{"as_of":"2026-08-06T09:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:edb5c0921ffb24e314b82e151b57e35d8afb03bb96655b3ce4e3b445dbf20e33","coverage":[{"denominator":297,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":102,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":102,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T00:42:42.583858Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-01T18:35:58.297524Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"cited_work":{"arxiv_id":"2606.23456","doi":null,"metadata_source":"pith","pith_arxiv_id":"2606.23456","snapshot_observed_at":"2026-07-01T18:35:58.297524Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","venue":"astro-ph.SR","work_id":"40a10851-6433-45ca-bf66-bb038987a1c5","year":2026},"citing_paper":{"arxiv_id":"2606.27468","last_updated":"2026-06-25T18:44:46Z","snapshot_observed_at":"2026-07-07T00:01:39.205208Z","submitted_at":"2026-06-25T18:44:46Z","title":"JWST Reveals Compact Nuclear Starbursts Masquerading as AGNs in Metal-Poor Dwarfs: Where Are the Accreting Intermediate-Mass Black Holes?","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-29T01:54:51.897942Z"},"links":{"cited_paper":"/paper/2606.23456","citing_paper":"/paper/2606.27468"},"observation_digest":"sha256:b64087684201143b380a1181d7eb8e05f5abf6c221ad715da036610aa6813c3b","observation_id":"82d9ea0c-1a54-469a-aa1d-3beaa77c9ba7","resolution":{"observed_at":"2026-07-01T18:35:58.298963Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.23456","snapshot_observed_at":"2026-08-01T00:42:42.583858Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.26147","last_updated":"2026-07-28T18:00:30Z","snapshot_observed_at":"2026-08-04T04:31:07.418447Z","submitted_at":"2026-07-28T18:00:30Z","title":"The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity","version":1},"reference_index":247,"source":"arxiv_source","source_observed_at":"2026-08-01T00:42:42.583858Z"},"links":{"cited_paper":"/paper/2606.23456","citing_paper":"/paper/2607.26147"},"observation_digest":"sha256:3ca6609c5f1af95041c313b19810a437969dae0851546d01728b03b77fc68831","observation_id":"657e84e7-6662-44c0-9d62-4aa6c0c34d38","resolution":{"observed_at":"2026-08-01T00:42:42.583858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2606.23456/citation-record","integrity":"/paper/2606.23456/integrity","json":"/paper/2606.23456/citation-record.json","paper":"/paper/2606.23456"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202037730","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Astronomy and Astrophysics","work_id":"71c6e8ea-d0a7-482b-9659-b446585003b7","year":2002},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:9778a1c4047de7f1afa451bdfeeb0ca7d471110b38dfc777d26c843c5c0978bb","observation_id":"01786443-2002-4603-8b60-fcc832515d82","resolution":{"observed_at":"2026-06-26T18:09:41.777829Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/422878","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal Supplement Series","work_id":"fab7126f-69dd-47d9-bd73-a5760c22faae","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:516caba1fe49a89022d4782683cd0a14d18337638efcc1d8eaa1397ed46e6776","observation_id":"c3ce19cc-5c7c-4934-8ac5-495de7d405af","resolution":{"observed_at":"2026-06-26T18:09:41.782199Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2006","doi":"10.1111/j.1365-2966.2006","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"and Yang , J","venue":null,"work_id":"7ef6cf0d-0877-424d-9dec-97ef68ca2212","year":2006},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:e561c3a2c55cc8add824c404a313259f0632a8006f9e8c37038b6cb1550c49a3","observation_id":"71654247-5225-483d-a5b5-c5e7106fc26c","resolution":{"observed_at":"2026-06-26T18:09:41.775783Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00243","last_updated":"2018-03-01T08:21:46Z","snapshot_observed_at":"2026-07-06T06:26:01.372123Z","submitted_at":"2018-03-01T08:21:46Z","title":"Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A","version":1},"cited_work":{"arxiv_id":"1803.00243","doi":"10.1051/0004-6361/201732376","metadata_source":"pith","pith_arxiv_id":"1803.00243","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A","venue":"astro-ph.SR","work_id":"1cfc65ab-8c1d-4b09-8c33-7a98da20ad3c","year":2018},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1803.00243","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:a72f799b9cb58f1c160ad821b32bb71c8e7b9fa750f56b2f6a88ebe13beb6568","observation_id":"1fce59fe-e933-40ae-843e-b344075c5347","resolution":{"observed_at":"2026-06-26T18:09:41.780945Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0901.2930","last_updated":"2009-03-25T20:19:09Z","snapshot_observed_at":"2026-07-06T01:49:41.580156Z","submitted_at":"2009-01-19T21:00:27Z","title":"The Kiloparsec-Scale Kinematics of High-Redshift Star-Forming Galaxies","version":2},"cited_work":{"arxiv_id":"0901.2930","doi":null,"metadata_source":"pith","pith_arxiv_id":"0901.2930","snapshot_observed_at":"2026-06-29T04:03:05.508931Z","title":"The Kiloparsec-Scale Kinematics of High-Redshift Star-Forming Galaxies","venue":"astro-ph.GA","work_id":"5c53273b-fbb0-454c-b56f-cd49af576d1f","year":2009},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0901.2930","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:d189add47ed3d16c7bdab20e7d62f71c5123a2ccd75f7440ecadbbf0dd0d1e08","observation_id":"0ed4f118-09d2-4d93-998f-d259337f7497","resolution":{"observed_at":"2026-06-26T18:09:41.770341Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.15571377","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.5281/zenodo.15571377 , version =","venue":"Zenodo (CERN European Organization for Nuclear Research)","work_id":"f1708e1c-3e92-455e-aa78-d32f013ba70b","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:fc6cecfa0fe07b3060420f50da516206609702ab868c8ca57bc6d154fc4f3192","observation_id":"2c9cded2-e027-4da4-8e5e-29f7bc9b7915","resolution":{"observed_at":"2026-06-26T18:09:41.774011Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/ada147","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Misselt, Karl A","venue":"The Astronomical Journal","work_id":"7a0f8e36-dc42-499a-8b86-515b9abfbb19","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:36a9b98fc1748a686c6128fbb2446b7dc0ce79505fd24e5e3812d597348e7694","observation_id":"3286fbe0-f1ef-4e29-ad3e-bd53c1933689","resolution":{"observed_at":"2026-06-26T18:09:41.762979Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/add73b","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal","work_id":"9f2c1b05-055a-4bc8-a34d-bb3f471d9e0e","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:f910735ca08e351e54c54f08fe0eadec805368792a8143dd223ba3a224f54682","observation_id":"99860663-3b98-4943-a362-0a86a9c6ba75","resolution":{"observed_at":"2026-06-26T18:09:41.778363Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ad91a6","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal Letters","work_id":"6dcc6c35-6448-4186-8292-1b851065b402","year":2041},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:be83aac279a48caa96fd3035850099ec7e984b9aefb7ddaf7d1a0caf8ac336ff","observation_id":"b8e1a39e-0229-40ba-b61d-ba3da5798b89","resolution":{"observed_at":"2026-06-26T18:09:41.784651Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202141018","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Astronomy and