{"as_of":"2026-08-11T06:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b42cfb37485fe2cd11fd391bb965355ff07d8b65ce85767caff97ebc44ebb0ea","coverage":[{"denominator":129,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T12:29:10.089534Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.04853/citation-record","integrity":"/paper/2607.04853/integrity","json":"/paper/2607.04853/citation-record.json","paper":"/paper/2607.04853"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T12:29:10.089534Z","title":"N., Matt, S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f0ddb27b3a62646fc383ecc98e515e7dfe939649ef6b8401fca32f7d32a3955f","observation_id":"f0dbe131-2988-4cad-a7cc-0280c395f04a","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2016, in IAU","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:a31ede86d5e318d463e8d9ffebfeb09fdcbc273cb8cae56de9a28d64237f34bc","observation_id":"2e0692c7-4065-466a-b838-c9e142fa2156","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/s174392131600226x","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"320, Solar and Stellar Flares and their Effects on Planets, ed","venue":"Proceedings of the International Astronomical Union","work_id":"9518742b-70c9-471f-a728-1e9f39864904","year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:4d1177a21de3007866eb3786b993ace95a881dd1976182f9505cd7ba5f49c3cf","observation_id":"9f0cf4fb-1876-408b-b7f5-9ab483df84c8","resolution":{"observed_at":"2026-07-11T12:38:00.740261Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:05.611354+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:05.611354+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"S., Jin, M., L¨ uftinger, T., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ce0a80a9ccdc59ec67cb771904f83bf2a20e404fc52dbe145acc198e53006d36","observation_id":"c128451a-e11c-4bfc-98a2-dfc156ce040c","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2018, Nature, 554, 211, doi: 10.1038/nature24671","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:3a7d7f859cb8e66903df5f07a1ed9581fc506e204570e9de45e73412f27b4777","observation_id":"1e746130-c395-4ab3-918a-80aecb7e65c4","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1051/0004-6361:200811131","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2008, A&A, 492, L35, doi: 10.1051/0004-6361:200811131","venue":"Astronomy and Astrophysics","work_id":"5e8ac695-6179-4608-bf97-049c1b296ebc","year":2008},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:32f584f6710af2a692862e5e21f45df4d0e3afd4ee855f7f890fe2a97828d11b","observation_id":"0b618446-6df5-4c8c-b047-458031af9f19","resolution":{"observed_at":"2026-07-11T12:38:00.941322Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:07.053344+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:07.053344+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41550-019-0781-4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., et al","venue":"Nature Astronomy","work_id":"013084c1-469a-4522-95ca-9e3bcb632df5","year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:51c1c79711eed88e3b3e395e2f1120cd7677118564b4125e92de0ddf5e93c9de","observation_id":"4274e005-2af9-435d-bf01-e27b0d6502d0","resolution":{"observed_at":"2026-07-11T12:38:01.079039Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:07.634103+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:07.634103+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"R., Tasse, C., Keers, R., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ab538e4b1ed6818667acad8a260c5a0f7c6c844b2928f285a834e9c8bbafb9db","observation_id":"bbbb3541-aca8-4b77-b6c9-af275c63b9f5","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/stad2100","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, MNRAS, 524, 5060, doi: 10.1093/mnras/stad2100","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"3619df7a-a5d6-4514-8ec1-1d70b0acc6ad","year":2023},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:eab06603b2e81b22c7552c2926a516d9a524259ae6e75b9f359311c677e2866d","observation_id":"5a6cb894-28fa-4a95-999b-86f28d7c8acb","resolution":{"observed_at":"2026-07-11T12:38:00.837780Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:08.710216+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:08.710216+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac739b","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, ApJ, 933, 92, doi: 10.3847/1538-4357/ac739b","venue":"The Astrophysical Journal","work_id":"f928081b-3caa-4c77-b6e9-d1332baaa34c","year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:2c218c541fa09d02bf68634e8b866736f9821e6af9c2cb29d2ca49080b9a4735","observation_id":"ab2c5d9f-124f-45ae-8c7e-2a0c98aaf12d","resolution":{"observed_at":"2026-07-11T12:38:00.761782Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:09.204594+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:09.204594+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f3afc86431535ec9d3b49492c204f2f93d0ee0ec41c69dfe3f24a0e4fb5de840","observation_id":"9efa686e-456a-497d-9266-0eb833f6db12","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"D., Cheng, X., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:4c8e328cf1ad64f9f74484709fd9d8a319f4e24aaeb04333ba3843355a538662","observation_id":"814e373a-fd00-45b0-b873-95756210522b","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/733/1/67","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., Drake, J","venue":"The Astrophysical