{"as_of":"2026-08-13T00:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:698815f809c13071f73a78201f3f161a816d418b1ce7a9f4c72ebbfbff465fc4","coverage":[{"denominator":125,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T14:37:35.274600Z","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":"2026-08-12T06:34:41.77262+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/2608.10909/citation-record","integrity":"/paper/2608.10909/integrity","json":"/paper/2608.10909/citation-record.json","paper":"/paper/2608.10909"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.806610Z","title":"doi:10.1007/978-3-642-30304-3 , adsurl =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.806610Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:3344ad878206f8926a54fcfdbf7bcf38baaca5e468cfcdfb0c32888ab6fef67d","observation_id":"388fa599-5273-4954-9bdd-729971c79652","resolution":{"observed_at":"2026-08-12T14:37:34.806610Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02714","last_updated":"2019-04-11T14:25:45Z","snapshot_observed_at":"2026-08-12T23:12:32.136561Z","submitted_at":"2019-04-04T18:00:00Z","title":"The dependence of convective core overshooting on stellar mass: reality check, and additional evidence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02714","snapshot_observed_at":"2026-08-12T14:37:34.811626Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.811626Z"},"links":{"cited_paper":"/paper/1904.02714","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d68f01c00ac21111d78de75fd1b6b07774b3f688bc4ba1b9c7241c78c21d742e","observation_id":"055df4ff-d8ec-42eb-a825-60349dd67955","resolution":{"observed_at":"2026-08-12T14:37:34.811626Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.03523","last_updated":"2018-08-28T12:01:00Z","snapshot_observed_at":"2026-08-12T23:12:32.368548Z","submitted_at":"2018-08-10T13:16:19Z","title":"Significant uncertainties from calibrating overshooting with eclipsing binary systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.03523","snapshot_observed_at":"2026-08-12T14:37:34.816885Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.816885Z"},"links":{"cited_paper":"/paper/1808.03523","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:509bc15866a21d22b3a1ce85e4f29d66477a9e8c5412f99faee582c36151b5e8","observation_id":"fd0d35f1-e656-4807-9255-cb28a483a80f","resolution":{"observed_at":"2026-08-12T14:37:34.816885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.11302","last_updated":"2021-02-22T19:00:38Z","snapshot_observed_at":"2026-08-02T20:46:09.749665Z","submitted_at":"2021-02-22T19:00:38Z","title":"Cepheids with giant companions. I. Revealing a numerous population of double-lined binary Cepheids","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.11302","snapshot_observed_at":"2026-08-12T14:37:34.822345Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.822345Z"},"links":{"cited_paper":"/paper/2102.11302","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:93aaa4d290cdafd30ac035fee4c4a0e35ee5b92fb33a8e04c4838c99ef831bc5","observation_id":"6aada1b3-46ed-4dff-a206-69bb1aca81f0","resolution":{"observed_at":"2026-08-12T14:37:34.822345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.827329Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.827329Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:cb98e733606fd592e7d87a183091b32843dad2d0ca55e7157ce192f6441d2b77","observation_id":"9791004a-2d08-4680-a019-b45216c0de86","resolution":{"observed_at":"2026-08-12T14:37:34.827329Z","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/andp.18792440910","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.926169Z","title":"u ber die H \\","venue":null,"work_id":"e746f988-3b97-4f54-9909-3c8b41f4d474","year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.832348Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:7d2fa411a6d0010d61685b16a5a7ee61a62ebe177ec34fb222c3c3cae08c0fd3","observation_id":"48225f8f-c6fa-4caa-ae33-3ef1caa9a7ee","resolution":{"observed_at":"2026-08-12T14:37:35.931969Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.0622","last_updated":"2010-05-04T20:00:31Z","snapshot_observed_at":"2026-07-06T02:09:56.593540Z","submitted_at":"2010-05-04T20:00:31Z","title":"Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations II. Predictions and Tests of the OGLE-III Fundamental-Mode Cepheids","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.0622","snapshot_observed_at":"2026-08-12T14:37:34.837245Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.837245Z"},"links":{"cited_paper":"/paper/1005.0622","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:9544ef75b986f9a0444b9995739c2290d7f1beac056b23d76746a60cdb2f5320","observation_id":"659bfcbc-8609-404c-9c43-45d73e018c08","resolution":{"observed_at":"2026-08-12T14:37:34.837245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.2793","last_updated":"2008-09-16T20:10:56Z","snapshot_observed_at":"2026-07-06T01:43:39.383145Z","submitted_at":"2008-09-16T20:10:56Z","title":"On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation. II. The Effect of Metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.2793","snapshot_observed_at":"2026-08-12T14:37:34.842514Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.842514Z"},"links":{"cited_paper":"/paper/0809.2793","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:50311a8f0887d0aeade37f39735648ff58c826493ab8206df550c42dd1868d64","observation_id":"6ffca1bb-6f02-4fc1-9c5f-721af33dbb59","resolution":{"observed_at":"2026-08-12T14:37:34.842514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.3001","last_updated":"2008-10-16T23:05:29Z","snapshot_observed_at":"2026-07-06T01:46:48.327938Z","submitted_at":"2008-10-16T23:05:29Z","title":"Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.3001","snapshot_observed_at":"2026-08-12T14:37:34.847256Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.847256Z"},"links":{"cited_paper":"/paper/0810.3001","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:52f2d922db359e5ff5aefd259e25e5cce3de13ad50bce8254a19d843b4e31242","observation_id":"aafe628d-d07e-41c4-9bc4-b18d4a30d1ad","resolution":{"observed_at":"2026-08-12T14:37:34.847256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.4198","last_updated":"2008-03-28T20:04:27Z","snapshot_observed_at":"2026-08-01T19:19:06.020520Z","submitted_at":"2008-03-28T20:04:27Z","title":"On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.4198","snapshot_observed_at":"2026-08-12T14:37:34.852063Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.852063Z"},"links":{"cited_paper":"/paper/0803.4198","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:01645c06dd07e63067353245e7031f2422880af6690169971ee447db42da2915","observation_id":"4cc967b2-6e3d-4fe7-9bb9-d2a35cc7b23d","resolution":{"observed_at":"2026-08-12T14:37:34.852063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.1638","last_updated":"2011-04-08T20:00:06Z","snapshot_observed_at":"2026-07-06T02:26:03.723768Z","submitted_at":"2011-04-08T20:00:06Z","title":"The Cepheid mass discrepancy and pulsation-driven mass loss","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.1638","snapshot_observed_at":"2026-08-12T14:37:34.856737Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.856737Z"},"links":{"cited_paper":"/paper/1104.1638","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:47c1ff8cb8d34391cb5de8b0daccf546e1df0b14abd3cf1ae3e94298847daea3","observation_id":"0156e42a-f3a2-42bc-a784-a602cbc28fe8","resolution":{"observed_at":"2026-08-12T14:37:34.856737Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.01183","last_updated":"2024-11-02T08:51:18Z","snapshot_observed_at":"2026-08-12T22:09:17.834554Z","submitted_at":"2024-11-02T08:51:18Z","title":"Stellar Pulsation and Evolution: a Combined Theoretical Renewal and Updated Models (SPECTRUM) -- I: Updating radiative opacities for pulsation models of Classical Cepheid and RR-Lyrae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.01183","snapshot_observed_at":"2026-08-12T14:37:34.862071Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.862071Z"},"links":{"cited_paper":"/paper/2411.01183","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:f28bf56c7ca12c796058980b0c79eac1c1c8c20065e6af67879f640a60ad3bc1","observation_id":"01b96ff5-3185-4d5d-9d89-023fabafbec3","resolution":{"observed_at":"2026-08-12T14:37:34.862071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.868081Z","title":"Models fitted to evolutionary tracks","venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.868081Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:46cb690d4eb1cff7644b2e8f586e5c694553ce3a05ea089137b543bf93f62563","observation_id":"8f3b43ec-dab4-4085-9df0-16266c6b7d1a","resolution":{"observed_at":"2026-08-12T14:37:34.868081Z","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/144.4.511","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.894727Z","title":"Models fitted to a new mass-luminosity relation","venue":null,"work_id":"ca86699c-8163-4432-8a1c-04af6b9453b5","year":1969},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.873608Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:91dd0c21aaac30829f263b87deb5a80f76e277935d410894f2df4352964ce5be","observation_id":"d7fdcaf4-3bdf-4461-8f58-682677f20019","resolution":{"observed_at":"2026-08-12T14:37:35.905317Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.878520Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.878520Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:b2898922cd7b4ff9fe6105ab64bfbcbce0cb6f8ff77226d8a753010b5e0daf6e","observation_id":"3c117d6e-1596-48d5-b5e9-06052c2a8a5b","resolution":{"observed_at":"2026-08-12T14:37:34.878520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.03464","last_updated":"2021-07-07T20:06:58Z","snapshot_observed_at":"2026-07-06T11:27:04.968794Z","submitted_at":"2021-07-07T20:06:58Z","title":"Using classical Cepheids to study the far side of the Milky Way disk. II. The spiral structure in the first and fourth Galactic