Astrophysics","work_id":"5de84b84-3a15-45f5-9050-1ac987a627c3","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:53e6c0470373f710c3472bae627cbd9ae42eaf76c4d06beca2de60dc489703b6","observation_id":"136bd4ca-32cd-4905-bb8a-882901c389cd","resolution":{"observed_at":"2026-06-26T18:09:41.786385Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/ac324a","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal Supplement Series","work_id":"ccadf379-c82f-4f30-9101-036ac48fb8b1","year":2022},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:6af7697cdbcfd147db127ba07586de5e193251aa18090faffa375ff09bb151e0","observation_id":"35c13b9f-b579-44f2-afdd-84b26a0aa679","resolution":{"observed_at":"2026-06-26T18:09:41.784448Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-05-24T08:53:34.359789+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T08:53:34.359789+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0067-0049/221/1/1","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"author Naz \\'e , Y","venue":"The Astrophysical Journal Supplement Series","work_id":"cbed3bf3-7e54-4253-a0e7-5786efffcc59","year":2015},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:5da2671ec22e40bb585d979f4fd9d9fc8212eac6ea99384f129aa6b8208f6c4b","observation_id":"4de76dd2-c4e3-49e9-9794-4014aa9913c0","resolution":{"observed_at":"2026-06-26T18:09:41.782800Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.03842","last_updated":"2016-04-13T15:48:12Z","snapshot_observed_at":"2026-08-02T17:57:41.243411Z","submitted_at":"2016-04-13T15:48:12Z","title":"Spectral classification and properties of the O Vz stars in the Galactic O-Star Spectroscopic Survey (GOSSS)","version":1},"cited_work":{"arxiv_id":"1604.03842","doi":"10.3847/0004-6256/152/2/31","metadata_source":"pith","pith_arxiv_id":"1604.03842","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Spectral classification and properties of the O Vz stars in the Galactic O-Star Spectroscopic Survey (GOSSS)","venue":"astro-ph.SR","work_id":"01bbc975-b366-445d-8837-cfc1cd5af74b","year":2016},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1604.03842","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:080f2e753f197ae8fa8c437b017807c53604c614d978ec068f822dad227c073a","observation_id":"9a0d053d-3af5-4b6a-963d-7b26ecd27bf8","resolution":{"observed_at":"2026-06-26T18:09:41.432093Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.01336","last_updated":"2016-02-08T16:50:09Z","snapshot_observed_at":"2026-07-06T04:45:01.522501Z","submitted_at":"2016-02-03T15:25:18Z","title":"The Galactic O-Star Spectroscopic Survey (GOSSS). III. 142 additional O-type systems","version":2},"cited_work":{"arxiv_id":"1602.01336","doi":"10.3847/0067-0049/224/1/4","metadata_source":"pith","pith_arxiv_id":"1602.01336","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Galactic O-Star Spectroscopic Survey (GOSSS). III. 142 additional O-type systems","venue":"astro-ph.SR","work_id":"1db50983-f7ee-4f5a-8b7c-4ce0d48acf0a","year":2016},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1602.01336","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:9f9912dd7ab40b8bde374884012d565fd02585890e6120aad808b3e09e65adaf","observation_id":"b3830a13-3a4a-42cd-a704-65b34f0bf7ca","resolution":{"observed_at":"2026-06-26T18:09:41.754044Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202039015","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Evidence of multiple star-forming bursts","venue":"Astronomy and Astrophysics","work_id":"e1b64e00-acea-49d1-8ae5-6dce451a5e85","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0d59d8220bec77a559a1a1fc5cf0841f1f8d7b39224b51664f1898c1b68f155f","observation_id":"b9774b3e-cfa4-4eec-99df-e9c3fa4edf5c","resolution":{"observed_at":"2026-06-26T18:09:41.737236Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0eb0b04c3d3f1ec8bb39f8b3ef9049a69a63883c5717fce85873f2d31911df39","observation_id":"ac9216e0-eb30-4e78-a489-48e4e9297ee4","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5469","last_updated":"2013-03-21T21:24:27Z","snapshot_observed_at":"2026-07-06T03:09:21.035057Z","submitted_at":"2013-03-21T21:24:27Z","title":"A Bake-Off Between CMFGEN and FASTWIND: Modeling the Physical Properties of SMC and LMC O-type Stars","version":1},"cited_work":{"arxiv_id":"1303.5469","doi":"10.1088/0004-637x/768/1/6","metadata_source":"pith","pith_arxiv_id":"1303.5469","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"A Bake-Off Between CMFGEN and FASTWIND: Modeling the Physical Properties of SMC and LMC O-type Stars","venue":"astro-ph.SR","work_id":"6c7a4f70-276c-449f-918b-eff7c42a97c0","year":2013},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1303.5469","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:b4bcebdca428a7f7f1b3aff71223a6dad152d3ccff24bd1019a4005ad40da1bc","observation_id":"bd384e7d-7553-43e9-9148-1a29860b7619","resolution":{"observed_at":"2026-06-26T18:09:41.378733Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20053522","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Astronomy and Astrophysics","work_id":"cffa2565-178b-4df0-b59d-eeb3c8459a89","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:bb3a42461e12b2a349ce842a8596f9b4bbaf8970f7e0bf4ab7747a75f8fb7005","observation_id":"e35b1b86-6435-4c13-a04f-8a94918fdb04","resolution":{"observed_at":"2026-06-26T18:09:41.292055Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Owocki, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:f5ff6ccca0c81319d751d8324c0c01c972e9a213ccdf7d6c8cd2485360400254","observation_id":"942dbac5-a55f-452a-b52a-9d44b4fb6ed1","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03500","last_updated":"2017-03-13T17:58:52Z","snapshot_observed_at":"2026-07-06T05:14:15.269065Z","submitted_at":"2016-10-11T20:00:51Z","title":"The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries","version":3},"cited_work":{"arxiv_id":"1610.03500","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.03500","snapshot_observed_at":"2026-06-29T02:33:04.062046Z","title":"The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries","venue":"astro-ph.SR","work_id":"65196484-0192-4261-817c-490977442cfc","year":2016},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.03500","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:84f1a79bd841b4a5ad5c15a39c1b07a3f56d6e0e687e6f93add5deb463a4d44a","observation_id":"9242b13f-9e79-4b3e-88ca-0ae3504fbd27","resolution":{"observed_at":"2026-06-26T18:09:41.224918Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:eb85dfe605e90429c57283f7c0327a68b74ab0ddb18ed86afbca06f1c0d1a41d","observation_id":"e02c6e36-7991-4838-a3e1-178f1a71d41d","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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/stae145","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"9c7c7530-ebe6-4776-8eb0-38e2ffdc9a16","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0bc4d2b0ea26f7a572cdc6e613a2e3a22cc9fd47a6cf7ef3430af344c217e4e3","observation_id":"7c795f16-2e3b-4c33-9b17-dc6581bc37c1","resolution":{"observed_at":"2026-06-26T18:09:41.315303Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"8711.2000","doi":"10.1046/j.1365-8711.2000","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"C., et al., 2000, @doi [ ] 10.1046/j.1365-8711.2000.03904.x , http://adsabs.harvard.edu/abs/2000MNRAS.318L..65F 