Journal","work_id":"386a27fd-d6a1-4ca0-99b7-0637e58c890d","year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:390b615e44aa9f64eec1ecd1926ee143b92b7eb76f418491099b2e9bfc71399d","observation_id":"a4477ec4-a5b7-4c1a-a945-ef94cf33082b","resolution":{"observed_at":"2026-07-11T12:38:00.809359Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:10.628681+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:10.628681+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e47c9cdef7ab2f18d2e1adefae0f1ae85b641556c29a07d05d50d9787a263c09","observation_id":"b0fc3733-e538-401c-a089-2bf311f624c8","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"R., & Winebarger, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:7a10e860520d6950974fc7882f3d0b60437c543dd72edfb0f829cf0ed2e6c467","observation_id":"7273fae2-3c58-4c10-974b-e5f1979fb978","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1007/s11207-016-1036-5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Solar Physics","work_id":"31111d01-dbcf-48ab-bfeb-9ddba234ea0d","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:acbbc4e18496222e27c5a4f49fbe9d69320b58d2b94be8d5cd530a997b6341e3","observation_id":"e125191b-1fd8-465f-9052-afad4125b774","resolution":{"observed_at":"2026-07-11T12:38:00.726879Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:12.175359+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:12.175359+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"L., Brun, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:c03bbb50c79f1bcfa9e4829f64f38123414e8796873c9ff9a961638ae71d77b0","observation_id":"d1c45fae-d0df-451d-88ab-617e354f07e1","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"F., & Brown, S","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:8761be25e7738e88118bc0bb04341faa89bcb82b89362f0a2789da51505d6b80","observation_id":"61cce79f-51e9-482f-b084-b8e969f07ee0","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"F., & Landstreet, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:8087d83d382a4b7fa926fbebc399dae274dcf86fc5ce4be78f4724e75394f74d","observation_id":"c4b1b4a0-2269-4e98-958d-96cfe2e16785","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"J., Cohen, O., Yashiro, S., & Gopalswamy, N","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:040d8ae410c4528acd5cbe882f4a2e8f620e50cdc52d46e11e592709876b400f","observation_id":"30f90ce5-4b32-4d0f-b4d0-d63f51f0971e","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/stad1650","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"C., Carter, B","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"e26441c9-6107-4e01-97cd-6b99361f3052","year":2023},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:b38ce2873e1e9e9f63061a56f9e159848f3605079d80614d5f63d57873272bb3","observation_id":"93302754-f788-48b4-a4e0-5ddfb152376e","resolution":{"observed_at":"2026-07-11T12:38:01.071321Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:13.57936+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:13.57936+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.201713403","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2017, Astronomische Nachrichten, 338, 753, doi: 10.1002/asna.201713403","venue":"Astronomische Nachrichten","work_id":"4343dcbf-3ab8-4714-908e-c1df9b47e368","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:daaf81b21257e485a46c003c775d45277679701145b3befad7d0b90bf43fb797","observation_id":"68167787-7cba-4414-b5b3-aebd6271db66","resolution":{"observed_at":"2026-07-11T12:38:00.918294Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:14.176708+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:14.176708+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/697/2/1529","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2009, ApJ, 697, 1529, doi: 10.1088/0004-637X/697/2/1529","venue":"The Astrophysical Journal","work_id":"93ba4b81-3700-4659-8ca8-adc757e7a620","year":2009},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:6f685e848978d8a9540b326d9a917147847d2e498edabfe9098722e5c06f60a1","observation_id":"800eb573-e9f6-4a13-82be-121972cb69a2","resolution":{"observed_at":"2026-07-11T12:38:00.780739Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:14.619831+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:14.619831+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9909041","last_updated":"1999-09-02T09:57:31Z","snapshot_observed_at":"2026-07-07T01:28:06.445754Z","submitted_at":"1999-09-02T09:57:31Z","title":"Spectroscopic analysis of a super-hot giant flare observed on Algol by BeppoSAX on 30 August 1997","version":1},"cited_work":{"arxiv_id":"astro-ph/9909041","doi":"10.48550/arxiv.astro-ph/9909041","metadata_source":"pith","pith_arxiv_id":"astro-ph/9909041","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Spectroscopic analysis of a super-hot giant flare observed on Algol by BeppoSAX on 30 August 1997","venue":"astro-ph","work_id":"d6f6a48b-00ab-4471-ab44-c11fc0df6d34","year":1999},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"cited_paper":"/paper/astro-ph/9909041","citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:fcd7a247b3deb79aa39d7469de386aceea6daf0ab1762a7e9df5e2ea98c4d1bd","observation_id":"33c118db-ce0f-4077-822e-0177f589b681","resolution":{"observed_at":"2026-07-11T12:38:00.748466Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:14.980091+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:14.980091+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"P., Bouvier, J., Petit, P., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e1cb87fb7a6b0efb0b9e92f2682d10f72b49175d579bff619640af5ff279b93a","observation_id":"92225f9f-05b9-453e-af69-db257a3a9a77","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1029/2024gl114040","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"D., Fu, H","venue":"Geophysical Research