quadrants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.03464","snapshot_observed_at":"2026-08-12T14:37:34.883828Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.883828Z"},"links":{"cited_paper":"/paper/2107.03464","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:ef96caadac3451524b0cb60071eca410f8491f5f3692ccde5a12ea7cfa6b07aa","observation_id":"6caa13f8-ed50-4890-b69f-322a3d0bceb1","resolution":{"observed_at":"2026-08-12T14:37:34.883828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.08220","last_updated":"2019-04-17T12:21:28Z","snapshot_observed_at":"2026-08-04T18:31:45.206587Z","submitted_at":"2019-04-17T12:21:28Z","title":"OGLE-ing the Magellanic System: Cepheids in the Bridge","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.08220","snapshot_observed_at":"2026-08-12T14:37:34.889110Z","title":", keywords =","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.889110Z"},"links":{"cited_paper":"/paper/1904.08220","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:f63df860955ca6efddcf59c43c082897a6341da158ffaae1d71e04dca83562a9","observation_id":"de4c61b7-3d9f-440b-b030-0317bf8ed2a5","resolution":{"observed_at":"2026-08-12T14:37:34.889110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.09141","last_updated":"2016-07-12T10:23:54Z","snapshot_observed_at":"2026-08-09T12:31:16.020516Z","submitted_at":"2016-02-29T20:59:18Z","title":"OGLE-ing the Magellanic System: Three-Dimensional Structure of the Clouds and the Bridge Using Classical Cepheids","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.09141","snapshot_observed_at":"2026-08-12T14:37:34.894008Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.894008Z"},"links":{"cited_paper":"/paper/1602.09141","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:ace4dcee9fb2f444292e4312353ac6fd6a3af5636108796b718f2a3b3c859063","observation_id":"e9577f31-41a6-40f7-a5f7-f57588403f21","resolution":{"observed_at":"2026-08-12T14:37:34.894008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0012376","last_updated":"2000-12-18T22:35:25Z","snapshot_observed_at":"2026-07-07T00:14:52.553775Z","submitted_at":"2000-12-18T22:35:25Z","title":"Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0012376","snapshot_observed_at":"2026-08-12T14:37:34.898321Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.898321Z"},"links":{"cited_paper":"/paper/astro-ph/0012376","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:ea5e9abaf63f8ee192bf15ce4f2d2a5bfefa256cf0d726ce04448f092d2a3227","observation_id":"da9ad911-7749-48ff-a4b5-5f4952a03200","resolution":{"observed_at":"2026-08-12T14:37:34.898321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.902522Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.902522Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:99214be6c1e35ffa7568f9463e5b7ffa7b1bf8932d1a74daf75efab956ee9b85","observation_id":"777bc6e1-8edc-42b6-aab3-c55678a4288b","resolution":{"observed_at":"2026-08-12T14:37:34.902522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.906719Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.906719Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:7f791567095e56e0d8c50ed0d398cdeb72cc68b34a852d25d755688be611373b","observation_id":"9f480c9f-7790-4f10-ae4c-45aae21a42b7","resolution":{"observed_at":"2026-08-12T14:37:34.906719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.910618Z","title":"Origin and Evolution of the Elements , year = 1993, editor =","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.910618Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:97dc728af0b108270452df7a4f6cf0d76f9bf0285e851ad770c72828b8560c44","observation_id":"34a3a622-91ea-4146-8ed1-2c6e19dc83e2","resolution":{"observed_at":"2026-08-12T14:37:34.910618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.915187Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.915187Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:6f64089fa574d37e9f104d047ecf81f06b2083c02865ac4dbb311dee11a17408","observation_id":"0e174198-c445-46e7-b123-8ad79cd0f30a","resolution":{"observed_at":"2026-08-12T14:37:34.915187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.1979","last_updated":"2008-09-11T12:42:30Z","snapshot_observed_at":"2026-08-12T16:01:32.518589Z","submitted_at":"2008-09-11T12:42:30Z","title":"Convective hydrocodes for radial stellar pulsation. Physical and numerical formulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.1979","snapshot_observed_at":"2026-08-12T14:37:34.919619Z","title":"Physical and Numerical Formulation","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.919619Z"},"links":{"cited_paper":"/paper/0809.1979","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:cc1d4aa640598dd4d64a5b349716fe95fecd8b5d0277b6483d64d9b57371ce12","observation_id":"c68b31d0-7cfd-448d-8597-70a67cfebd07","resolution":{"observed_at":"2026-08-12T14:37:34.919619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.925142Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.925142Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:a97a7f8c0f6b8d66b323bc5063318f31e241f60b4e18a4a1fc63da1741211b34","observation_id":"078ca03b-cfd6-4e89-985f-f782f707e999","resolution":{"observed_at":"2026-08-12T14:37:34.925142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.929540Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.929540Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