation_id":"8db91758-1881-48a0-bcd9-83c013dcd051","resolution":{"observed_at":"2026-08-12T15:13:21.534802Z","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":"2026-08-12T15:13:21.540323Z","title":"and González-Fernández, C","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.540323Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:23cb142c62fb27ab3b7c3b0afc8afdcd799ab94ec5de516c3d196d2ff8871bba","observation_id":"b9cde3e3-9758-4daa-b071-dc2946bc722a","resolution":{"observed_at":"2026-08-12T15:13:21.540323Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T15:13:21.548649Z","title":"and Patrick, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.548649Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:7bbb4abb45f38ae1810473eb8dab4a691835b047e615d0154b0345e2844a8a61","observation_id":"65b488b0-1345-41ed-8601-594c620dc619","resolution":{"observed_at":"2026-08-12T15:13:21.548649Z","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":"2026-08-12T15:13:21.555566Z","title":"R., Dufton, P","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.555566Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:4403e95e0250d1c293c666095789c9cc88c3ca6aa41affed4c795976eba705b7","observation_id":"adc0a84b-5b64-4303-9802-22a7b9405178","resolution":{"observed_at":"2026-08-12T15:13:21.555566Z","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":"2026-08-12T15:13:21.566158Z","title":"J., Izzard, R","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.566158Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f625b39315fbab16e989beb601971ccd48114261b7b3a7383155bb3d4ef579bc","observation_id":"2c9912b1-695e-4cf1-b8d0-2d3b2a259892","resolution":{"observed_at":"2026-08-12T15:13:21.566158Z","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/ab90ff","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.551625Z","title":"M., Eikenberry, S","venue":null,"work_id":"8a5319ec-5a39-4fee-bb72-2b2f8b916698","year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.572191Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2fdff3bfb65cc3327438cd58520668aebd4aa1276f4c05d4e1894c3bf808f9f3","observation_id":"a134ff02-50c8-4001-9bc1-db5c9f0e3b4f","resolution":{"observed_at":"2026-08-12T15:13:22.556686Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.161581Z","title":null,"venue":null,"work_id":"23ca726b-9fc1-4ceb-bfd2-82b2f4540d7a","year":2008},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.578911Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f76bd94465fdb15e7727438d3ac5c9f4b63688076520605d415865b83d695864","observation_id":"a1f05e5a-e085-4000-9bac-99a8e3230a61","resolution":{"observed_at":"2026-08-12T15:13:23.168229Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.584360Z","title":"and Otero, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.584360Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:98647cf4b3c151120172ccdf0c2ee1ec42a67b751e0065bf8844d2ed06e4d9da","observation_id":"d8cf4db4-002e-4a75-bbe9-4d23d81bc28e","resolution":{"observed_at":"2026-08-12T15:13:21.584360Z","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/abbe01","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.523443Z","title":"H., Lebzelter, T., Fekel, F","venue":null,"work_id":"91d553dd-f98c-4aca-890d-ac61bd824927","year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.590268Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2382b9f091ce8bfc68f996cef329d235c3c763355b4189bc4ca675badd932be4","observation_id":"4bc599e2-cec4-45ae-ac1c-42739de5f616","resolution":{"observed_at":"2026-08-12T15:13:22.528996Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/180755","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.505653Z","title":"M., Strecker, D","venue":null,"work_id":"7b97cf03-9dd9-4471-976e-c38871579436","year":1971},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.598014Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a6f5c323947b5e8b69daa2da7f30768b4aee709b2a977d06645cceff17f6d1aa","observation_id":"62622615-ab6d-47bd-9942-a35a84f5ef4b","resolution":{"observed_at":"2026-08-12T15:13:22.510747Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.603729Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.603729Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a6507e8fa52c7ddabd68e893ef7aebc2d35104eada514ee4def640b76e7df098","observation_id":"e21c2397-f471-4998-bde6-2deea8ec6a36","resolution":{"observed_at":"2026-08-12T15:13:21.603729Z","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":"2026-08-12T15:13:23.139027Z","title":"and