Letters","work_id":"a2f90f03-b08c-47a9-bef8-7fc564f637ce","year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f936c599af49b3b88a901b0ae47838ed442f1ede99d02d6e646186ad8c99a5bb","observation_id":"3431940d-eea7-4abb-a9ee-a9dea3fe6918","resolution":{"observed_at":"2026-07-11T12:38:00.817015Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:15.409592+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:15.409592+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"D., Cohen, O., & Drake, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f657e3cf160f2f1d98b78a0090ececa9fa051398c53a14f5c78936b1523d3df5","observation_id":"e61fd928-f522-47ee-8f53-972b463dac86","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8205/833/1/l4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., & Cohen, O","venue":"The Astrophysical Journal Letters","work_id":"9bd2a0a7-af67-407b-9f9a-b11e054ec066","year":2016},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:544025953b6437ec68e0e38ac08cb5f627fd9826a79c782ea6613e5e94092bdc","observation_id":"251f0f6a-de3c-4e8c-8bfe-3b5571f4c7a0","resolution":{"observed_at":"2026-07-11T12:38:00.669836Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:16.351661+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:16.351661+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"E., & Low, B","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:38578401baa5209180e66bfa009013a3fe4600868345f5d786c35be86daccce4","observation_id":"b3d17f2e-bef0-4119-9cb7-dbbd528ac020","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:0224a98d0ff9a7f52ab0364c2fb114b2b6ff9a6b9330eb7aef4ff828823fa557","observation_id":"fa7be0e2-d038-46e6-b1db-ae47d1293f46","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"I., Chen, Y., Glocer, A., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:6367912ac0355b22a85d97b9e5ae4ebc3382bca33def110799e1d2f5f5001d4b","observation_id":"19ac2086-eb00-4099-93ed-7add904b330a","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04165","last_updated":"2025-01-07T22:55:22Z","snapshot_observed_at":"2026-07-06T18:41:44.784690Z","submitted_at":"2024-07-04T21:54:33Z","title":"The SOHO LASCO CME Catalog -- Version 2","version":2},"cited_work":{"arxiv_id":"2407.04165","doi":"10.48550/arxiv.2407.04165","metadata_source":"pith","pith_arxiv_id":"2407.04165","snapshot_observed_at":"2026-07-11T18:15:01.373222Z","title":"The SOHO LASCO CME Catalog -- Version 2","venue":"astro-ph.SR","work_id":"cf0efdcc-e925-46c2-a4f9-5ce6aed43d72","year":2024},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"cited_paper":"/paper/2407.04165","citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:22ba2b15b6222c6aaecc14530c3a81b2c7b056456e241ec1705a866977f6b090","observation_id":"9bbdbf2f-ba5f-4eb5-a9fc-54e1a1670221","resolution":{"observed_at":"2026-07-11T12:38:00.773539Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:18.600883+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:18.600883+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2009, Earth Moon and Planets, 104, 295, doi: 10.1007/s11038-008-9282-7","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:3cdcc6116f52fceb8764a7b8cbdc9640add7a5c90d0b8acae0a8caf14934c979","observation_id":"57036d69-17bf-4e17-9173-ffb6d8ff90e7","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2018, SSRv, 214, 46, doi: 10.1007/s11214-017-0462-5","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:7a6ed022540c957f7ba35f154f9032fd3a32385dd521521dd37f662aa3a0187b","observation_id":"355132b3-eca2-4c97-8302-3347f6bcdde7","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"3910.1002","doi":"10.1029/2019ja02763910.1002/essoar.10502458.1","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T18:15:01.373222Z","title":"2020, Journal of Geophysical Research (Space Physics), 125, e27639, doi: 10.1029/2019JA02763910.1002/essoar.10502458.1","venue":null,"work_id":"7fe8b043-be39-47c4-8915-2393ca3c03b5","year":2020},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:745bd35a25c5add76b018c55c549e49c4ef8973ad5e0d999ba0b2420b3f1ad98","observation_id":"8e7d3573-37db-4485-b1a7-08898ce9bc8d","resolution":{"observed_at":"2026-07-11T12:38:00.895347Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:20.137455+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:20.137455+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"W., & Emerson, J","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:9ded6359a5f33b53c4e213db6e31711a838765c72fe6e7b79f3e047e25f159d3","observation_id":"669e008e-6f44-4b96-aaae-bf8fe2992b33","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/stae2559","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A., Carolan, S., Villarreal D’Angelo, C., & ´O Fionnag´ ain, D","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"db16c1fb-68a9-40eb-b071-31b888a6b2a7","year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:23f9b18c96f3784d8a0237e5e448712b5abf1b4ac0b81c1fe01231b5a1d83291","observation_id":"1fe3fcf8-a98a-4d60-bb7f-47c34b4ded52","resolution":{"observed_at":"2026-07-11T12:38:00.767165Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:20.624852+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:20.624852+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"R., Foing, B","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:6244d78d7d40e823a7f859297967deb5c8065e7668803c5c6f94293d10e849e4","observation_id":"f33366a9-849f-4897-b5ab-0b493bafe3b1","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:500b19365563be1a9c7652333dab8240c8e3309ca707230249fc65cf44741871","observation_id":"f351d4c7-9b7c-465c-9282-a760e9be2d55","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/acb7e8","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, ApJ, 948, 9, doi: 10.3847/1538-4357/acb7e8","venue":"The Astrophysical