{"as_of":"2026-08-11T15:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a42cfc7ebd0de771b0fdacacf8ef2d161f01d3fd9c73fee59cd3a8b8c234bfe2","coverage":[{"denominator":47,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":47,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-30T15:57:50.423323Z","state":"measured"},{"denominator":47,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":47,"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/2605.22956/citation-record","integrity":"/paper/2605.22956/integrity","json":"/paper/2605.22956/citation-record.json","paper":"/paper/2605.22956"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.099543Z","title":"S., et al., 2000, ApJ, 528, 965","venue":null,"work_id":"917bfd42-30ab-44ed-a972-ec432dbe9916","year":2000},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:660c277e17dea7d4d3576d7da44f1502cdb8f5ab150aeff77f7556d71766b84f","observation_id":"b5ced898-db93-4b66-b8eb-e049a69a6d99","resolution":{"observed_at":"2026-07-08T15:05:04.100633Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.080727Z","title":"2010, A&A, 516, L2","venue":null,"work_id":"a20e5b2c-4005-43a4-b27b-4a6899713d5b","year":2010},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:196a5f2bf0e2566ad75110d4357af8c5246a895cea86632238780b9b76ac65af","observation_id":"91de3dd2-dfcb-4b4a-a921-d5271539b2ce","resolution":{"observed_at":"2026-07-08T15:05:04.081762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.085322Z","title":null,"venue":null,"work_id":"82287acd-eac1-47ca-90b0-ef435cd97002","year":2024},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:28e89694f5be5680f9e6a5438e869ef6717c5e3588107759633ee8cd9a1c8c2d","observation_id":"2a6861cc-5ba2-4c1e-9ee9-a6b812e466c5","resolution":{"observed_at":"2026-07-08T15:05:04.086393Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.090910Z","title":null,"venue":null,"work_id":"c76875ab-9749-4fd2-9f31-ae767a4e044d","year":1988},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:28a776fd6801ba24b7ec7a965865a690eae2dd198f9e48063d6885d1caac8e8f","observation_id":"b47f8400-1700-4b8e-87e3-66fd9387931d","resolution":{"observed_at":"2026-07-08T15:05:04.092137Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.069323Z","title":"H., & Willson, L","venue":null,"work_id":"340bbf13-8ef9-439a-82b2-edc78c32dced","year":1991},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:626e11ac47cc3e029db95bc6a6bdbe8a65a1dccec902522fe6ee14a395a0f2dc","observation_id":"8bf11752-664d-4d15-974c-46f3dc68e463","resolution":{"observed_at":"2026-07-08T15:05:04.070340Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.070907Z","title":"G., et al., 1988, ApJS, 68, 345","venue":null,"work_id":"a4b07128-ff3a-46d1-bacb-3371ad0ab462","year":1988},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:eb3ba256758f0663eeb59960a26913043fd12a3b1dd569a1fc5f8e541ede8601","observation_id":"2a227aea-2161-4045-a11f-5da80ad70ff7","resolution":{"observed_at":"2026-07-08T15:05:04.071979Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.053281Z","title":null,"venue":null,"work_id":"b7aed341-d8aa-4292-a2de-a166165a3157","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:0166a8872d07d11b43972bfec2df59270e53000fb9de7674014bc8f1e48740aa","observation_id":"46073153-ca12-40bf-b63c-e66a833acfb3","resolution":{"observed_at":"2026-07-08T15:05:04.054352Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.067745Z","title":null,"venue":null,"work_id":"5390cfe6-eadc-4fa5-96fc-31f73b8e7a34","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:ffed2cc3a16853ba104016142eb2d41507de0f966467c89c8b492664f7c321dc","observation_id":"8affd330-f989-47c3-9faa-e9a1d7de132a","resolution":{"observed_at":"2026-07-08T15:05:04.068790Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.105977Z","title":"K., et