Jaschek, M","venue":null,"work_id":"5ec1efbb-79d6-4d08-b20b-2bdb34f91993","year":1963},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.609012Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:71af4928c02a27756bd6d45b0bba02d573393575cd577efec763768f98150845","observation_id":"65978b0e-b8d1-4cd4-8cbb-ba3769a219a3","resolution":{"observed_at":"2026-08-12T15:13:23.144985Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:23.116646Z","title":null,"venue":null,"work_id":"3a1b058d-93f5-455d-845b-e2f35c7f0fdb","year":null},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.621759Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:cd6ec4de63c7370ebb53c40eef2890abc5ec6ca4214d2a4c3b73f753177c67bf","observation_id":"6408a85f-51b9-455a-8e8f-7cd4941565a6","resolution":{"observed_at":"2026-08-12T15:13:23.122077Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.630915Z","title":"and Plez, B","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.630915Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:3c5a48c95f46fe27a597d75133e5521e9b2793106e8d134d47c0561680937e68","observation_id":"66ad3382-0969-45f8-99da-5171b01b02d8","resolution":{"observed_at":"2026-08-12T15:13:21.630915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/697/","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.445425Z","title":"L., Manoj, P","venue":null,"work_id":"c7d722b3-3dd9-47e1-a6e8-ce5e0aea9e9c","year":2009},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.637506Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:066d7db610fc7e052be2b3fd16237fbab9a9e6d1eefc5e952624b191fc168d4b","observation_id":"d359d91a-1576-44ae-b898-690355cd6126","resolution":{"observed_at":"2026-08-12T15:13:22.450882Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.642934Z","title":"A., Kiminki, D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.642934Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:d39e5679afc59a6855896e825b5997f7828c54487b337ef8f43e8d59a465de1c","observation_id":"d6bf7ee2-e6c9-4ebc-b134-89a76f36243e","resolution":{"observed_at":"2026-08-12T15:13:21.642934Z","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":"2026-08-12T15:13:21.648604Z","title":"U., Tauris, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.648604Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:651bb01b3b381511ed05cb5770f9703cea8224947de676f5bb6042aa55a7fd3c","observation_id":"7be41842-61e0-452f-89a5-0a6554ff2fb2","resolution":{"observed_at":"2026-08-12T15:13:21.648604Z","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":"2026-08-12T15:13:23.097627Z","title":null,"venue":null,"work_id":"d3da50b2-e80f-4802-a361-7a5352b2ba70","year":1978},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.655373Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:01b2394d9172fa1955e4bcfc8d2382189d73943272e7e455f4595f30334e148b","observation_id":"04501407-2a63-40b6-aa8e-57884bd18716","resolution":{"observed_at":"2026-08-12T15:13:23.103021Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.661342Z","title":"J., Mahy, L., de Mink, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.661342Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a0b21d897da3fc63282891290ae670082a6d09ab7aa40a023ed63646a00d813b","observation_id":"0e40c761-a122-4e8c-915c-ed5dee79d63a","resolution":{"observed_at":"2026-08-12T15:13:21.661342Z","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":"2026-08-12T15:13:23.069557Z","title":"(1998) A spectroscopic study of the long-period binary star WY Gemino- rum","venue":null,"work_id":"05d7664f-3fff-41d9-a39f-92d46fa3ddb0","year":1998},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.666941Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:0a34d3be0c8b897336abf7555fa98a2592fc589f8ae8bc8ab77588b4584876bd","observation_id":"22d16e32-7631-40ab-8b5b-c56b0a000cd1","resolution":{"observed_at":"2026-08-12T15:13:23.074829Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.671884Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.671884Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:0b1b92d4ceacc5bfe205e8aeda0222164c8c5ec6562eb9d6a08e297cd04ca012","observation_id":"3a020f77-7383-4921-94bf-2f002cb06b32","resolution":{"observed_at":"2026-08-12T15:13:21.671884Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T15:13:23.053596Z","title":"M., de