Journal","work_id":"574ad79d-5356-458a-a699-00ae9edefd7b","year":2023},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ec94de9f651c1f865a411a3439b6771e654e6402e200c223746687e96ba250c2","observation_id":"8073c95b-3a6d-4ddc-8230-e098cbd12f1f","resolution":{"observed_at":"2026-07-11T12:38:00.900146Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:21.655979+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:21.655979+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ad5667","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"B., Enoto, T., et al","venue":"The Astrophysical Journal Letters","work_id":"04bfe1ca-a6a4-416a-b46c-55cebbe6d2c9","year":2024},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d723c3941b61bf2a426f4baefcf61bfbee7cdbd42cc6a9bf4625537c64ff38d5","observation_id":"09064755-026e-4e14-b019-3e2272dbf616","resolution":{"observed_at":"2026-07-11T12:38:00.724887Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:22.146593+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:22.146593+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2024, in AAS/Division for Extreme Solar Systems Abstracts, Vol","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:8ce68b746519ecc47c2e9d269e51d90ad8bc26fbb80c9b26ad2f21f4041d3e6b","observation_id":"5054807c-1dfb-46bb-b8ad-e75654366a47","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1086/378178","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Moon, Y","venue":"The Astrophysical Journal","work_id":"c510160e-5592-4ab8-a9dc-f0cf3cc8bf09","year":2003},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:96d416d921f91b33a864dacc5a39a2d29127fc0b1f96123a7c0697a30176f612","observation_id":"df3c15f5-4a97-4397-b31e-83201b588035","resolution":{"observed_at":"2026-07-11T12:38:00.787915Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:22.559652+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:22.559652+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"T., Yurchyshyn, V., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:bae4a4b37fbc78f29baa038c396cf157b7631e023e9ffba9a7a2046fe0f4c9ae","observation_id":"d65e706d-8154-4efc-869c-551ea5a534f8","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2021, Nature Astronomy, 5, 1126, doi: 10.1038/s41550-021-01414-z","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:32ad42ce77d321078e3e20ca765063d5986f6357eeea5fe59e6a561175d53ab7","observation_id":"18d595b3-074f-49fe-9172-f154111d7bb3","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"B., van der Holst, B., et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:990419df28bfdd98d5e62447f88c9f30460670666c82dba9d22b8f42cb99ee29","observation_id":"4a048d69-c8ab-4f16-a210-aadbc1e7fec0","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/s1743921320000575","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":"28990b58-8988-4c62-9906-cf5e72e94f05","year":2020},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f1f1a1def45c22efe2632a14013006afecd11a60843db282f612f4704f57e9cf","observation_id":"67930f4f-52a9-4087-99b2-0b5cdedf3a08","resolution":{"observed_at":"2026-07-11T12:38:00.748706Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:24.503572+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:24.503572+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"D., Albelo-Corchado, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:4e7511b7cd02903a2be206d99eccf43b93cdf13bc10cd24be08dc4503a827ce9","observation_id":"a25b7803-9f76-4e64-a736-791ac0310cf5","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"L., Ribas, I., Lammer, H., et al","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:799ab6452266d38515e3883f3555d5b386fc7037efdc7a7006ccd3246627ac03","observation_id":"82bf526c-37f4-4ec0-8b5e-90fad55cdb82","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1002/asna.201713310","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"G., et al","venue":"Astronomische Nachrichten","work_id":"59d9f801-310e-4de1-8e0e-ab18120da4c3","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:67b90e51bca03e45c1de03d864b73dd6001c9bea258cb8189003e3b9976a6ce0","observation_id":"086b080e-9be1-40e2-a4bb-7d3b557bc3aa","resolution":{"observed_at":"2026-07-11T12:38:00.881240Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:26.071644+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:26.071644+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"C., Vedantham, H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d172f2ddb9b1ea0d87888e400ebdbc6b7a5780273956fb8bfb37b15d489a8078","observation_id":"c62a15ae-24b3-4f27-bb8e-8639e1984d75","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:531be7e8d421887f48809e062a3f6b1a8c2b39562a168e8bc21889f2011019b5","observation_id":"3225d71b-6d5b-4f34-abcd-4349e48ac435","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1051/0004-6361/201117675","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2012, A&A, 539, A131, doi: 10.1051/0004-6361/201117675","venue":"Astronomy and Astrophysics","work_id":"78d70749-9dd9-4a97-be47-1316c3f22cb7","year":2012},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:08847709cf1b52d9f00fa643f2bb7c895658527738fdfcf0a52d98a6b7cd2f98","observation_id":"c7648ef9-1a87-4b27-9b50-c69fee91aed7","resolution":{"observed_at":"2026-07-11T12:38:00.883912Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:27.991863+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:27.991863+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:0c1f904123c7e3af837d50d1a5228dc61294f36a7534fd3aff307ed32dd7889d","observation_id":"45a100d2-6510-4c9b-b8e5-96a5322e9dd5","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1007/s11214-019-0605-y","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., Floyd, O., Boclet, B., et