:170641f244f754d5eb46d0bc0c4ac3259fb00f25445b097a01ddf50ed71724bf","observation_id":"c2d5dbc2-866e-4c51-9ca8-1c6346344d26","resolution":{"observed_at":"2026-08-12T14:37:34.929540Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9907194","last_updated":"1999-07-14T19:50:18Z","snapshot_observed_at":"2026-08-11T22:31:32.195081Z","submitted_at":"1999-07-14T19:50:18Z","title":"The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9907194","snapshot_observed_at":"2026-08-12T14:37:34.934862Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.934862Z"},"links":{"cited_paper":"/paper/astro-ph/9907194","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:a87a4c077455a88c58d5fbeffb20c4212b42f36bfa7b5e4221fc4b88ae6c173f","observation_id":"1d1feecd-a9d0-4b86-8a9e-d0d31b3df985","resolution":{"observed_at":"2026-08-12T14:37:34.934862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807286","last_updated":"1998-07-28T14:39:25Z","snapshot_observed_at":"2026-07-07T01:21:39.736900Z","submitted_at":"1998-07-28T14:39:25Z","title":"The NextGen Model Atmosphere grid for $3000\\le \\Teff \\le 10000\\K$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807286","snapshot_observed_at":"2026-08-12T14:37:34.939594Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.939594Z"},"links":{"cited_paper":"/paper/astro-ph/9807286","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:c1c6d93cd0d98ef3e44dec82d703fcafd158faa9f70963ad55fad670281a2317","observation_id":"7a57f46e-43cf-4aae-8975-5a95db662889","resolution":{"observed_at":"2026-08-12T14:37:34.939594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.944649Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.944649Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:eac1b6ec521619d0606256379fd734582b44c02179f0ab356a4cf823c5f43f7b","observation_id":"5a552c5a-fad6-423a-a02f-ede2cf9d1c83","resolution":{"observed_at":"2026-08-12T14:37:34.944649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.948913Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.948913Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:5397036863cd4fd463a5ed2c433cd882d600fa6ff519ab6976b51bd0edf812b6","observation_id":"19ae4c0f-5807-4af0-82df-9fcc176bac0f","resolution":{"observed_at":"2026-08-12T14:37:34.948913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.953340Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.953340Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d2ad67435767285b27e9adc9aaf4d262cf6f93e742bc70e8d17248f17f00ad1b","observation_id":"0b2472eb-e6e7-4b2e-94b7-2531f4db28d0","resolution":{"observed_at":"2026-08-12T14:37:34.953340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0009261","last_updated":"2002-04-03T15:04:53Z","snapshot_observed_at":"2026-08-11T01:10:49.704752Z","submitted_at":"2000-09-16T10:05:02Z","title":"Equation of state of fully ionized electron-ion plasmas. II. Extension to relativistic densities and to the solid phase","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0009261","snapshot_observed_at":"2026-08-12T14:37:34.957808Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.957808Z"},"links":{"cited_paper":"/paper/astro-ph/0009261","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:17be07b4092e33db74e9adb285845ba9dce05914353efe762bdf40bd83a821f6","observation_id":"e65985db-e721-4265-9665-ab3f912c2f1c","resolution":{"observed_at":"2026-08-12T14:37:34.957808Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.0690","last_updated":"2010-01-05T12:19:31Z","snapshot_observed_at":"2026-07-06T02:04:42.018285Z","submitted_at":"2010-01-05T12:19:31Z","title":"Thermodynamic functions of dense plasmas: analytic approximations for astrophysical applications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.0690","snapshot_observed_at":"2026-08-12T14:37:34.962297Z","title":"Contributions to Plasma Physics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.962297Z"},"links":{"cited_paper":"/paper/1001.0690","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:253fcee3fa83568c5df193aa9359ea570d28fbd8ee7b6b507b2ddb6dc34d2c69","observation_id":"f5b19555-7a1b-4360-82f9-0a1d516efc79","resolution":{"observed_at":"2026-08-12T14:37:34.962297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.01852","last_updated":"2019-02-05T18:56:13Z","snapshot_observed_at":"2026-07-06T07:31:19.424498Z","submitted_at":"2019-02-05T18:56:13Z","title":"A new equation of state for dense hydrogen-helium mixtures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.01852","snapshot_observed_at":"2026-08-12T14:37:34.967056Z","title":", keywords =","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.967056Z"},"links":{"cited_paper":"/paper/1902.01852","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:0b0850fccd0b5173c23b5774e746fe11ff1f2fa4485c82f3bcf1fbe2e3136af4","observation_id":"d09f4300-c3f9-407e-81df-81d9ecc7b192","resolution":{"observed_at":"2026-08-12T14:37:34.967056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.00691","last_updated":"2021-04-01T18:00:01Z","snapshot_observed_at":"2026-08-10T18:54:05.403663Z","submitted_at":"2021-04-01T18:00:01Z","title":"Skye: A Differentiable