Mink, S., Mandel, I","venue":null,"work_id":"28dd67f4-f550-43f8-bc66-ca42d78c7437","year":2017},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.677058Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f9069351421d165245b8c7463a618c386eec1bfe213b70b228e1d3c3083f71df","observation_id":"a747eb10-4c7b-4eb5-aa4c-4c24f30cf20a","resolution":{"observed_at":"2026-08-12T15:13:23.058469Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.681795Z","title":"and Frontera, F","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.681795Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:28e497a1b8d4b07dee711ed85b12b74b1ad8cc42dcdb0928ea695d6ca9559928","observation_id":"172661e1-a663-4cdc-a245-efe128be9ca7","resolution":{"observed_at":"2026-08-12T15:13:21.681795Z","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":"2026-08-12T15:13:21.692368Z","title":"and Di Stefano, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.692368Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:74ce7734cc871e860f50704440a332753f16fb3ea68e3cc55df7de94bd87db75","observation_id":"7238faf7-2b3a-4700-9e22-110ba40abf14","resolution":{"observed_at":"2026-08-12T15:13:21.692368Z","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":"2026-08-12T15:13:23.035159Z","title":"F., Levesque, E","venue":null,"work_id":"73df41e3-70c1-4e44-9296-eed7c929192b","year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.697648Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a47c34158e78e5f2b4d364fba0974ceece45cd01386503f427974fc994f8b439","observation_id":"f0c2dfd7-1cd3-4b70-bc02-4b5b7d9beed8","resolution":{"observed_at":"2026-08-12T15:13:23.041434Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.703063Z","title":"F., Levesque, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.703063Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:f564727c889898555bec1d2a77b4906f63aebecf4f02880f085d446d0024c5b6","observation_id":"510b38e7-2fda-4afc-a40b-c818118c0690","resolution":{"observed_at":"2026-08-12T15:13:21.703063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.10066","last_updated":"2022-12-07T14:47:27Z","snapshot_observed_at":"2026-08-16T03:08:16.258766Z","submitted_at":"2022-03-18T17:19:32Z","title":"The Origin and Evolution of Multiple Star Systems","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.10066","snapshot_observed_at":"2026-08-12T15:13:21.708014Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.708014Z"},"links":{"cited_paper":"/paper/2203.10066","citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:b854bac1e272af06ca08436a50a5e8e67c94231cbcf22032236132cc7bca649d","observation_id":"dd62e960-53c1-44a6-a017-5dbd15905832","resolution":{"observed_at":"2026-08-12T15:13:21.708014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.17177","last_updated":"2024-09-09T13:45:09Z","snapshot_observed_at":"2026-08-17T22:16:00.342584Z","submitted_at":"2024-06-24T23:31:58Z","title":"Binary Yellow Supergiants in the Magellanic Clouds I: Photometric Candidate Identification","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.17177","snapshot_observed_at":"2026-08-12T15:13:21.713750Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.713750Z"},"links":{"cited_paper":"/paper/2406.17177","citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:5e7e783f469a9228ce756cb2809a4127d2d4a078ef1d90496b16d5f42fb4d721","observation_id":"2babc21b-73af-49f1-8731-a3d294976a6c","resolution":{"observed_at":"2026-08-12T15:13:21.713750Z","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":"2026-08-12T15:13:23.017009Z","title":null,"venue":null,"work_id":"c6264803-fd85-4a2c-926d-52b679714fb9","year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.719234Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:58470e614d5e7deb49441e9ae6919c0061d20e62f2c4d2a41ac7f2b96ed1697c","observation_id":"ce2af0d4-3c3d-4cd4-bbb9-629091fc8389","resolution":{"observed_at":"2026-08-12T15:13:23.023207Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.724182Z","title":"R., Lennon, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.724182Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:c6d086ac47fa18d046471a99acbdcd556f5bca63045deac7265b6546adf8ffbd","observation_id":"8e656aec-a633-4af9-87a1-9090bc5c2fab","resolution":{"observed_at":"2026-08-12T15:13:21.724182Z","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":"2026-08-12T15:13:21.729195Z","title":"R., Lennon, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.729195Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:a34a79b14dcc6e672a99d4cc7e40c2e24fc060688a7a57bd3c0d2c674daacc71","observation_id":"6324e324-4d9e-42c9-b051-383520ccf47d","resolution":{"observed_at":"2026-08-12T15:13:21.729195