al","venue":"Space Science Reviews","work_id":"4c4115d7-bf10-4517-ad11-b75d2f18f94e","year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:540ce1cf088e5f163c9613829fb49c2fbc060c3b76a436c5b0ad8baeeca24c6c","observation_id":"45fda577-37b6-4139-859f-0b218bb148ad","resolution":{"observed_at":"2026-07-11T12:38:00.769913Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:29.114538+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:29.114538+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201015985","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2011, A&A, 536, A62, doi: 10.1051/0004-6361/201015985","venue":"Astronomy and Astrophysics","work_id":"c477705e-1d1f-4251-b75f-9f660c3fc230","year":2011},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d824c568eca4d9695aa423be00535dd65b036d6bc4e89c7b92a7b4328097b23e","observation_id":"44357c64-9b64-4eb8-912f-71286012221a","resolution":{"observed_at":"2026-07-11T12:38:00.758875Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:29.536062+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:29.536062+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2024a, Science in China E: Technological Sciences, 67, 1592, doi: 10.1007/s11431-023-2534-8","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:a63f0d8b03453d5c6decde74b646b056e1f44c14b5240996679fab2ff258d72b","observation_id":"ca53b04d-14e3-4e74-b62c-da2ef0de584b","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab3121","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2019, ApJ, 881, 151, doi: 10.3847/1538-4357/ab3121","venue":"The Astrophysical Journal","work_id":"7be16fe4-d905-44a9-b169-754bbac482f1","year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:7e626d4e91edb17b0ee65889fd4988771d69c2b6954214e876f62fca13fa3fb3","observation_id":"674cc17f-f177-4dcc-bf59-2797a0a80bab","resolution":{"observed_at":"2026-07-11T12:38:01.011738Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:30.523054+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:30.523054+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2024b, ApJ, 964, 159, doi: 10.3847/1538-4357/ad2e90","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e51b7fed86bd4b9c10aa0b20a121a6bd69be2d6b6c3b2936baa92dd313d4a3d2","observation_id":"19c46b4a-b56d-4d1e-91b9-760896fb165c","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2004, SoPh, 219, 169, doi: 10.1023/B:SOLA.0000021798.46677.16","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:47b3d09e57e2a0c9ab209551a8e1f0a81e6e8eb7a7d794d5ecd50050bad83356","observation_id":"a65089f2-9c9e-46b9-bc0b-4d3a3578fe86","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1086/428080","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"7ad4e0dc-5ac3-4340-9007-1bf6c825639f","year":2005},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:6eae5ba0224266f80272e4fa74d70508942331f79af79aa2979f10aeb5ca39d7","observation_id":"445f9b08-0692-450a-9f01-5a07fc1e3803","resolution":{"observed_at":"2026-07-11T12:38:00.923524Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:31.95278+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:31.95278+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1674-4527/20/10/165","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2020, Research in Astronomy and Astrophysics, 20, 165, doi: 10.1088/1674-4527/20/10/165","venue":"Research in Astronomy and Astrophysics","work_id":"a408d235-10c8-48de-9fdd-a9e7ba231c38","year":2020},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:6f33c94ab19fef22e8e3ef8c2dd8a9bf4aefb9290efe14a06ed5e03e11a91977","observation_id":"fb75aa66-c571-42a6-911d-5940e84fce31","resolution":{"observed_at":"2026-07-11T12:38:00.713775Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-07-12T06:30:07.952705+00:00","source":"paper_reference_links","state":"open"},"event_date":"2021-03-19","event_type":"correction","notice_doi":"10.1088/1674-4527/21/2/50","provenance":{"observed_at":"2026-07-11T03:02:26.424803+00:00","source":"crossref","source_record_id":"10.1088/1674-4527/21/2/50->10.1088/1674-4527/20/10/165:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac91c7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, ApJ, 938, 7, doi: 10.3847/1538-4357/ac91c7","venue":"The Astrophysical Journal","work_id":"461a0f20-4643-46c9-b40b-9361c0ec714a","year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:a96fad85936a2e9edb00ee5e822bb92a7988b9929b83ada6ee40ae32416a43df","observation_id":"93051e05-9c8d-4891-868f-c7e3dfbcfe77","resolution":{"observed_at":"2026-07-11T12:38:00.792307Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:33.103592+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:33.103592+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202142909","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2022, A&A, 663, A140, doi: 10.1051/0004-6361/202142909","venue":"Astronomy and Astrophysics","work_id":"3d1cac3f-d1b0-4382-8cca-6ca6baa0e213","year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ed5b1e5130b1c663ef50aecf48339d25dd6bd3ee12129d8cb5922deab488818d","observation_id":"28ebf56c-aa88-4cbc-8615-af67d12874e2","resolution":{"observed_at":"2026-07-11T12:38:00.753557Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:33.691453+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:33.691453+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2025, ApJL, 978, L32, doi: 