318, L65","venue":null,"work_id":"e31c33b4-236e-4afb-a4c1-f6c6b1d1a91d","year":2000},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:da6361251079695f03b9cf2c9792e99a31dca2119801366f08c4cc8a9a6a28a7","observation_id":"c298e264-8b2e-4a99-be3e-9688f3c4bc9d","resolution":{"observed_at":"2026-06-26T18:09:41.684096Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/232.4.821","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"7ae9f0ad-a4ad-427d-8878-e032e7f5747a","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c1659d67402ee5d511d463ea54692647ec50183b8c900ab771f964332810bf2b","observation_id":"f33a5055-50dd-40fe-baf7-035e4b12859d","resolution":{"observed_at":"2026-06-26T18:09:41.308301Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/430122","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1086/430122 , eprint =","venue":"The Astrophysical Journal","work_id":"ef2b0bec-5261-4f6b-9369-c13a30992db5","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:31abcbf7367d966b861737afd9415d94ce8f8c5af824505b27fd4227bd6b8373","observation_id":"9a20bc52-90b1-4bc2-97bd-70175b28b1b1","resolution":{"observed_at":"2026-06-26T18:09:41.316935Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-11T02:50:00.357749+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T02:50:00.357749+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201322754","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Astronomy and Astrophysics","work_id":"3674c000-00b7-4dca-b5bb-ee15ac10d822","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:b83c43edf7b0086663b6a012ff07cf49c2dcb7339cba4278a6a7116f8501cdca","observation_id":"bdb351cd-ccd8-45c6-b07d-9c668ac05e76","resolution":{"observed_at":"2026-06-26T18:09:41.321123Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20020269","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"R., 2002, @doi [ ] 10.1051/0004-6361:20020269 , https://ui.adsabs.harvard.edu/abs/2002A&A...387..244G 387, 244","venue":"Astronomy and Astrophysics","work_id":"6003ac8d-a713-4e58-b528-5452236e86de","year":2002},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c37c5e10ac91cdad21dc2fd45cac604df2b5fa82a215cc6994c019387eb8332f","observation_id":"fdc0b2e6-a100-4d1a-a7cf-ee5c1ae641b3","resolution":{"observed_at":"2026-06-26T18:09:41.207345Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Castor, John I","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:7ca6e8a1fdca545183b03776a71c5acfc0548228ecd40ab214fec1230d36d0a6","observation_id":"6ac34d0d-b91c-4ae6-94cd-550115aaca8c","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:081f3452001218400af5af9dd14d5a4dbbf15110f838232d33f0a60f56284199","observation_id":"30d09b49-3262-4492-a5b0-a11b77b35b03","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3361","last_updated":"2010-01-06T15:49:51Z","snapshot_observed_at":"2026-07-06T02:00:39.112907Z","submitted_at":"2009-11-17T18:10:16Z","title":"Mass loss from inhomogeneous hot star winds I. Resonance line formation in 2D models","version":2},"cited_work":{"arxiv_id":"0911.3361","doi":null,"metadata_source":"pith","pith_arxiv_id":"0911.3361","snapshot_observed_at":"2026-07-04T12:09:49.757356Z","title":"Mass loss from inhomogeneous hot star winds I. Resonance line formation in 2D models","venue":"astro-ph.SR","work_id":"e3d1bc9c-74b0-4736-8cdf-01a58fe6afae","year":2009},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/0911.3361","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:37f1372ea502599f5af7c47ff80a3b831562e5d57273dc1d3dcaf4ab209b26e7","observation_id":"eb2174bb-8573-45ff-9eb2-c0c7b2227ee6","resolution":{"observed_at":"2026-07-04T12:09:49.758626Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Prinja, Raman K","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:d49125695f0cc8943e1bfb7f92ad9b87dac3e29da4a73483fd8a4aa320d51ab8","observation_id":"0c98cbfc-801e-419c-ba07-2d9bdc1e6f5a","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0487","last_updated":"2008-11-04T12:14:51Z","snapshot_observed_at":"2026-07-06T01:45:37.676808Z","submitted_at":"2008-11-04T12:14:51Z","title":"Mass loss from hot massive stars","version":1},"cited_work":{"arxiv_id":"0811.0487","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.0487","snapshot_observed_at":"2026-07-04T12:09:49.759758Z","title":"Mass loss from hot massive stars","venue":"astro-ph","work_id":"2696ca61-1a47-43db-8700-005fcc79e922","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/0811.0487","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:7e2dbf0065f1d74261b3305091657c2c33cde813f821b3dd25e92b4304b8249e","observation_id":"514b548b-196d-472f-8ce7-be8085aab596","resolution":{"observed_at":"2026-07-04T12:09:49.760916Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6397","last_updated":"2012-07-26T20:00:01Z","snapshot_observed_at":"2026-07-06T02:52:39.013453Z","submitted_at":"2012-07-26T20:00:01Z","title":"Binary interaction dominates the evolution of massive stars","version":1},"cited_work":{"arxiv_id":"1207.6397","doi":null,"metadata_source":"pith","pith_arxiv_id":"1207.6397","snapshot_observed_at":"2026-07-08T17:55:20.560750Z","title":"Binary interaction dominates the evolution of massive stars","venue":"astro-ph.SR","work_id":"61e71e48-3e95-4faa-91e9-ab5164faf8e5","year":2012},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1207.6397","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:497cce5ea2d09fa0f1d950546fc95c127d3457246f41db8e98f9916315fc97ce","observation_id":"75c1e5de-02e1-49dd-88b1-da24fb5c7420","resolution":{"observed_at":"2026-07-04T12:09:49.753815Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:56dd5f418c2ab0555a536995cd63a6b720874bae1574083a99a8b307516f6ab6","observation_id":"67030689-eb0f-4da0-9865-9b871f503e3d","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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/staa3705","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1093/mnras/staa3705 , eprint =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"24f2ae74-7f58-4946-89a3-26161096d7f8","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:8c651912ead17df3db0bf785dd002e0bf39bc6b86785e4a66871ce9fb8ca1414","observation_id":"2bb895a9-b1c2-401d-b630-b0748a683217","resolution":{"observed_at":"2026-06-26T18:09:41.337114Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01451","last_updated":"2020-01-06T09:36:14Z","snapshot_observed_at":"2026-07-06T08:48:39.509290Z","submitted_at":"2020-01-06T09:36:14Z","title":"The VLT-FLAMES Tarantula Survey XXXII. Low-luminosity late O-type stars -- classification, main physical parameters, and silicon abundances","version":1},"cited_work":{"arxiv_id":"2001.01451","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2001.01451","snapshot_observed_at":"2026-07-04T12:09:49.727282Z","title":"and Puls, J","venue":null,"work_id":"87e1519b-ec81-4094-9473-57e250d72f18","year":2001},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/2001.01451","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:dcc3933917108eef72f50822d3b60b82699eaee2ce435b3755c1fb0555fcdd9b","observation_id":"3702290f-c1e4-445b-8d8f-97f65acbafa0","resolution":{"observed_at":"2026-07-04T12:09:49.728560Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:d364b60462ac13b9550d29036631f757b3e44f557f0dbdc432535069119490e8","observation_id":"f7108a02-d177-4c50-af97-76f81833aca4","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201936331","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Astronomy and Astrophysics","work_id":"83b53fec-38b2-45f3-a48c-e4eae5d84123","year":1910},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:3a88c2ebba37964695d90104e1d7647637d84eb82b3d49338ac3898a16e97071","observation_id":"46f83571-319b-4961-bbf6-d75d6954708e","resolution":{"observed_at":"2026-06-26T18:09:41.751376Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.13148","last_updated":"2019-08-24T17:38:26Z","snapshot_observed_at":"2026-07-06T08:11:17.778786Z","submitted_at":"2019-07-30T18:00:28Z","title":"Distances