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921322003064","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.293015Z","title":"R., Thilker, D., Lennon, D., Bianchi, L., Schootemeijer, A., Dorda, R., Langer, N","venue":null,"work_id":"f27d8482-90a4-45cb-84e5-ee1c2fb67125","year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.734532Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:93604caf1a5655a61c2639faf4a4b4c5b60289d943c640275f02bc8523bf7d62","observation_id":"dbb70c0e-6b59-41e5-aed6-caca8e2b75c3","resolution":{"observed_at":"2026-08-12T15:13:22.299942Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.740368Z","title":"R., Thilker, D., Lennon, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.740368Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:edb50d7c3efbb58f55aa3f824d5b4b3b22975d357dacef5585e2511118c55b43","observation_id":"134607e6-0826-4f71-b623-340fc8a60cb2","resolution":{"observed_at":"2026-08-12T15:13:21.740368Z","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":"2026-08-12T15:13:21.745891Z","title":"J., Mamajek, E","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.745891Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:d5e23544ed519c037cfee73aef6e9c32ca0bed1dec49402720d1a763a183c2d5","observation_id":"9bf8ff64-5aa1-4943-bc6e-b16420121bd2","resolution":{"observed_at":"2026-08-12T15:13:21.745891Z","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":"2026-08-12T15:13:21.751489Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.751489Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:e1a17d55be5c155033e2602dae131876d2c7ee90bef7eeea43cc142ab023a1dd","observation_id":"16e9d44a-cb1b-4d4a-9854-cf094f0b18dd","resolution":{"observed_at":"2026-08-12T15:13:21.751489Z","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":"2026-08-12T15:13:22.997468Z","title":"(2022) Supplementary Intermediate Report (July 2022) to the Spectroscopic Monitoring of the 2017-2019 Eclipse of VV Cephei","venue":null,"work_id":"3c966160-db7a-41b2-9461-8c6e1e77c667","year":2022},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.757981Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:0ff7e8dcbeeb4087f4eae24f0a7c8dad7efd07eb1ee6ad7f5554300f303409aa","observation_id":"8cc63255-289e-481f-8ffc-244da650ba6d","resolution":{"observed_at":"2026-08-12T15:13:23.004996Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:22.978274Z","title":"and Bennett, P","venue":null,"work_id":"3f25798a-b781-4117-b098-82d9074d1f98","year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.764337Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:5fdf6a39c47a844cb228479ac3566ed99b0ec281a949dd405a92815636e9e351","observation_id":"8b7f10c5-f7ff-4b48-91c9-9a622bcb7fcd","resolution":{"observed_at":"2026-08-12T15:13:22.984549Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.769870Z","title":"J., Baade, R","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.769870Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:655d5e8133986d1118c9c3fd64e76adce2aadac201702c150de5d43574ae054f","observation_id":"564d22f9-a82e-4d79-8f2f-a542948bf624","resolution":{"observed_at":"2026-08-12T15:13:21.769870Z","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":"2026-08-12T15:13:22.955073Z","title":"B., Friedjung, M","venue":null,"work_id":"46804bf1-b99d-4244-9dc4-0575954ff2c8","year":1992},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.774700Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:b2fe23ba34e945fc0bc63b2141e4c6c2cd82b8aa339b5220d134ef1e8301a949","observation_id":"31fee1dc-0aa2-4d19-8f38-158cfefc2323","resolution":{"observed_at":"2026-08-12T15:13:22.963376Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:22.932266Z","title":"E., de Koter, A., Langer, N., Evans, C","venue":null,"work_id":"930ab108-b696-4b9b-8f42-0338f95576f6","year":2012},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.779771Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:592aae8a115677fbce3d42501c6031f8c7ad62b0ad278617bc23a0ea6616c034","observation_id":"2f5f0e4e-3526-48ff-acae-fd1b01c8aa20","resolution":{"observed_at":"2026-08-12T15:13:22.937973Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.785239Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.785239Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:87157625ad7f1669cbc9af090be2b2dbafb5ff0a6cdb38f510e00bed7f1f79e4","observation_id":"327e1f55-dfff-4cf8-8d79-1e1b25d65783","resolution":{"observed_at":"2026-08-12T15:13:21.785239Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T15:13:22.910