10.3847/2041-8213/ad93cc","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:da097daec263ed376cadbb52fa1d14e8077de36390cbce9b8cd0734108f8d851","observation_id":"034dc684-fc95-4087-b701-609a7fe5a6a7","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"B., Gombosi, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:8d1f3d47b44660686970d04775321e229d30f5d2559bc63b166b0fc41ea8d563","observation_id":"7d6e381d-e82e-48fa-bf95-bd99519bacb1","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1051/0004-6361/202452071","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2024, A&A, 691, L12, doi: 10.1051/0004-6361/202452071","venue":"Astronomy and Astrophysics","work_id":"4c35787b-43ff-4972-ae84-b5c68f7c7c81","year":2024},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d5cc579ee8321feee047235e221faf57e4416e6e9caf1bdcfa514be50a4ad554","observation_id":"ef6b8398-7cb4-45b3-88a3-09d9ff64dfb4","resolution":{"observed_at":"2026-07-11T12:38:00.842956Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:35.173717+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:35.173717+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"L., Sterling, A","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:61ff34c6fe71eac04fe30621293ae0031fadd9456861e51b5668f1d95f21e9d6","observation_id":"aba2f079-07d2-44f5-974a-e68d9eedd092","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aa9520","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Cohen, O., Alvarado-Gomez, J","venue":"The Astrophysical Journal","work_id":"ab485380-5513-4157-8bb5-4fc8d8e57dcb","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:16eed0dab19bc586613d926a689da6646de38685b8fb194c98c9737cdaf12c37","observation_id":"c843c296-a20a-41d9-8c60-731a827e417d","resolution":{"observed_at":"2026-07-11T12:38:00.832705Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:36.133511+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:36.133511+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"J., Cohen, O., et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:9f87a35ee09f38de24f701024ffc5414d57dbf5fa2bc32d50ade8e7a27d48f91","observation_id":"ac28ee77-4f56-46a8-8d6a-7a5048ff4674","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1007/s11207-018-1287-4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A., Guerra, J","venue":"Solar Physics","work_id":"ad0af486-edc9-4a97-81d1-0100e523bd86","year":2018},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:8b2b586d7a5c9002d0d80368eb547404c7ca7ba5e4d04313f147882fd8e54a80","observation_id":"2f266fca-7f9f-45ed-a2ae-20e4e564ea69","resolution":{"observed_at":"2026-07-11T12:38:00.670139Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:37.123635+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:37.123635+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2021, Nature Astronomy, 6, 241, doi: 10.1038/s41550-021-01532-8","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:229310e16b521787e900caab9f6d040c18ddf998d683c4b469ac17057c9865ba","observation_id":"739a28b6-72ce-42f0-a71f-6effaeacc16f","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2026, Nature Astronomy, 10, 64, doi: 10.1038/s41550-025-02691-8 ´O Fionnag´ ain, D., Kavanagh, R","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d2ca9e595e6d272111cd118fc8f02dae5678d825831d523b6b4225fc5afce84f","observation_id":"9fc3afc4-2ad0-4c92-bda6-331bc675539a","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/stx1969","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2017, MNRAS, 472, 876, doi: 10.1093/mnras/stx1969","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"cd6f2ae1-d49a-49d9-98ec-c0ad4a98d194","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:4bcc16cd7c6164d4f1cbc248d344525b10809189ff2ed05597ac457b18bcef87","observation_id":"2fb2b670-302a-41fe-9396-4f6a2e3928e3","resolution":{"observed_at":"2026-07-11T12:38:00.690139Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:38.681942+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:38.681942+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/528792","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., Tsuneta, S., Lites, B","venue":"The Astrophysical Journal","work_id":"073f6271-38d0-4167-8824-c375f9e41c52","year":2008},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:3d1eb7e227e707271695c8e10b4cdd689d739d79921f50f69f8bf2ae768a2b3f","observation_id":"b31c2c81-2742-48a2-bb83-e48a84b5691e","resolution":{"observed_at":"2026-07-11T12:38:00.674703Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:39.089356+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:39.089356+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab8230","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"c47858b0-42ce-4968-a9b2-662dd3d186a9","year":2020},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:a75444e1bc38c9179ab09b9c78e3eabbc25619050235a3d888decc9bd3fdf084","observation_id":"bba095b1-ebd2-443e-b45a-d3ae355b83d5","resolution":{"observed_at":"2026-07-11T12:38:00.674513Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:39.490785+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:39.490785+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/adb8d3","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, ApJ, 982, 194, doi: 10.3847/1538-4357/adb8d3","venue":"The Astrophysical Journal","work_id":"8502fdff-6ba7-4c41-961e-d64bc00dabe3","year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:a09a9f5de863a01de121865601952dcc1ecd5f9c80959209c0579491770b31fd","observation_id":"dbdf024d-b1fa-4d52-a3a2-a80b97be84f7","resolution":{"observed_at":"2026-07-11T12:38:00.696931Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:39.980235+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:39.980235+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201630043","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"E., Valori, G., et al","venue":"Astronomy and