to Galactic OB-stars: Photometry vs. Parallax","version":2},"cited_work":{"arxiv_id":"1907.13148","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.13148","snapshot_observed_at":"2026-07-04T12:09:49.719185Z","title":"Michael and Danforth, Charles W","venue":null,"work_id":"3985e2ff-995b-4713-a7af-3fcd2dc4eef4","year":1907},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1907.13148","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:118c0d80b9419e5442e3743b21c5e1e0ee4e8ca3e57023adea7d64fc3e1e9e1b","observation_id":"5d925be4-b691-42dc-b75b-a97d50512e88","resolution":{"observed_at":"2026-07-04T12:09:49.720461Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-3-7908-1832-1_4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1007/978-3-7908-1832-1_4 , pages =","venue":"Studies in fuzziness and soft computing","work_id":"a521b060-e61a-4d81-8599-7dbfe04e859c","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:58f6e2cb2275d244ae4609c1d80fb5d8a208000202c71c8c46ae729cf81ee3ce","observation_id":"b215843d-ce6c-4bd3-bfd7-8c4064e636c3","resolution":{"observed_at":"2026-06-26T18:09:41.613466Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.3552","last_updated":"2012-06-22T17:30:39Z","snapshot_observed_at":"2026-08-02T18:09:43.417262Z","submitted_at":"2012-04-16T16:17:07Z","title":"Star Formation in the Milky Way and Nearby Galaxies","version":2},"cited_work":{"arxiv_id":"1204.3552","doi":"10.1146/annurev-astro-081811-125610","metadata_source":"doi_reference","pith_arxiv_id":"1204.3552","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"C., Evans N","venue":"astro-ph.GA","work_id":"7baa6132-38a3-4aca-993e-ef2c2d4dcc57","year":2012},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1204.3552","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:da2fa918e68d4c944d8ca45e15123ab52f670bcc0662e4ea9c1520918bff35c7","observation_id":"2b83090f-2d1c-4d1c-98ed-7250ca8f5ff4","resolution":{"observed_at":"2026-06-26T18:09:41.598646Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-18T15:21:13.636344+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-18T15:21:13.636344+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05912","last_updated":"2018-10-13T18:50:26Z","snapshot_observed_at":"2026-07-06T07:07:53.573096Z","submitted_at":"2018-10-13T18:50:26Z","title":"An absorption profile centred at 78 megahertz in the sky-averaged spectrum","version":1},"cited_work":{"arxiv_id":"1810.05912","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.05912","snapshot_observed_at":"2026-07-10T17:37:25.694094Z","title":"An absorption profile centred at 78 megahertz in the sky-averaged spectrum","venue":"astro-ph.CO","work_id":"c3745e5a-7842-46d6-af4d-5d0d3174f59a","year":2018},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1810.05912","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:db9144bb3223a72d686b4d3b3f6c3bc4b8d5fbb3376e27a8f37b05b4f47529ea","observation_id":"93e22f4e-bfac-44cc-91e8-e4ec453b80ad","resolution":{"observed_at":"2026-07-04T12:09:49.740168Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Howarth, Ian D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:67ecb57a8e2fc828dc61dcf6401ca4dcbde91b6be05aa0b557e123241045847e","observation_id":"298ac46c-6434-47dc-b744-e09b0a869aaa","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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/s1743921308020747","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1017/S1743921308020747 , eprint =","venue":"Proceedings of the International Astronomical Union","work_id":"d63459db-f0d4-470b-859e-d8d89944c35b","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:77a72365d522a0c3ce8364a8e4d93813c553ea3d0e1b838e1f78db72d467102e","observation_id":"184192dd-aa78-4638-bdb9-a51137c3c4ba","resolution":{"observed_at":"2026-06-26T18:09:41.591986Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":", issn =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:3c3a6ccc4640062fd08a20563a0715fbea08cb0dcea7223a72b9389120c88e1b","observation_id":"7d2ba04e-1d5d-4fe7-9922-89224b6065be","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.3360","last_updated":"2013-11-14T01:42:21Z","snapshot_observed_at":"2026-07-06T03:28:07.857415Z","submitted_at":"2013-11-14T01:42:21Z","title":"The IACOB project: I. Rotational velocities in Northern Galactic O and early B-type stars revisited. The impact of other sources of line-broadening","version":1},"cited_work":{"arxiv_id":"1311.3360","doi":null,"metadata_source":"pith","pith_arxiv_id":"1311.3360","snapshot_observed_at":"2026-07-04T15:59:56.883852Z","title":"The IACOB project: I. Rotational velocities in Northern Galactic O and early B-type stars revisited. The impact of other sources of line-broadening","venue":"astro-ph.SR","work_id":"456df310-8c23-412e-96be-b53df33890ea","year":2013},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1311.3360","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:71af904e91f613405a878c306c93b9bfec07286d1f3796c0e7807e155ddb2367","observation_id":"6dc27d60-9167-4132-ac4f-a0a141d96340","resolution":{"observed_at":"2026-06-26T18:09:41.483164Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.newast.2013.03.009","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1016/j.newast.2013.03.009 , file =","venue":"New Astronomy","work_id":"28ef4e31-a8e0-4062-b95f-f5c0ffe8f904","year":2013},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:329d9b5ca04c9a82a2394d241255383ba4d4876e9df237bc4fd4461762f774e1","observation_id":"a73d5584-ab96-4bac-b8eb-de6fe1f4cb06","resolution":{"observed_at":"2026-06-26T18:09:41.644118Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c60b02d686b0bae6bc696ee2a8ae5ed24c9752ca40a598541c2a97b3777ca259","observation_id":"9d8c9679-5154-4d50-a0f5-473f5a0d55a5","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2966.2012","doi":"10.1111/j.1365-2966.2012","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"and Shibahashi , H","venue":null,"work_id":"91cc99ad-bdb6-42b2-afbd-e26dad5ec964","year":2012},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:f2466982938987d51e92bc3cbcc1175184a2739b12740b52e90c538c49e7a9fc","observation_id":"5762bbbf-48a5-4082-add5-224518f05f4d","resolution":{"observed_at":"2026-06-26T18:09:41.740521Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:49:50.088461+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:49:50.088461+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:8dd39f6e505908041cf0e572918ed3e756b92cf17d0a8cef7a8bc7468cf115d5","observation_id":"cf1a761c-9ff5-4483-870d-092019309966","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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/stw1205","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"I., Schaerer, D., Thuan, T","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"ef44fbb6-3ab9-4df6-bb08-8d574cc4c240","year":2016},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:6d0494f4fa95c254606c45bb873085226da7be49753af30212b1833c78a5a196","observation_id":"7161be41-f2b3-4133-b0f2-212171f4e40f","resolution":{"observed_at":"2026-06-26T18:09:41.540104Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-13T13:52:30.557794+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T13:52:30.557794+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa355","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"dfc70acd-80e7-4cd3-8309-eb44a6b72753","year":1910},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:e5c692f024783a911e207befff50d54d69af5d7cc69d8680541b63d991e4e95f","observation_id":"9aa2f15c-ca14-4c3c-9