977Z","title":null,"venue":null,"work_id":"95cfe831-2add-4c27-8d22-658f36e2d9c7","year":2019},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.790725Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:4dd6e0a59e22d77d26f72c68a11be3ac7c14bf8c0dbc6a5d8621826eee69f7fd","observation_id":"76a4a138-e75d-4f1b-ae3b-693146cafa2b","resolution":{"observed_at":"2026-08-12T15:13:22.918520Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:22.891616Z","title":null,"venue":null,"work_id":"151a966c-2be4-44d8-84da-f34f36d12d5a","year":2007},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.796659Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:01fad12b09831819d8238057b95dad0557f87397d6839b7ba300f4d831a8e038","observation_id":"3d598d88-f37c-497f-971b-27ad5234804a","resolution":{"observed_at":"2026-08-12T15:13:22.897327Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.802753Z","title":"A., Lennon, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.802753Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:839704b9f6af16fd009071de2f416abd05fdcd3d205a2083a8a8106457e13cf2","observation_id":"59db0bba-ae30-4990-93ca-5813ce36c9a4","resolution":{"observed_at":"2026-08-12T15:13:21.802753Z","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":"2026-08-12T15:13:21.808965Z","title":"A., Gromadzki, M., Her- rero, A., Langer, N., Marchant, P., Schneider, F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.808965Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:d487e48713474835212a8cd6024b22f933bc85031a845de195294c8fcbb1b014","observation_id":"bf852767-0c53-49cd-864f-c2d9e810f693","resolution":{"observed_at":"2026-08-12T15:13:21.808965Z","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":"10.1093/mnras/sty399","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.031787Z","title":"M., Dorda, R., Negueruela, I","venue":null,"work_id":"415e2ca3-ec18-4274-8d7a-fdb817f096e5","year":2018},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.814917Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:2fa75bb8d877e9d6eaa3cb5da1f6458cc30cdf6d8450295900a631232a735355","observation_id":"98b590e8-5fe3-4138-a197-3c9a3812d179","resolution":{"observed_at":"2026-08-12T15:13:22.041513Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:22.873524Z","title":"I., Shenar, T., Bodensteiner, J., Sana, H., Crowther, P","venue":null,"work_id":"288d6e7e-aa77-4a9f-b7a1-5c2ba265420e","year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.820113Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:706cd3b4d5dbce66a2722e7858a00f3269116b92c47252ee6c85f12cd57351ae","observation_id":"a30ff8d1-5137-47ae-88f5-ec8980441059","resolution":{"observed_at":"2026-08-12T15:13:22.879887Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:21.827366Z","title":"and Hastings, B","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.827366Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:ab3f979227ca86efdf80e6fab5ea71ce49c7695d7bc2d8f2208c56e4702db53e","observation_id":"5255685e-ca27-477a-8ec2-6ba9d15e17ea","resolution":{"observed_at":"2026-08-12T15:13:21.827366Z","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":"10.1093/mnras/161.4.427","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:21.995222Z","title":null,"venue":null,"work_id":"8413bf61-9b66-4e24-93f9-a43f87d74896","year":1973},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.833521Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:051958a09a90b6ec7710aa1614c9b944674ea0b291085057a5465cc67b38a68c","observation_id":"aaf2671b-3f5b-45b5-bc34-330939f35404","resolution":{"observed_at":"2026-08-12T15:13:22.003251Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201731569","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:21.972856Z","title":"J., Arroyo-Torres, B., Chiavassa, A., Guirado, J","venue":null,"work_id":"7556cd0b-52b3-4053-85ba-bb7a9df2d3ae","year":2017},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.840035Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:8ab47a78482a074b62f52673dda10393ad41f29c07e7a2753b5f5ab0a82f158e","observation_id":"3764328f-4eb8-415c-bef8-e39d92594bad","resolution":{"observed_at":"2026-08-12T15:13:21.979955Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201629349","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:21.954531Z","title":"M., Abellan, F","venue":null,"work_id":"db61248f-6a52-46a9-bbcd-a8565bc01832","year":2017},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.846363Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:0caaba3212b2b7fcbe26c46affdeea850bd5ec8d7394ad5e9b0a679b115ba722","observation_id":"d064db14-50b2-4709-a58f-68dcaa1c767b","resolution":{"observed_at":"2026-08-12T15:13:21.960612Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/0083-6656(70)90038-3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:21.934331Z","title":null,"venue":null,"work_id":"bc0323e6-da1c-43e3-8f56-1c43931643bc","year":1970},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.852460Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:6cfb49f5d9619c74e47f53567621a08170f8434757736a3f89090ba4358fe54d","observation_id":"25b7098e-c94b-427f-a7cb-46dfe346f54e","resolution":{"observed_at":"2026-08-12T15:13:21.940901Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+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":"2026-08-12T15:13:22.855395Z","title":null,"venue":null,"work_id":"81a7f942-78b0-45b2-9420-bcfce3ccada1","year":1977},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.859211Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:22278ba2bb5a51d633f30d398004e4d03a353f788603a6ad7df268db5e2aabcc","observation_id":"a921bdf2-336c-4072-ab38-f8520a6cecc9","resolution":{"observed_at":"2026-08-12T15:13:22.861038Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.02655","last_updated":"2024-11-04T22:44:07Z","snapshot_observed_at":"2026-08-16T13:02:58.455840Z","submitted_at":"2024-11-04T22:44:07Z","title":"Multiwavelength study of 1eRASS J085039.9-421151 with eROSITA NuSTAR and X-shooter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.02655","snapshot_observed_at":"2026-08-12T15:13:21.864369Z","title":"M., Weber, P., Dauser, T., Berger, K., Kretschmar, P., Pottschmidt, K., Pradhan, P., Islam, N., Maitra, C., Coley, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.864369Z"},"links":{"cited_paper":"/paper/2411.02655","citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:0b5db70167d5c44a5977ec63cc09e489747e126e04a6f9c625b2690f7cefda4a","observation_id":"7a7f809a-2f2b-40eb-bc9e-021897b2d527","resolution":{"observed_at":"2026-08-12T15:13:21.864369Z","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":"10.1086/148284","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.664789Z","title":null,"venue":null,"work_id":"08efc902-8b1c-4923-b04e-28081074ad77","year":null},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":299,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.498673Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:fac8390ac7b12fd7e6840b20419cee8460fdbd3781929b655109250cb1dbb899","observation_id":"1b412070-3f46-47e2-b8b4-355cd06d58f9","resolution":{"observed_at":"2026-08-12T15:13:22.670942Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/176579","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.725879Z","title":null,"venue":null,"work_id":"3d27244d-de85-4afd-ad81-afb1bd561a1a","year":null},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":317,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.461718Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:1e01884f94da6b73b44df66273443774539b7b9f0551cc75b7c052ab551f3668","observation_id":"7cd110ce-deb7-411a-9df6-85de2089b3cf","resolution":{"observed_at":"2026-08-12T15:13:22.731053Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/128017","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T15:13:22.477511Z","title":null,"venue":null,"work_id":"5b6023c6-d224-43c8-b877-fd5c330635f6","year":null},"citing_paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems","version":1},"reference_index":509,"source":"pdf_text","source_observed_at":"2026-08-12T15:13:21.615159Z"},"links":{"citing_paper":"/paper/2411.14540"},"observation_digest":"sha256:009a7e1888ebf9d4f9a800a3c60bb2104959c71b8fdf5f05d14a40bfeecb42b4","observation_id":"405172b4-710a-40d3-831f-3fc33347fc69","resolution":{"observed_at":"2026-08-12T15:13:22.483200Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.14540","last_updated":"2024-11-21T19:14:57Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-13T05:59:07.471908Z","submitted_at":"2024-11-21T19:14:57Z","title":"Hot and cool: Characterising the companions of red supergiant stars in binary systems"},"reference_resolution":{"displayed":72,"state_counts":{"malformed_identifier":12,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":34,"verified_exact":16,"verified_fuzzy":10},"total_outbound_references":72},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 72 of 72 outbound references and 0 inbound Pith citation observations for arXiv:2411.14540."}