Astrophysics","work_id":"0e4a9299-08ba-46a3-9b65-706bef5be026","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:5a009957f04b38b61da8a8bf1cfb78b2a806176f2978bb5067559c732404076f","observation_id":"5a3eca49-4b5c-482a-9b69-2681693ad27f","resolution":{"observed_at":"2026-07-11T12:38:01.054666Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:40.465976+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:40.465976+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/187324","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A., Canfield, R","venue":"The Astrophysical Journal","work_id":"9be9bfca-4952-4fb4-a938-cbc44de98a1d","year":1994},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:0d68c023ff60afa3ed0c4654e0861981dda1a301f48d31d859b9c7832843557c","observation_id":"9f2eeeb7-814a-4bcb-859c-69d1dc8e6447","resolution":{"observed_at":"2026-07-11T12:38:00.873840Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:40.821551+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:40.821551+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"A., Fisher, G","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e0222e99d970910a321f43106ba6173d4fb6c4ad1acca3660f6d6df45995c497","observation_id":"8d6c98be-abdc-4ce2-92ee-94860202f816","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"G., Roe, P","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:d7c72f8b54915922bdeef960bccdfeabaec7818c971b9026afac885c369db51b","observation_id":"3e97cfb3-9ef7-4333-83bc-609767e4c0b2","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2000, Magnetic Reconnection: MHD Theory and Applications, doi: 10.1017/CBO9780511525087","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ec5b246704c64ad7ca5ad4e2eaee45efd69e80be8e30bdd351913ba166fed785","observation_id":"ece68d6e-c06f-4a98-bbc9-39ca2da7a300","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae4bd9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, ApJ, 1000, 205, doi: 10.3847/1538-4357/ae4bd9","venue":"The Astrophysical Journal","work_id":"9a010db6-63e1-4273-9bb6-e3e1e7fe5fb4","year":2026},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f1e5fdb7030026e591ac5e5d64f35ffb54e1cafbecad770e0fde55f199bed895","observation_id":"0a308ed5-0a33-4c63-a55b-d5c19860220f","resolution":{"observed_at":"2026-07-11T12:38:01.046321Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:42.100135+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:42.100135+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/s1743921305000657","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"K., & Forbes, T","venue":"Proceedings of the International Astronomical Union","work_id":"3b086076-e5b4-4b73-b4c9-3716f59b73f4","year":2005},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:f6f485ec45f49d6ec042cd084f74d3a401fc5dc6f8fa89ad1b46d0f4a721e004","observation_id":"21a39f65-e089-4069-92c9-e7b3ad7b616c","resolution":{"observed_at":"2026-07-11T12:38:00.850640Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:42.517199+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:42.517199+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2012, Living Reviews in Solar Physics, 9, 1, doi: 10.12942/lrsp-2012-1","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:88632aa1efc3f71b9f4098656fbf1c417da57c1fafea1940dfd0cbee7e0a9a10","observation_id":"781459eb-0180-4c69-8e3a-0dd096be796c","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"J., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:163e0a8daa07b21c28181ffe430f3bf1672452754711e693c99b210ec4674d34","observation_id":"9452935c-8278-47ee-b7ab-4eb45ddb233a","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1086/320237","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., & Title, A","venue":"The Astrophysical Journal","work_id":"17684cb7-8325-4832-b683-b3d8216f929b","year":2001},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:ee457c10c62457d454a312364d00b696a6a43c8dc6e3d611708e8773c7952932","observation_id":"08a8598c-a88a-4aa3-aec4-71887da492d1","resolution":{"observed_at":"2026-07-11T12:38:01.038394Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:42.946036+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:42.946036+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stw3094","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"A., et al","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"bfb4af65-e4d6-4801-8c4a-73b53f915d63","year":2017},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:300f99141d62a1b10ebcf107f834f84897fb3e4e6712d058281b2b69fabd6183","observation_id":"886a5569-eea9-40d0-8485-a50b214f7452","resolution":{"observed_at":"2026-07-11T12:38:00.708281Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:43.567481+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:43.567481+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2022, Reviews of Modern Plasma Physics, 6, 8, doi: 10.1007/s41614-022-00069-1","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:b9733c947af88a522efd2f288ffe14ed939770780d097eda41c4d25065460fa6","observation_id":"84d9c430-52ff-4ea6-8d52-df21f783e5d2","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"2026-07-11T12:29:10.089534Z","title":"2019, A&A, 626, A86, doi: 10.1051/0004-6361/201935315","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:7f62d87917f8da7c514a9a539bd9045cf863ac8399e533770db79b2e6401ddcc","observation_id":"c80cf5e1-a695-45eb-ab38-771bedfbed21","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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/stab3249","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"Monthly Notices of the Royal Astronomical