al","venue":null,"work_id":"9d3f774b-c41c-4864-936f-dd47d8e6c7c7","year":2022},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:35438765d1c57fb835189b4c789afd6da94e35bd732971694c063e42af8378b6","observation_id":"d7ab71f3-57e0-41f6-bea8-410f71b8b1e6","resolution":{"observed_at":"2026-07-08T15:05:04.107002Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.061428Z","title":"K., Cristofari, P","venue":null,"work_id":"fa89a986-8d6a-41b4-895f-6f853cb8584d","year":2026},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:ea188135dff70984e5550da91c5010f0de67dfedc2df2048b6d87bec1fe7b0e0","observation_id":"b4595914-8163-4260-8c17-b7a8f5bf6ed7","resolution":{"observed_at":"2026-07-08T15:05:04.062451Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.066110Z","title":"2023, A&A, 669, A155","venue":null,"work_id":"63b73614-fc24-46ac-beae-bb9944c98a19","year":2023},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:700a4b285a4a89398e653eec1001e5ef3504c360bf800e58e745c785b9dedacc","observation_id":"941d228f-c0d7-42b6-9a28-7f69e8991ea0","resolution":{"observed_at":"2026-07-08T15:05:04.067188Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/310043","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"L., & Dupree, A","venue":"The Astrophysical Journal","work_id":"14b180fa-5d6f-41dc-b867-88dbbef7c753","year":1996},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:2f8baab2e177c0667956e27820002a1400d568eaaf87d6ae7c353d285faa40f4","observation_id":"405bbd85-8afe-4d16-88aa-03f06f2215f8","resolution":{"observed_at":"2026-06-30T16:04:52.143400Z","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":"2026-05-25T17:54:22.708804+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-25T17:54:22.708804+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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.059867Z","title":"R., van Loon, J","venue":null,"work_id":"6e20d8e0-0686-4167-9b86-1b56b2992046","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:b1699e966f6b127113b773573cc1e41358eb7e1a952fb16380a6cb664ae62e00","observation_id":"3bc187d1-fe7f-46f2-8f5a-78ca20908a18","resolution":{"observed_at":"2026-07-08T15:05:04.060899Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.112943Z","title":"S., & Humphreys, R","venue":null,"work_id":"e4febaa0-ffe3-4369-97d7-b3fe5c252768","year":2019},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:b45c504a1297a9155c1613a7da806623a01e78ae97404b4ddd2c2719057045e4","observation_id":"51a138e2-c08f-4dab-90ac-b0a431656961","resolution":{"observed_at":"2026-07-08T15:05:04.114129Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.083769Z","title":"A., Decin, L., Richards, A","venue":null,"work_id":"2885afa9-25c0-428a-a0b1-856dcbb7649f","year":2022},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:2a66de09f6d330a67ad54c0e8038f2740f267671ad93854d57ee45faba763bf0","observation_id":"39c824fe-08c6-4892-8eba-31bc6b029dc3","resolution":{"observed_at":"2026-07-08T15:05:04.084802Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.088972Z","title":"J., & Olofsson, H","venue":null,"work_id":"7c285462-5461-4633-8ce1-bd78ad460551","year":2003},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:3b1516b3d6891448a8926068ae4c1e0a13db5fe87d62bbf367adcfea120eddb0","observation_id":"a6e878e3-f03a-49d4-9fa6-100ba07654a1","resolution":{"observed_at":"2026-07-08T15:05:04.090263Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.075796Z","title":"M., Brown, A., & Lim, J","venue":null,"work_id":"6d56a736-0147-4067-b072-600557f544fe","year":2001},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:755e19b684f2264fde8a94c35fa21ba57b7ac2e21ec5ebf2c5a6835926f5b46d","observation_id":"538a596d-eb1f-4db1-a0a2-696dd211f1aa","resolution":{"observed_at":"2026-07-08T15:05:04.076958Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.111020Z","title":"2008, A&A, 491, L1","venue":null,"work_id":"db54914a-7b66-4ec9-9683-2c36edbeb842","year":2008},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:5ec7c29c25732cd054c2b34fc1b5d30da6ef99713f933653b4293f72851aea24","observation_id":"4e5567ac-985f-4b69-8def-3eeea636879a","resolution":{"observed_at":"2026-07-08T15:05:04.112240Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.101186Z","title":"2018, A&ARv, 26, 