Equation of State","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.00691","snapshot_observed_at":"2026-08-12T14:37:34.971887Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.971887Z"},"links":{"cited_paper":"/paper/2104.00691","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:7d37ba03c813381fa71c7da0054bee060b18b69ede2417d7be2ce3b1b34c0534","observation_id":"edccb19d-f29c-4361-b27b-a7032302307f","resolution":{"observed_at":"2026-08-12T14:37:34.971887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502045","last_updated":"2005-02-02T18:09:32Z","snapshot_observed_at":"2026-07-07T00:47:53.969693Z","submitted_at":"2005-02-02T18:09:32Z","title":"Low Temperature Opacities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0502045","snapshot_observed_at":"2026-08-12T14:37:34.976780Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.976780Z"},"links":{"cited_paper":"/paper/astro-ph/0502045","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:82cfeb884115e7557ce034decfd0a9645c43fe46c0f71eea6448e790bbb82bef","observation_id":"566b221f-ddb6-4cbf-87ae-b7186924cc78","resolution":{"observed_at":"2026-08-12T14:37:34.976780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.981844Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.981844Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:4ebab6cd3296dae33a9bfa428af81f5a2cb024a60cf390a734c3b26367d373ee","observation_id":"7247281c-6026-4028-8cb1-c1ee60da3c39","resolution":{"observed_at":"2026-08-12T14:37:34.981844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.986415Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.986415Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d5f9dc6618a790574291f5675e1b1693fbe12073721591682613a6cfe77111f7","observation_id":"a97bb179-9f51-4e0c-a474-02d88e3262c6","resolution":{"observed_at":"2026-08-12T14:37:34.986415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.990916Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.990916Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:51c4a74bb7c0668e7c60f3dc5bac5f6033bf17442e8982969046cceb32d61ec5","observation_id":"f65652ac-661a-4b81-9fc7-5eb291c12973","resolution":{"observed_at":"2026-08-12T14:37:34.990916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.10529","last_updated":"2021-08-24T05:39:31Z","snapshot_observed_at":"2026-07-06T11:40:56.544714Z","submitted_at":"2021-08-24T05:39:31Z","title":"The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.10529","snapshot_observed_at":"2026-08-12T14:37:34.995159Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.995159Z"},"links":{"cited_paper":"/paper/2108.10529","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:558c50711998021e7e41c9e0ff5565d9e2a421adc8b175feed5e29ed84ebccc2","observation_id":"6130c6f9-feb4-4e46-8453-805a5b370a50","resolution":{"observed_at":"2026-08-12T14:37:34.995159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:34.999585Z","title":"EAS Publications Series , year = 2009, editor =","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:34.999585Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:9a5701d9834d67905665746de6b9dd32aabeb8723ccee11d745ae25d313ed0f1","observation_id":"dc5a1f44-de1e-435e-84ab-17b2ab029f43","resolution":{"observed_at":"2026-08-12T14:37:34.999585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.04611","last_updated":"2015-04-17T19:27:59Z","snapshot_observed_at":"2026-07-06T04:15:19.038975Z","submitted_at":"2015-04-17T19:27:59Z","title":"The Araucaria Project: The First-Overtone Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-2532","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.04611","snapshot_observed_at":"2026-08-12T14:37:35.003639Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.003639Z"},"links":{"cited_paper":"/paper/1504.04611","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:e56c1ab9703dba8548b4a90fca427fb7a681f497feac6f07f017b958e4a6ce59","observation_id":"6655e22f-d4c7-4a15-a4ff-06687b48497a","resolution":{"observed_at":"2026-08-12T14:37:35.003639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.007854Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.007854Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:243feec37df82bf1aea0e0588a14f00939a6dc92fb8426893ca4632220e3ac99","observation_id":"943750f2-63ff-4c36-8e37-72d6fe0844fb","resolution":{"observed_at":"2026-08-12T14:37:35.007854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.0394","last_updated":"2011-01-02T09:36:12Z","snapshot_observed_at":"2026-07-06T02:21:29.140279Z","submitted_at":"2011-01-02T09:36:12Z","title":"A Classical Cepheid in a LMC eclipsing binary: evidence of shortcomings in current stellar evolutionary models?