389-01df4be5f390","resolution":{"observed_at":"2026-06-26T18:09:41.608979Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201098","last_updated":"2002-01-07T21:09:22Z","snapshot_observed_at":"2026-07-07T00:24:25.145904Z","submitted_at":"2002-01-07T21:09:22Z","title":"The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems","version":1},"cited_work":{"arxiv_id":"astro-ph/0201098","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0201098","snapshot_observed_at":"2026-07-09T20:56:34.029626Z","title":"The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems","venue":"astro-ph","work_id":"ea8d08ff-9d11-4a88-8b07-e109ece86e94","year":2002},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0201098","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:82fdc6832dbfb1af2f7991696a6eadfee29f764918466c04601fa75ab16da37e","observation_id":"f721057d-962c-47b0-9dc4-7ed45e0a850e","resolution":{"observed_at":"2026-06-26T18:09:41.215614Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad5292","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"b3f3604f-f314-4192-9084-57faf24e9445","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:ea44da20a782ebcf3e24f10a60de458b02ce437cf04bec63b2c060087adc894c","observation_id":"88762deb-491c-4d80-93c1-7e01ffe4e508","resolution":{"observed_at":"2026-06-26T18:09:41.417973Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.03094","last_updated":"2018-11-07T19:00:00Z","snapshot_observed_at":"2026-07-06T07:13:21.130146Z","submitted_at":"2018-11-07T19:00:00Z","title":"CIGALE: a python Code Investigating GALaxy Emission","version":1},"cited_work":{"arxiv_id":"1811.03094","doi":"10.1051/0004-6361/201834156","metadata_source":"pith","pith_arxiv_id":"1811.03094","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"2019, A&A, 622, A103, doi: 10.1051/0004-6361/201834156","venue":"astro-ph.GA","work_id":"be5550c0-1319-4534-89a4-4f1e0cbd4f29","year":2018},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1811.03094","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:b4fa42ac1eec39d4955cfa0fc6bc54cd23d90016e197f422f96ffd39d3f3a431","observation_id":"8677301e-2b94-4490-8b45-ac1742aa013c","resolution":{"observed_at":"2026-06-26T18:09:41.246913Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-20T19:21:57.589023+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T19:21:57.589023+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2009","doi":"10.1111/j.1365-2966.2009","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607","venue":null,"work_id":"23562d5d-936a-4b08-a6f0-15466b0fcd7c","year":2009},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:adc56619c5a1c8827fc3bfa528311da833fcee8965ebee43304991028e114173","observation_id":"0df2dd98-6a26-4c9d-b8ba-d1b7b073a9d2","resolution":{"observed_at":"2026-06-26T18:09:41.660633Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9701019","last_updated":"1997-01-06T19:58:21Z","snapshot_observed_at":"2026-07-07T01:15:28.898450Z","submitted_at":"1997-01-06T19:58:21Z","title":"A standard stellar library for evolutionary synthesis: I. Calibration of theoretical spectra","version":1},"cited_work":{"arxiv_id":"astro-ph/9701019","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9701019","snapshot_observed_at":"2026-06-26T18:09:41.465021Z","title":"A standard stellar library for evolutionary synthesis: I. Calibration of theoretical spectra","venue":"astro-ph","work_id":"d6f50bed-2e29-4a62-9358-698be5773583","year":1997},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/9701019","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:db1df5d4a19986edc454fe8eac7220454ea232abde4ac3a108c6a3267b31ad21","observation_id":"d346cfb9-ff7d-436f-b420-8763764073c4","resolution":{"observed_at":"2026-06-26T18:09:41.466838Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.13254","last_updated":"2025-08-26T23:49:43Z","snapshot_observed_at":"2026-07-06T19:35:04.087584Z","submitted_at":"2024-10-17T06:21:22Z","title":"Lyman Continuum leakage from massive leaky starbursts: A different class of emitters?","version":2},"cited_work":{"arxiv_id":"2410.13254","doi":"10.48550/arxiv.2410.13254","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.13254","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"9ec54ef1-8025-4997-997e-df7ba57d2528","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/2410.13254","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:8c2faef85835c8f25eaa1bf5e5fcfec203a82b01e9f2e12589a6108861a14718","observation_id":"1161f8e7-ce37-42d4-828d-c32e28ff651a","resolution":{"observed_at":"2026-06-26T18:09:41.586281Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/ac5331","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"R., Jaskot, A","venue":"The Astrophysical Journal Supplement Series","work_id":"0e9a8766-7374-4f4d-a4de-8970f7cc380a","year":2022},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c58a41871fa75b006c3d984adee39279670830f620a7278a3fa940e30b9d3116","observation_id":"578ee9b2-4bc4-4a5d-8096-358faeaac16b","resolution":{"observed_at":"2026-06-26T18:09:41.460760Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-07-11T03:18:58.750852+00:00","source":"paper_reference_links","state":"open"},"event_date":"2024-12-06","event_type":"correction","notice_doi":"10.3847/1538-4365/ad7bb9","provenance":{"observed_at":"2026-07-11T03:01:18.018303+00:00","source":"crossref","source_record_id":"10.3847/1538-4365/ad7bb9->10.3847/1538-4365/ac5331:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Owocki, S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:d89cad5fc631f9539e7760694b9b8f5833a32257675cdff4dbfdb4074d9401db","observation_id":"c61006d5-f456-4a18-bf54-30f5fe805ea2","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.4444","last_updated":"2012-05-20T18:32:14Z","snapshot_observed_at":"2026-07-06T02:48:25.933186Z","submitted_at":"2012-05-20T18:32:14Z","title":"Nitrogen line spectroscopy in O-stars -- III. The earliest O-stars","version":1},"cited_work":{"arxiv_id":"1205.4444","doi":"10.1051/0004-6361/201218955","metadata_source":"pith","pith_arxiv_id":"1205.4444","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Nitrogen line spectroscopy in O-stars -- III. The earliest O-stars","venue":"astro-ph.SR","work_id":"5efda37f-20f9-405b-81ac-daf4960e33dd","year":2012},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.4444","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:6f8f8aa60e9e43a97e15c72ff13379284b043cbd23873dc5c87d0596e66d1f97","observation_id":"941bf11f-3906-4770-a0e3-ea06762cd79e","resolution":{"observed_at":"2026-06-26T18:09:41.480301Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.5148","last_updated":"2011-10-24T07:39:26Z","snapshot_observed_at":"2026-07-06T02:36:17.251994Z","submitted_at":"2011-10-24T07:39:26Z","title":"Nitrogen line spectroscopy in O-stars -- II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud","version":1},"cited_work":{"arxiv_id":"1110.5148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1110.5148","snapshot_observed_at":"2026-06-26T18:09:41.461871Z","title":"Nitrogen line spectroscopy in O-stars -- II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud","venue":"astro-ph.SR","work_id":"e2638281-26d8-48ca-adca-ad8df3e4af34","year":2011},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1110.5148","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:55f44beceecb568786c1a2fe798409da95b103f13a9dc77b15d95644eb566d03","observation_id":"0ec23bc7-24b2-444e-802f-ad2bb370f496","resolution":{"observed_at":"2026-06-26T18:09:41.463517Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201117101","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1051/0004-6361/201117101 , file =","venue":"Astronomy and Astrophysics","work_id":"943d431f-097b-421f-af9c-672ad2d990ed","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:18bc9a6aece95d035963d0943f5ee1d1bb10a72ad45e1bb1292c0057b610b8b7","observation_id":"298ae282-b520-4b5f-9710-4e0ad7e815db","resolution":{"observed_at":"2026-06-26T18:09:41.323871Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201322390","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1051/0004-6361/201322390 , eprint =","venue":"Astronomy and Astrophysics","work_id":"5d1ee05d-8718-4e57-98d2-7f93c9d68a40","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:141c00f5c5b2baad6135dc71cd301cb9e53be23fe1293ecffc2de458a2cafa20","observation_id":"54a9c24a-e9f3-4a9e-bc16-cc3d86848fae","resolution":{"observed_at":"2026-06-26T18:09:41.504564Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0805.3162","last_updated":"2008-05-20T20:56:46Z","snapshot_observed_at":"2026-07-06T01:37:53.334247Z","submitted_at":"2008-05-20T20:56:46Z","title":"Adaptive Optics Photometry and Astrometry of Binary Stars. III. A Faint Companion Search of O-Star Systems","version":1},"cited_work":{"arxiv_id":"0805.3162","doi":null,"metadata_source":"pith","pith_arxiv_id":"0805.3162","snapshot_observed_at":"2026-07-04T12:09:49.729694Z","title":"Adaptive Optics Photometry and Astrometry of Binary Stars. III. A Faint Companion Search of O-Star Systems","venue":"astro-ph","work_id":"da0d9ed4-130f-473d-ac59-82f98db180f1","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/0805.3162","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:05206e43c01ea14ac0b1ab06daabeeed759576ed6fbfa63eb1a2bafe05f50a54","observation_id":"cbbab505-ba78-4ac6-88dc-eed0f07292f5","resolution":{"observed_at":"2026-07-04T12:09:49.730999Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.7995","last_updated":"2014-01-30T21:00:18Z","snapshot_observed_at":"2026-07-06T03:34:47.050393Z","submitted_at":"2014-01-30T21:00:18Z","title":"Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive","version":1},"cited_work":{"arxiv_id":"1401.7995","doi":"10.1093/mnras/stu008","metadata_source":"pith","pith_arxiv_id":"1401.7995","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive","venue":"astro-ph.SR","work_id":"536e7bc1-19fb-4a9f-acf6-4c4bd729acdc","year":2014},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1401.7995","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:74339bbbb6695c84c804cdb6ffc10afaacfe626582747489f4fab8103e131e83","observation_id":"60de25ad-e6f4-48aa-8204-9ed72c474d6e","resolution":{"observed_at":"2026-07-04T12:09:49.756226Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-06-01T22:58:39.912236+00:00","source":"crossref_status_cache"},{"observed_at":"2026-06-01T22:58:39.912236+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201732050","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1051/0004-6361/201732050 , eprint =","venue":"Astronomy and Astrophysics","work_id":"5f4a8484-ad39-4c5a-9787-b42c98332673","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:215ea578145a3d15010a1457794c992c9759e0e8d9b91bc2ae381f56d81b2eac","observation_id":"7c26d2e9-588b-4a64-a61a-9f796516edc8","resolution":{"observed_at":"2026-06-26T18:09:41.648383Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921312009350","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", booktitle =","venue":"Proceedings of the International Astronomical Union","work_id":"c63e3da8-2ced-4c24-9383-be6ab5efa1f2","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:56a497cdc33c40ea0f9731d34f8679c66abce7c6ff6c47a8bb5fc783f1e1ab2b","observation_id":"90eeff18-d51b-45bd-b0c1-1badb8cbab28","resolution":{"observed_at":"2026-06-26T18:09:41.555101Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.09444","last_updated":"2018-11-23T12:11:17Z","snapshot_observed_at":"2026-07-06T07:16:36.095212Z","submitted_at":"2018-11-23T12:11:17Z","title":"A VLT/FLAMES survey for massive binaries in Westerlund 1 V. the X-ray selected blue stragglers Wd1-27 and -30a","version":1},"cited_work":{"arxiv_id":"1811.09444","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.09444","snapshot_observed_at":"2026-07-04T12:09:49.732163Z","title":"A VLT/FLAMES survey for massive binaries in Westerlund 1 V. the X-ray selected blue stragglers Wd1-27 and -30a","venue":"astro-ph.SR","work_id":"0ad065d1-702e-457e-9749-9737c00d5749","year":2018},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1811.09444","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:93087be381a5f296e89670fb673436f4e82207f69bd6e0582d52935bf131b0e5","observation_id":"9af5d0a8-c594-4c8d-8190-291dfe577a43","resolution":{"observed_at":"2026-07-04T12:09:49.733448Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"The Messenger , pages =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:fd700dfe37197488a4b82bc0209bab42187ab56306d7a441e7cc0199a15f3f17","observation_id":"16d97e08-b2cb-47ab-918e-c34e2a0eddcf","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c182324c62871ddfbc950471414605b4a428edc04159d870f5af23f6fe8553ee","observation_id":"b1b491ce-a1d1-44aa-a3d3-b3bd344175c9","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201424312","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Sana, H","venue":"Astronomy and Astrophysics","work_id":"b5e3fff7-6a36-4ac0-8b16-9eabbaa14e4d","year":2014},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:1b110c8a299bae4e4f95fa13d2c1e1a0bbb62ca03a8eeb4b3284846d34dcaebd","observation_id":"60d2a4b0-e091-43c3-a5b2-255cb7ce6ab8","resolution":{"observed_at":"2026-06-26T18:09:41.546744Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20064995","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Astronomy and Astrophysics","work_id":"abc0ae57-6278-4d05-b75e-34cb27e618cd","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:be0529f24076688d04b35ff4253d38b0a873d95d3ca221c5ea1bb1d5b04480b6","observation_id":"6252a463-dd6b-49e9-9934-40eac310248f","resolution":{"observed_at":"2026-06-26T18:09:41.225933Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Urbaneja, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:481f3f1a4a287524155ae7dfce2f6f1009a8bbf4c32db90018c44ef60969245d","observation_id":"af20db1f-b018-4095-9c73-0d57b207ce92","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":"John and Miller, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c7e26e6652269925379c6c9eaa4ad8ec853f67e2c5d6d2ee7edf86f7ec3b4e32","observation_id":"e1b0ba58-a28f-4b13-a8d9-caed405907ba","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07780","last_updated":"2017-10-21T10:22:48Z","snapshot_observed_at":"2026-07-06T06:05:18.459253Z","submitted_at":"2017-10-21T10:22:48Z","title":"2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach","version":1},"cited_work":{"arxiv_id":"1710.07780","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.07780","snapshot_observed_at":"2026-07-04T12:09:49.741417Z","title":"2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach","venue":"astro-ph.SR","work_id":"70ab323f-1cad-459d-9549-0a309b1ae5ca","year":2017},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1710.07780","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:7723519c074014d61d6af7cf8617694402104fed77e3a7a3340e6a0225f38a66","observation_id":"a685405c-3768-4556-8112-418364fd4a38","resolution":{"observed_at":"2026-07-04T12:09:49.742703Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Lanz, T and