Society","work_id":"80e8380b-6028-4063-9857-1784635ecdde","year":2022},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:21790a8f3f8ef60c13ab6c6c47d4c376ac74e15b31ea31d06b301fde9c5cf28f","observation_id":"530ac6d3-63bd-4353-a1e6-86ff65c7148f","resolution":{"observed_at":"2026-07-11T12:38:00.870225Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:45.28129+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:45.28129+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"G., Hoeksema, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:0a776828ef56c9e618f61e80238bd14855ee4c3d732cda245f015e05592fe4f8","observation_id":"b50c77a9-861d-42f0-b53d-c93895402118","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/adf18b","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, ApJ, 990, 45, doi: 10.3847/1538-4357/adf18b","venue":"The Astrophysical Journal","work_id":"76c77cdc-d7ea-4011-9cd4-ace97144761e","year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:dd5dd26d8ee8399154468d0cff839bf39312a2120be7d07129191b549bd8bb99","observation_id":"db6fbcc1-238e-43ab-baad-ecaefcac5156","resolution":{"observed_at":"2026-07-11T12:38:00.806877Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:46.208598+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:46.208598+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ace5b1","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2023, ApJ, 953, 148, doi: 10.3847/1538-4357/ace5b1","venue":"The Astrophysical Journal","work_id":"8d125beb-6396-4bba-aaec-939076c2d9e2","year":2023},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e997f2102f04150b9d2d173e9183ed8ae5fe3ce283ef839faaa694d9e8924154","observation_id":"db2a4d2b-7d55-4fe5-8f4b-fb1e449c8e80","resolution":{"observed_at":"2026-07-11T12:38:00.861770Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:46.788433+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:46.788433+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202348734","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2024a, A&A, 686, A148, doi: 10.1051/0004-6361/202348734","venue":"Astronomy and Astrophysics","work_id":"9136ac8e-a890-4325-9517-6b8e544d44c7","year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:901352c8b05816e1147fa71f1ae52e724b9b79ada953e8986f4ac6a7ff31ce52","observation_id":"80949785-7341-4778-8186-3a8acbbe9803","resolution":{"observed_at":"2026-07-11T12:38:00.855363Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:47.278018+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:47.278018+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s11207-024-02329-4","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2024b, SoPh, 299, 93, doi: 10.1007/s11207-024-02329-4","venue":"Solar Physics","work_id":"69d966e7-ba49-4877-af80-5d5d0cd2e9ad","year":null},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:4854eba96984458b4a3985b462bf607322d7252b9ccdc1cea067df0509237ba5","observation_id":"85f990f0-0cec-482a-adc7-b9f429d8c7ca","resolution":{"observed_at":"2026-07-11T12:38:01.050320Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:47.841268+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:47.841268+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"2019, Living Reviews in Solar Physics, 16, 3, doi: 10.1007/s41116-019-0019-7 T´ oth, G., Sokolov, I","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:654d68de3c3602bfaef11d5709210ae3e3ecf29d3f9b93101037d07adb02b6ec","observation_id":"a4f4b94c-9450-45ef-83a4-21ad439d5bcd","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","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":"10.1029/2003gl018100","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2003, Geophys","venue":"Geophysical Research Letters","work_id":"fba476c5-7d0c-41b8-bf6e-24dd851deac0","year":2003},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:322d56d781dbbaf20b817cf95d2efa76d4bc9382101d81495d87c2ce6edcf75e","observation_id":"dc7f233b-2a8d-4821-afe5-f1688554e598","resolution":{"observed_at":"2026-07-11T12:38:00.983273Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-07-12T01:19:49.055008+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T01:19:49.055008+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-07-11T12:29:10.089534Z","title":"M., Odert, P., Leitzinger, M., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:317ddc0f837d6757a37dabff047c1de99942bf51926c1f1942fd236eada97c79","observation_id":"40e8242a-7664-4075-b3c1-fc2a73fa3ee5","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.19228","last_updated":"2025-05-25T16:44:19Z","snapshot_observed_at":"2026-08-08T23:47:36.891151Z","submitted_at":"2025-05-25T16:44:19Z","title":"Coronal dimmings and what they tell us about solar and stellar coronal mass ejections","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.19228","snapshot_observed_at":"2026-07-11T12:29:10.089534Z","title":"M., Dissauer, K., Kliem, B., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-07-11T12:29:10.089534Z"},"links":{"cited_paper":"/paper/2505.19228","citing_paper":"/paper/2607.04853"},"observation_digest":"sha256:e813cfe7e171516b99c6d835b72d38fd7f17503560806fa2e3893230229123ad","observation_id":"2c362b45-7d0c-43bf-aaab-898a3764ad6f","resolution":{"observed_at":"2026-07-11T12:29:10.089534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.04853","last_updated":"2026-07-06T09:29:29Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-06T03:12:05.039903Z","submitted_at":"2026-07-06T09:29:29Z","title":"How Magnetic Field Strength Affects Stellar Coronal Mass Ejection Dynamics"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":52,"verified_exact":47,"verified_fuzzy":0},"total_outbound_references":129},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 129 outbound references and 0 inbound Pith citation observations for arXiv:2607.04853."}