1","venue":null,"work_id":"97f32b44-189a-4d54-a49a-1a215d6229ba","year":2018},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:b078ea5b8b3c57370c4cb8c1e28f9c420a31de622051e1018c331a33197dea6c","observation_id":"5d9b4431-a3c9-4695-ac2e-065b17a3d12f","resolution":{"observed_at":"2026-07-08T15:05:04.102218Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.077608Z","title":"M., Ziurys, L","venue":null,"work_id":"0666ddf6-be30-4827-a6fc-fb5a0cf26b4d","year":2019},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:892cd91bf42130d2d7cb3bb8f9c175ae3bf42dcb10738328debdecda6f3f58e0","observation_id":"863cc67e-e1cf-4dd8-9aa8-fa01e67f28b1","resolution":{"observed_at":"2026-07-08T15:05:04.078646Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.114718Z","title":"M., Richards, A","venue":null,"work_id":"ccc3cc29-65f2-428a-8036-b72b58060b4f","year":2024},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:91ec3f21a4f7c7b93bd47f870fb94bf05e29889e8a8e92f816e3c2c9c89d1a9d","observation_id":"fb15989c-ebb2-4159-ac20-16415e8ebfe8","resolution":{"observed_at":"2026-07-08T15:05:04.115780Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.092705Z","title":"M., Jones, T","venue":null,"work_id":"1f47a332-ee45-4ba8-be1a-286fb0815685","year":2025},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:093ff33908507e4702b223aef341857d88db66cc43ccfc7ca091e4e7d94c2ea7","observation_id":"187765a4-5bea-4b9e-a498-9edd3299325e","resolution":{"observed_at":"2026-07-08T15:05:04.093795Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.107527Z","title":"J., Humphreys, R","venue":null,"work_id":"eb07a9d7-12e0-4971-8d12-d5e9b7e2fba9","year":2025},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:36bb6cee3b8393d7cf8f516615163232566781cdad9b4f39e44bffc983a9fe78","observation_id":"d8aa856b-0844-4366-bd12-99a3891fd7f2","resolution":{"observed_at":"2026-07-08T15:05:04.108587Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.097554Z","title":"R., & Luttermoser, D","venue":null,"work_id":"a444410d-a30e-4a50-8e2c-170fea943a79","year":1987},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:99361f389d8add8f7c54d8161420d0e619fb34919869b195d4095b4b3c6d99dc","observation_id":"7c828fe8-ffbf-416f-984b-330d6e896694","resolution":{"observed_at":"2026-07-08T15:05:04.098733Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.064545Z","title":"G., & Stencel, R","venue":null,"work_id":"48975cfe-a7ba-4593-8ed9-5acb7872595f","year":1991},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:a3adfd2a7298ab8f4d0cb14ebb3a36d85bb502723ddba56e4a438bf4059e5565","observation_id":"83ab6aa0-178e-4329-a8ee-96359f347a7b","resolution":{"observed_at":"2026-07-08T15:05:04.065557Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.079190Z","title":null,"venue":null,"work_id":"b76118dc-ebff-4b11-9113-b086c6ca31f0","year":2016},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:1e9c2e9c8aeac05c2dbf235939656183695e7a6c14fd67e3051b94a45ad19978","observation_id":"3ecfa6fa-6c3b-44f8-a68b-2af620f1dd64","resolution":{"observed_at":"2026-07-08T15:05:04.080206Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.119663Z","title":null,"venue":null,"work_id":"fe0cedb0-117e-44e9-a5b8-cef5516ce497","year":2019},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:199bcefe7263ff0b0664d9620df9a04e9a6aefc8193b8e5771f4c91fd19caabb","observation_id":"01bd42d8-ae52-4850-9fdf-4fc6cea9759d","resolution":{"observed_at":"2026-07-08T15:05:04.120716Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.116429Z","title":null,"venue":null,"work_id":"8423f956-a461-4430-8800-9d5abd517ea0","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:482f02e0944c84cecffcbb169290337b847bdf423fd3bb83dee169a467a65643","observation_id":"f58da268-53ff-4714-bc89-2a28505e91a1","resolution":{"observed_at":"2026-07-08T15:05:04.117526Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.00231","last_updated":"2025-03-31T21:13:41Z","snapshot_observed_at":"2026-08-08T17:00:07.612446Z","submitted_at":"2025-03-31T21:13:41Z","title":"The Case for High Resolution Spectroscopy in the Ultraviolet","version":1},"cited_work":{"arxiv_id":"2504.00231","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2504.00231","snapshot_observed_at":"2026-06-30T16:04:53.056881Z","title":"L., et