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.0394","snapshot_observed_at":"2026-08-12T14:37:35.011852Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.011852Z"},"links":{"cited_paper":"/paper/1101.0394","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:072005a11b27649d2518858968f633a7ceee6f370f38860d59f0f8d25ff3be3a","observation_id":"2da65194-863c-44d1-9c4d-76153b7bf63b","resolution":{"observed_at":"2026-08-12T14:37:35.011852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.10653","last_updated":"2019-08-01T13:54:45Z","snapshot_observed_at":"2026-08-04T09:23:38.346625Z","submitted_at":"2018-06-27T19:32:58Z","title":"A three-dimensional map of the Milky Way using classical Cepheid variable stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.10653","snapshot_observed_at":"2026-08-12T14:37:35.016191Z","title":"Science , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.016191Z"},"links":{"cited_paper":"/paper/1806.10653","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:3491f2c7e1b053790a156a330836e02afa0337a64187fe60a4012f71bc0dae53","observation_id":"e4de3f36-0062-4224-87c7-74f281a5c211","resolution":{"observed_at":"2026-08-12T14:37:35.016191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07603","last_updated":"2019-03-27T15:38:08Z","snapshot_observed_at":"2026-08-03T04:46:01.318400Z","submitted_at":"2019-03-18T17:50:59Z","title":"Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07603","snapshot_observed_at":"2026-08-12T14:37:35.020886Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.020886Z"},"links":{"cited_paper":"/paper/1903.07603","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:ce1262c4151e005b696195c1e913e00e58b3f7cf7a4a0895d9bdff3941c1be49","observation_id":"8cb336df-83fc-49f8-badc-7684b503d9e4","resolution":{"observed_at":"2026-08-12T14:37:35.020886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.025694Z","title":"Harvard College Observatory Circular , year = 1912, month = mar, volume =","venue":null,"work_id":null,"year":1912},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.025694Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:f94ec3eb26de8082b40da5ac181b38d6013dee7edb0c455490ee5fc1925e8e9b","observation_id":"092712c2-85e8-4204-b05f-b21f4550bde3","resolution":{"observed_at":"2026-08-12T14:37:35.025694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.030097Z","title":"Annals of Harvard College Observatory , year = 1907, month = jan, volume =","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.030097Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:9cf0b1a487d1c05aacd582da48901c9872fc97b2a3a21b56e14448181479e5e3","observation_id":"fc4bf47f-733d-4e00-af8a-91c6cbcda7bf","resolution":{"observed_at":"2026-08-12T14:37:35.030097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.3617","last_updated":"2014-03-14T15:46:31Z","snapshot_observed_at":"2026-08-07T15:09:31.848484Z","submitted_at":"2014-03-14T15:46:31Z","title":"The Araucaria Project. OGLE-LMC-CEP-1718: An exotic eclipsing binary system composed of two classical overtone Cepheids in a 413-day orbit","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.3617","snapshot_observed_at":"2026-08-12T14:37:35.034400Z","title":"OGLE-LMC-CEP-1718: An Exotic Eclipsing Binary System Composed of Two Classical Overtone Cepheids in a 413 Day Orbit","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.034400Z"},"links":{"cited_paper":"/paper/1403.3617","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:4a73762b940e53aa84e1b847ff9620f4a05234c015d7a88dac37b1f364f4ebfe","observation_id":"83070b95-7e8b-4518-9a87-8364cded0fa6","resolution":{"observed_at":"2026-08-12T14:37:35.034400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.6657","last_updated":"2011-10-30T21:24:17Z","snapshot_observed_at":"2026-07-06T02:36:39.374465Z","submitted_at":"2011-10-30T21:24:17Z","title":"Is there a mass discrepancy in the Cepheid binary OGLE-LMC-CEP0227?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.6657","snapshot_observed_at":"2026-08-12T14:37:35.039141Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.039141Z"},"links":{"cited_paper":"/paper/1110.6657","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:174134797f852417dffefd871b846e559b50874e5302c5e4c4838ae466873b4a","observation_id":"eb2528e9-de55-4a67-9f9d-8b60f3b837fe","resolution":{"observed_at":"2026-08-12T14:37:35.039141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.04518","last_updated":"2022-12-08T19:00:25Z","snapshot_observed_at":"2026-08-06T10:33:22.472359Z","submitted_at":"2022-12-08T19:00:25Z","title":"Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.04518","snapshot_observed_at":"2026-08-12T14:37:35.043779Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.043779Z"},"links":{"cited_paper":"/paper/2212.04518","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:000382a7fbe09d2f9d6ecc176022400ad45d7931c63af1c75be640bcea3d9a80","observation_id":"0e9f0ec3-37b6-4485-a866-b4d95d00d11d","resolution":{"observed_at":"2026-08-12T14:37:35.043779Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.09076","last_updated":"2025-02-24T09:42:26Z","snapshot_observed_at":"2026-08-10T20:08:29.685554Z","submitted_at":"2025-01-15T19:00:07Z","title":"A novel q-PED method: precise physical properties of a merger-origin binary Cepheid