Hillier, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:d825d257a391e5463d429a6af919915fef5e547cd913b2cd23454e79305341bf","observation_id":"6647aa95-95fa-4b29-ac09-e3d6dfa2e10b","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.04812","last_updated":"2016-11-14T17:59:39Z","snapshot_observed_at":"2026-07-06T05:14:45.281211Z","submitted_at":"2016-10-16T02:39:46Z","title":"Modeling the early evolution of massive OB stars with an experimental wind routine","version":2},"cited_work":{"arxiv_id":"1610.04812","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.04812","snapshot_observed_at":"2026-07-04T12:09:49.743874Z","title":"Modeling the early evolution of massive OB stars with an experimental wind routine","venue":"astro-ph.SR","work_id":"5da67692-0125-4b2f-afda-6b1373b0b9fc","year":2016},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1610.04812","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:b55e2b6202cfdf5045b16f99c504a7a99fda955895e54bb95a133ac5034a020d","observation_id":"d734a314-cd19-49cb-8816-d8a8b8ee510f","resolution":{"observed_at":"2026-07-04T12:09:49.745351Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.06586","last_updated":"2019-10-15T08:20:25Z","snapshot_observed_at":"2026-08-01T20:25:14.203427Z","submitted_at":"2019-10-15T08:20:25Z","title":"New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars. I. Method and first results","version":1},"cited_work":{"arxiv_id":"1910.06586","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1910.06586","snapshot_observed_at":"2026-07-04T12:09:49.721563Z","title":null,"venue":null,"work_id":"293408f1-4fe7-4453-94cd-5f4264ab3e7a","year":1910},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1910.06586","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:5abe6c527a1b29273d9a39745e6e8100878024faf6b47b21636771fb6b055ff7","observation_id":"8ee6cee3-2e9b-487a-8435-0ab3435f8abf","resolution":{"observed_at":"2026-07-04T12:09:49.723061Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"and Fullerton,, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:6538e1056ec6dbb26ec25bcb07489a3053e9e4f620dcfb62cb56bfb16785ca8d","observation_id":"c661bc8f-82de-4a59-a131-b1a9c5a254b2","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:b700b6b3f005ff1cc8d1190253aec24531bfa7068be4a73fa241a17e9b598935","observation_id":"b5cd8ce7-2f35-42a7-8feb-a3c370694d29","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.1762","last_updated":"2011-11-07T22:19:15Z","snapshot_observed_at":"2026-07-06T02:37:10.370619Z","submitted_at":"2011-11-07T22:19:15Z","title":"A generalised porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds","version":1},"cited_work":{"arxiv_id":"1111.1762","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.1762","snapshot_observed_at":"2026-07-04T12:09:49.749386Z","title":"A generalised porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds","venue":"astro-ph.SR","work_id":"0feb0415-2506-4640-938d-9869bb57d3fb","year":2011},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1111.1762","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:cd41b993a2a08c58226730ca9b693d33d999a98ae371044c626d5b294f53e424","observation_id":"e7c0bbd8-2390-4502-b78f-057e9599b719","resolution":{"observed_at":"2026-07-04T12:09:49.751330Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abba24","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal","work_id":"07a92ed6-cb40-4a36-8ebb-9a6e6abd7868","year":2009},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:5d4771518334df9e9411cd5bddb61b1570a18aa928925f6d620226cde7425ab2","observation_id":"0b42fed0-45dd-4e9c-99e5-5640c9b1c8ed","resolution":{"observed_at":"2026-06-26T18:09:41.240802Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"The Astrophysical Journal , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:f18a9759f1b55a3001c60afc0ca6b0492f8faac591a50e8ed2e0ef05fb4c8476","observation_id":"6f48c8ec-1d6a-4c92-b183-c317188b8f70","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.05417","last_updated":"2015-09-17T20:16:24Z","snapshot_observed_at":"2026-07-06T04:30:16.025246Z","submitted_at":"2015-09-17T20:16:24Z","title":"Local Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak","version":1},"cited_work":{"arxiv_id":"1509.05417","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.05417","snapshot_observed_at":"2026-07-04T12:09:49.746482Z","title":"Local Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak","venue":"astro-ph.SR","work_id":"66b48704-4d56-4cbd-b82c-94563278570b","year":2015},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1509.05417","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:8eb8383038a8baaf2ba35a4830fd1b92658ce151608e3158cfacb9c19f8dc76b","observation_id":"82cd9f16-be7d-442c-85cb-ddfa2ad137ec","resolution":{"observed_at":"2026-07-04T12:09:49.748151Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0704.2390","last_updated":"2007-11-20T12:59:39Z","snapshot_observed_at":"2026-07-06T01:26:31.626011Z","submitted_at":"2007-04-18T17:13:22Z","title":"Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates","version":2},"cited_work":{"arxiv_id":"0704.2390","doi":null,"metadata_source":"pith","pith_arxiv_id":"0704.2390","snapshot_observed_at":"2026-07-04T12:09:48.649438Z","title":"Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates","venue":"astro-ph","work_id":"3ecb4623-6bc1-4b9c-9d7a-14a0cbf1ac3a","year":2007},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/0704.2390","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:fa812118b18bdf2b5e77d0a3474c9ce65e6a410f6db53e8277280f94662e2ec2","observation_id":"e8f30698-ab47-4c06-aeb6-5ef5335666d9","resolution":{"observed_at":"2026-07-04T12:09:48.651209Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0808.2233","last_updated":"2008-08-16T03:15:14Z","snapshot_observed_at":"2026-07-06T01:41:36.546288Z","submitted_at":"2008-08-16T03:15:14Z","title":"On the Importance of the Interclump Medium for Superionization: O VI Formation in the Wind of Zeta Pup","version":1},"cited_work":{"arxiv_id":"0808.2233","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.2233","snapshot_observed_at":"2026-07-04T12:19:48.976116Z","title":"On the Importance of the Interclump Medium for Superionization: O VI Formation in the Wind of Zeta Pup","venue":"astro-ph","work_id":"dab38b09-33c3-4097-a063-758765f0e6f1","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/0808.2233","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:91b04afb7bc3b8b27b0aa94e56955f26f68bae8740242f272fa27361a0b746f1","observation_id":"8f79d781-e8d3-42ab-b3e9-eb27454a7246","resolution":{"observed_at":"2026-07-04T12:19:48.981656Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1407.1837","last_updated":"2014-07-07T20:00:01Z","snapshot_observed_at":"2026-08-01T20:56:17.208824Z","submitted_at":"2014-07-07T20:00:01Z","title":"The VLT-FLAMES Tarantula Survey XVII. Physical and wind properties of massive stars at the top of the main sequence","version":1},"cited_work":{"arxiv_id":"1407.1837","doi":null,"metadata_source":"pith","pith_arxiv_id":"1407.1837","snapshot_observed_at":"2026-07-04T12:09:49.734729Z","title":"The VLT-FLAMES Tarantula Survey XVII. Physical and wind properties of massive stars at the top of the main sequence","venue":"astro-ph.SR","work_id":"7ee08bb5-aa59-449c-8cfe-b05a697cfd7c","year":2014},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1407.1837","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:58ff086810d61a9c8b53568e5a3416458b07b71943d97832da51bd951f479b5a","observation_id":"aecde0ad-ae54-44be-ab06-c6e7d426a4a4","resolution":{"observed_at":"2026-07-04T12:09:49.736055Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"0186.001553","doi":"10.1146/annurev.aa.24.090186.001553","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"volume =","venue":"Annual Review of Astronomy and Astrophysics","work_id":"0046f75b-29eb-4ffe-8adb-2a4afb1abb99","year":1986},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:3d465165e5422e2975958e402e8bbf2bd246342b6879bc504908e8b5498d098f","observation_id":"89b0400c-6675-469d-9290-b1483d9c234a","resolution":{"observed_at":"2026-06-26T18:09:41.440977Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-05-22T08:24:10.89233+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-22T08:24:10.89233+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.1643","last_updated":"2012-02-08T10:06:25Z","snapshot_observed_at":"2026-07-06T02:42:31.472562Z","submitted_at":"2012-02-08T10:06:25Z","title":"Genetic algorithms in astronomy and astrophysics","version":1},"cited_work":{"arxiv_id":"1202.1643","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.1643","snapshot_observed_at":"2026-07-04T12:09:49.724988Z","title":"Genetic algorithms in astronomy and astrophysics","venue":"astro-ph.IM","work_id":"fe8143dc-6fab-4c60-b5ee-22677cc28811","year":2012},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1202.1643","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:22d6b55da337fdc8178c9b2370e487a29274d30e0c9640677e9f6d0296d68c32","observation_id":"ed095603-4969-4f0c-babc-c993c399525e","resolution":{"observed_at":"2026-07-04T12:09:49.726130Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/2041-8205/741/1/l8","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Sana, H","venue":"The Astrophysical Journal Letters","work_id":"1aecb20a-49e6-46f5-9eca-cc46dc67e6cb","year":2041},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0799fc33a6b4386276c37ecc67e0c70ce66503e95af0e0f2a2cbbc6873c38b65","observation_id":"cf2364d0-87d4-408d-b834-0e71abc43479","resolution":{"observed_at":"2026-06-26T18:09:41.399676Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1101.5293","last_updated":"2011-02-08T10:05:46Z","snapshot_observed_at":"2026-07-06T02:22:38.190996Z","submitted_at":"2011-01-27T14:18:56Z","title":"Mass loss from inhomogeneous hot star winds II. Constraints from a combined optical/UV study","version":2},"cited_work":{"arxiv_id":"1101.5293","doi":null,"metadata_source":"pith","pith_arxiv_id":"1101.5293","snapshot_observed_at":"2026-07-04T12:09:49.761984Z","title":"Mass loss from inhomogeneous hot star winds II. Constraints from a combined optical/UV study","venue":"astro-ph.SR","work_id":"3d8a5b9f-232a-4f22-9af3-3eda92ac997b","year":2011},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"cited_paper":"/paper/1101.5293","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:0ff872b95790c53e6bc0c431438b7b90d10668b46c9cbe335e536f9f2fe1b271","observation_id":"9a75434f-1f09-460e-8e77-0346c0ace93d","resolution":{"observed_at":"2026-07-04T12:09:49.763177Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:ef5e44962d08a9f199c87b15555e526b6a3c3c7ff0761322e0f0e33d173010cf","observation_id":"a70701cc-391a-4722-be96-c2ef5d9bbcf3","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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/s1743921307001603","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Proceedings of the International Astronomical Union","work_id":"28e534e3-ef1b-42a2-8097-9954ae0a54cd","year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:a541de2d5797ce4f9525437bf124d3ef36302de2ba350301469ec787e78d495e","observation_id":"a2d91961-3d47-4beb-83ff-873b01da3d5d","resolution":{"observed_at":"2026-06-26T18:09:41.666387Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-26T07:09:31.413097Z","title":"John and Lanz, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:7cab51a947230433b173b8e41ad65b02550c6d2e82be76b1e31cd30928dc13f5","observation_id":"20cc9f8b-95cc-4b1f-8dbb-bc1275350f3a","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:c0f0c6b47817017c835ac2217b38654b346f21ae7730bed3936c180c8e2e86f1","observation_id":"8d1aa6f8-9e59-458d-87fe-37197afe0740","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"2026-06-26T07:09:31.413097Z","title":", issn =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:4dac8f26ece2a71d641d43bc63a81f646cdfe0ae6e83622c7f0a9a3b05132feb","observation_id":"6588f1db-19e4-4bdf-a24a-080c76c14217","resolution":{"observed_at":"2026-06-26T07:09:31.413097Z","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":"10.1086/169224","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"K., Barlow, M","venue":"The Astrophysical Journal","work_id":"77f15604-32af-4fc1-96f7-4fbe00684ece","year":1990},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-06-26T07:09:31.413097Z"},"links":{"citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:9fccfe80ba8cedfc55c43da2f6e1e9d0e25012f64f42038ca3bae096351e43bb","observation_id":"05b1c7f9-4ae8-4398-a7e9-dd114d4d9862","resolution":{"observed_at":"2026-06-26T18:09:41.700594Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-05-23T07:53:23.059264+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-23T07:53:23.059264+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11010","last_updated":"2018-05-28T16:11:02Z","snapshot_observed_at":"2026-07-06T06:41:36.871103Z","submitted_at":"2018-05-28T16:11:02Z","title":"Atmospheric NLTE-models for the spectroscopic analysis of blue stars with winds. IV. Porosity in physical and velocity space","version":1},"cited_work":{"arxiv_id":"1805.11010","doi":"10.1051/0004-6361/201832993","metadata_source":"pith","pith_arxiv_id":"1805.11010","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Atmospheric NLTE-models for the spectroscopic analysis of blue stars with winds. IV. Porosity in physical and velocity space","venue":"astro-ph.SR","work_id":"0d5b1f1e-4691-4b8f-aa80-f431a946de91","year":2018},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1805.11010","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:26e0d2794f3bbba1421e038c67f4653f270b575cb0dc2bd75c3847f1c815298c","observation_id":"2e5d3017-c493-4117-9681-28fce72d5dd5","resolution":{"observed_at":"2026-06-26T18:09:41.375660Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0811.0487","last_updated":"2008-11-04T12:14:51Z","snapshot_observed_at":"2026-07-06T01:45:37.676808Z","submitted_at":"2008-11-04T12:14:51Z","title":"Mass loss from hot massive stars","version":1},"cited_work":{"arxiv_id":"0811.0487","doi":null,"metadata_source":"pith","pith_arxiv_id":"0811.0487","snapshot_observed_at":"2026-07-04T12:09:49.759758Z","title":"Mass loss from hot massive stars","venue":"astro-ph","work_id":"2696ca61-1a47-43db-8700-005fcc79e922","year":2008},"citing_paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0811.0487","citing_paper":"/paper/2606.23456"},"observation_digest":"sha256:7171357a2bee9526a40425ad03f5dbb3ab25c635e1defb0a33335ee741a6a6c6","observation_id":"75c49971-0cd0-4a81-9303-215a03379891","resolution":{"observed_at":"2026-06-26T18:09:41.725532Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2606.23456","last_updated":"2026-06-22T15:06:44Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T23:58:11.694332Z","submitted_at":"2026-06-22T15:06:44Z","title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":11,"parse_uncertain":0,"unresolved":25,"verified_exact":64,"verified_fuzzy":0},"total_outbound_references":297},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 100 of 297 outbound references and 2 inbound Pith citation observations for arXiv:2606.23456."}