al","venue":null,"work_id":"1df9b9b7-e42e-4576-a25c-babdbc5c2e27","year":2025},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"cited_paper":"/paper/2504.00231","citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:c4e9d72053e41d7b57db3b92c11236c6706a2243b9c6c0e9891cebd97f205503","observation_id":"0b7768aa-a07c-4865-9bbd-e614e4f61fc1","resolution":{"observed_at":"2026-06-30T16:04:53.058168Z","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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.118073Z","title":null,"venue":null,"work_id":"f1b953ec-f225-4336-af6f-72822f6ba8be","year":2000},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:9adf1c74244e2734bc92524ebd1335f1c5060a52998d87fb619c0b85cf004b73","observation_id":"5765a042-a01c-4016-9b37-5d8fb1545a0a","resolution":{"observed_at":"2026-07-08T15:05:04.119099Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.121424Z","title":"G., Johnson, H","venue":null,"work_id":"c0132ff6-03d2-42c2-9534-d5dda04a2ed2","year":1989},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:89f678d8b9123558b0958caf7fa89555878def432dfbba681f4da846c9ab87e4","observation_id":"ded85b5b-ec56-4826-b030-d725bf3e36c0","resolution":{"observed_at":"2026-07-08T15:05:04.122491Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.072665Z","title":null,"venue":null,"work_id":"bb281644-dee6-4bb2-b8b4-5ff99becaf24","year":2009},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:0fed85c9aaa20181985c459125bb26d1b1d74f8cf99456ce2d154d007aa29296","observation_id":"0be04ac2-9f4d-44e3-909e-ec0d7505a027","resolution":{"observed_at":"2026-07-08T15:05:04.073701Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.062995Z","title":null,"venue":null,"work_id":"be9f398c-8eff-4738-b707-6d984d0a30d7","year":2024},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:51ecb7b7779aab10fb5eb6aa869b3e333c703c0cbea3f1d72758495860fdefee","observation_id":"57b47298-6bca-46d7-948f-8deeb49340d6","resolution":{"observed_at":"2026-07-08T15:05:04.064004Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.086995Z","title":"2012, A&A, 546, A105","venue":null,"work_id":"e8fcf3e5-0db2-4f07-8290-a5b4e6422a1f","year":2012},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:bcfae9f0ec3838a7b9e55803c8cf0c5722ae8647da6d74d757f5d9cb6e6dc694","observation_id":"04d1ffd2-8ce3-4fc2-b93e-18407dff83c3","resolution":{"observed_at":"2026-07-08T15:05:04.088279Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.056687Z","title":"M., et al","venue":null,"work_id":"393993b6-97ec-4761-b5e6-5941abe302d0","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:e94df12b1eec7e091dfe7d19bc8959616ae3f9911b44d8d5d19c3afc16157e8f","observation_id":"300727a9-c84a-4260-8d06-c49f56ea05c2","resolution":{"observed_at":"2026-07-08T15:05:04.057762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.094328Z","title":"M., Ohnaka, K., et al","venue":null,"work_id":"63c046fa-741c-4d6d-9622-784bc45120a8","year":2020},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:5c54f5e75f1e1bb6f9013ecf3a7f4b2e6a5bb7d69895335ef10f62417d68e440","observation_id":"e91b7438-4fc0-47fa-a648-2f80ab3af40d","resolution":{"observed_at":"2026-07-08T15:05:04.095388Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.048021Z","title":"2011, A&A, 529, A163","venue":null,"work_id":"a8edc10e-1dae-420d-95a3-29868c1ad0e7","year":2011},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:c615c0d9a8a605566882567cc743c954b0289a8be74bfeb0bda7db33ce2c0e63","observation_id":"f6204c9f-5190-4010-b17d-6efefe2284bb","resolution":{"observed_at":"2026-07-08T15:05:04.049116Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.051410Z","title":null,"venue":null,"work_id":"664ffa23-e250-4135-86cb-096542c0be18","year":2019},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:601b27eec0dcfeb1ab5ee5fd139e06d946ffef36b148ae0bda6ed931580fba58","observation_id":"64032ab6-9a2e-4ebe-943e-5647ba8b9830","resolution":{"observed_at":"2026-07-08T15:05:04.052520Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.082273Z","title":"2018, Nature, 553, 