OGLE-LMC-CEP-1347","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.09076","snapshot_observed_at":"2026-08-12T14:37:35.048332Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.048332Z"},"links":{"cited_paper":"/paper/2501.09076","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:badba728bf81fa9c9254d2f1f2df7d7f431077078f8471cab7b946b24d3ef8c1","observation_id":"509b3c1f-777a-4baa-9168-1934209a9207","resolution":{"observed_at":"2026-08-12T14:37:35.048332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.02725","last_updated":"2015-08-11T20:11:17Z","snapshot_observed_at":"2026-07-06T04:26:27.164004Z","submitted_at":"2015-08-11T20:11:17Z","title":"The strange evolution of the Large Magellanic Cloud Cepheid OGLE-LMC-CEP1812","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.02725","snapshot_observed_at":"2026-08-12T14:37:35.053316Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.053316Z"},"links":{"cited_paper":"/paper/1508.02725","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:218f495b6cda613f1d8a636d63a7a5b4eba1772552c83f08a92c2e7c4e067db0","observation_id":"94973cf3-bfe5-4a6c-97b9-d517e7cdfc73","resolution":{"observed_at":"2026-08-12T14:37:35.053316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.5414","last_updated":"2011-09-25T23:21:18Z","snapshot_observed_at":"2026-07-06T02:34:36.789470Z","submitted_at":"2011-09-25T23:21:18Z","title":"The Araucaria Project. Accurate determination of the dynamical mass of the classical Cepheid in the eclipsing system OGLE-LMC-CEP-1812","version":1},"cited_work":{"arxiv_id":"1109.5414","doi":null,"metadata_source":"pith","pith_arxiv_id":"1109.5414","snapshot_observed_at":"2026-08-12T14:37:37.019111Z","title":"The Araucaria Project. Accurate determination of the dynamical mass of the classical Cepheid in the eclipsing system OGLE-LMC-CEP-1812","venue":"astro-ph.SR","work_id":"f6948249-d39f-4c99-af63-cb18a06127ea","year":2011},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.057980Z"},"links":{"cited_paper":"/paper/1109.5414","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:f9f56b6b7c7e360ca3b518c45fd555418daacf736297864fba1bed20248177ca","observation_id":"d9dca0c9-aa6e-42b6-8359-173c1dfed77f","resolution":{"observed_at":"2026-08-12T14:37:37.024278Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1308.5023","last_updated":"2013-08-23T00:50:35Z","snapshot_observed_at":"2026-07-06T03:21:14.653991Z","submitted_at":"2013-08-23T00:50:35Z","title":"Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227","version":1},"cited_work":{"arxiv_id":"1308.5023","doi":null,"metadata_source":"pith","pith_arxiv_id":"1308.5023","snapshot_observed_at":"2026-08-12T14:37:36.998085Z","title":"Physical parameters and the projection factor of the classical Cepheid in the binary system OGLE-LMC-CEP-0227","venue":"astro-ph.SR","work_id":"0ed941a9-3821-409a-a1c9-1dfc8df209c5","year":2013},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.062599Z"},"links":{"cited_paper":"/paper/1308.5023","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:185459b0edcc65264ed4c3fbef94753ba66bba192658ae04f6a0ef28324731c8","observation_id":"66a459dc-4f8e-4f91-b8fd-8eefa1b97d67","resolution":{"observed_at":"2026-08-12T14:37:37.003313Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01318","last_updated":"2016-01-19T22:25:40Z","snapshot_observed_at":"2026-08-12T14:52:55.917796Z","submitted_at":"2016-01-06T21:00:02Z","title":"The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01318","snapshot_observed_at":"2026-08-12T14:37:35.066976Z","title":"Classical Cepheids in the Magellanic System","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.066976Z"},"links":{"cited_paper":"/paper/1601.01318","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:457cb5ea010a669c09657ae2cc9ee38ab0c1d0355fdcb507638101fd8c1d1668","observation_id":"9c80ba6f-532a-42ff-968a-c8db8e92b34e","resolution":{"observed_at":"2026-08-12T14:37:35.066976Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.02020","last_updated":"2016-01-19T22:28:57Z","snapshot_observed_at":"2026-07-06T04:42:18.589186Z","submitted_at":"2016-01-08T21:00:03Z","title":"Multi-Mode and Non-Standard Classical Cepheids in the Magellanic System","version":2},"cited_work":{"arxiv_id":"1601.02020","doi":"10.48550/arxiv.1601.02020","metadata_source":"pith","pith_arxiv_id":"1601.02020","snapshot_observed_at":"2026-08-12T18:16:22.223912Z","title":"Multi-Mode and Non-Standard Classical Cepheids in the Magellanic System","venue":"astro-ph.SR","work_id":"43867df1-454b-4a69-890f-d745374b3a45","year":2016},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.071943Z"},"links":{"cited_paper":"/paper/1601.02020","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:5a2adde2ade809cfd34973efcde515da0903364eb3646dd519e0c38ce0f55d93","observation_id":"6b0a3e98-2306-4196-990c-2e61abf60042","resolution":{"observed_at":"2026-08-12T14:37:35.753975Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.05691","last_updated":"2016-04-19T18:58:39Z","snapshot_observed_at":"2026-08-11T20:17:39.856055Z","submitted_at":"2016-04-19T18:58:39Z","title":"On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.05691","snapshot_observed_at":"2026-08-12T14:37:35.076596Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.076596Z"},"links":{"cited_paper":"/paper/1604.05691","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:7a38a2369c669a00ae743ff156232b6bfc41e3210316a216b0b5dbfdff59a3d4","observation_id":"4edfb45d-338a-4be9-b21f-eb1491d10bff","resolution":{"observed_at":"2026-08-12T14:37:35.076596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.0809","last_updated":"2014-03-04T15:16:19Z","snapshot_observed_at":"2026-07-06T03:37:33.009560Z","submitted_at":"2014-03-04T15:16:19Z","title":"On