310","venue":null,"work_id":"5ed9a639-73ac-448c-a351-72bbc71c95f3","year":2018},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:4f08cf81e371272dc7b08cee4983efdd594ff8e50f8ce13ac80c76891d989c3f","observation_id":"f7f36496-3e13-4c35-9794-5f2e54e550ff","resolution":{"observed_at":"2026-07-08T15:05:04.083254Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.095908Z","title":"2017, A&A, 605, A126","venue":null,"work_id":"b03056bd-0928-45e6-9e29-94a43901b1dc","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:b13a3d3667134ea4eeb10b09a7f36ad086b61507925ee3c90ee757eb859fa51f","observation_id":"a5487f41-6ad5-4c47-8b2e-2e9d7709944c","resolution":{"observed_at":"2026-07-08T15:05:04.096979Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.109136Z","title":"2026, in prep to be submutted to A&A","venue":null,"work_id":"d466bb3a-41c6-430b-863c-107d44ae821d","year":2026},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:09574ea7262e27ea9289b2c4bab5dae8046c886ffd178a5fd5b4e8a53908a564","observation_id":"aee30e34-9d52-4f7d-b75b-251197ae7b89","resolution":{"observed_at":"2026-07-08T15:05:04.110297Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.102766Z","title":"E., et al., 1981, MNRAS, 196, 47P–53","venue":null,"work_id":"5a716163-4563-4718-b1b5-c9f186ca4c94","year":1981},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:8052664316ab6cfa76306f110d15ae48f813e661c426e6cdfb2bc608b659989d","observation_id":"2dbba4a4-f934-4c20-b3e7-f1888f5cdb2c","resolution":{"observed_at":"2026-07-08T15:05:04.103868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.054901Z","title":null,"venue":null,"work_id":"c3b0c52c-cd26-408d-97f1-6c07351bb5fd","year":2025},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:4efcf0e53626b4b6f2c3faa04cd72b419050219a11fd673e8f04053c562ede54","observation_id":"11d9952a-2670-4b94-b72b-4d0ec34100d8","resolution":{"observed_at":"2026-07-08T15:05:04.056125Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.058325Z","title":null,"venue":null,"work_id":"eb90601d-8618-47d9-bd7c-02d1f3167f03","year":2017},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:ec716b8f9bafed60512189d0e15b1fac3502cfed6642a4501e2fc1c87360954c","observation_id":"0568e994-4684-49f5-ba39-dc16e7d6e7ef","resolution":{"observed_at":"2026-07-08T15:05:04.059356Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.074224Z","title":null,"venue":null,"work_id":"5b36e7c0-ef26-4790-9825-37e9d1062da8","year":2006},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:7efd5b220ae76b5c373b8051cb9a1d5953b0a8a444bd05393a871176b1a99cc1","observation_id":"97b92384-bdf5-416a-aa49-7e36a7441aa0","resolution":{"observed_at":"2026-07-08T15:05:04.075222Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.104423Z","title":"E., Karovska, M., & Hack, W","venue":null,"work_id":"c9dfe884-8d0a-4927-861c-60de5231fa07","year":2000},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:49e781b0f0e2d6d5aadecc761e5de634094a0e716b818e4c1c63f7b96d7044a6","observation_id":"f5d68733-fc3b-44b1-bd8c-43425d098ce5","resolution":{"observed_at":"2026-07-08T15:05:04.105444Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T15:05:04.049775Z","title":"E., Harper, G","venue":null,"work_id":"89a4e32b-95c3-4cde-9118-9af6add56da9","year":2024},"citing_paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-30T15:57:50.423323Z"},"links":{"citing_paper":"/paper/2605.22956"},"observation_digest":"sha256:980531b014a88f96bf12d2b6e04f096e2a1c70daf0ff297d9c24af869f0cbe83","observation_id":"e21036d2-858f-4f91-9093-85a0f149c651","resolution":{"observed_at":"2026-07-08T15:05:04.050834Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.22956","last_updated":"2026-06-06T21:38:43Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-07-06T23:33:14.457450Z","submitted_at":"2026-05-21T18:43:35Z","title":"The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars"},"reference_resolution":{"displayed":47,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":14,"verified_exact":2,"verified_fuzzy":31},"total_outbound_references":47},"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 47 of 47 outbound references and 0 inbound Pith citation observations for arXiv:2605.22956."}