the effect of rotation on populations of classical Cepheids I. Predictions at solar metallicity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.0809","snapshot_observed_at":"2026-08-12T14:37:35.081283Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.081283Z"},"links":{"cited_paper":"/paper/1403.0809","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:79d52b675bfaf7cdefe808601abe9dd0eeb0c1ac3956c00f9fff7de0f1f71623","observation_id":"5fa800a8-b3a9-49bb-a197-d76a62d43d4c","resolution":{"observed_at":"2026-08-12T14:37:35.081283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.1342","last_updated":"2008-01-09T01:06:59Z","snapshot_observed_at":"2026-07-06T01:37:47.227262Z","submitted_at":"2008-01-09T01:06:59Z","title":"Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy","version":1},"cited_work":{"arxiv_id":"0801.1342","doi":null,"metadata_source":"pith","pith_arxiv_id":"0801.1342","snapshot_observed_at":"2026-08-12T14:37:36.944924Z","title":"Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy","venue":"astro-ph","work_id":"0340a329-6b13-41bf-adc7-029fa4e9a306","year":2008},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.086027Z"},"links":{"cited_paper":"/paper/0801.1342","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:06b586252e0e1b95b33d499d61df27ced6b612acd4126fe9f9d51321baa2a82b","observation_id":"d8eed683-ebdf-47aa-a623-9c6463101050","resolution":{"observed_at":"2026-08-12T14:37:36.949661Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.090827Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.090827Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:6772c6777d614486f099d9c8f98be707d23664ec5e35c36537b2fe8e4d9f0e8d","observation_id":"77e2da00-d8e2-469e-a97a-756a80924d1e","resolution":{"observed_at":"2026-08-12T14:37:35.090827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.095077Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.095077Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:042b266995236a8902b8496941d29129c20fe7a4d888ebfcba547072f3c2394e","observation_id":"e4aaebf1-b30d-45ed-a1cc-3dec251865f8","resolution":{"observed_at":"2026-08-12T14:37:35.095077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.099548Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.099548Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:123f3e4cc3d700bb63a25db680ed1b4c8fed9b3f3be7abcab7abc0545733cc6b","observation_id":"67463b42-22d1-4f61-b5c1-390308691fed","resolution":{"observed_at":"2026-08-12T14:37:35.099548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.103637Z","title":", year = 1968, month = mar, volume =","venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.103637Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:6b91da42a2d38453c3a412df1c3b79ec888e598005d50b863e8d6dd70169058a","observation_id":"646347c6-246a-433c-b085-e5f7018f4cd3","resolution":{"observed_at":"2026-08-12T14:37:35.103637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.2855","last_updated":"2012-02-13T21:00:03Z","snapshot_observed_at":"2026-07-06T02:42:48.975962Z","submitted_at":"2012-02-13T21:00:03Z","title":"On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud","version":1},"cited_work":{"arxiv_id":"1202.2855","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.2855","snapshot_observed_at":"2026-08-12T14:37:36.850448Z","title":"On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud","venue":"astro-ph.SR","work_id":"7ce9c457-8c6b-40a4-9b23-8c6f03c38064","year":2012},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.107929Z"},"links":{"cited_paper":"/paper/1202.2855","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:fec3a403eff713b6f59c02cd904dbd0f5a604122e5a0e553ea14632b460ccf1c","observation_id":"b8f3b82b-77c2-45da-8d08-d0f81ce8b870","resolution":{"observed_at":"2026-08-12T14:37:36.855070Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1012.0231","last_updated":"2010-12-01T15:51:14Z","snapshot_observed_at":"2026-07-06T02:20:02.160540Z","submitted_at":"2010-12-01T15:51:14Z","title":"Accurate dynamical mass determination of a classical Cepheid in an eclipsing binary system","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1012.0231","snapshot_observed_at":"2026-08-12T14:37:35.113015Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.113015Z"},"links":{"cited_paper":"/paper/1012.0231","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:fb30a191e2a9ca3abc3a2477e1ec21f4fbb80fb6f1f89ddcf02973cc061d067a","observation_id":"e8fc5723-b49f-4d1c-a980-b6fc9b3526ec","resolution":{"observed_at":"2026-08-12T14:37:35.113015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.3087","last_updated":"2009-08-21T10:10:58Z","snapshot_observed_at":"2026-07-06T01:59:46.137460Z","submitted_at":"2009-08-21T10:10:58Z","title":"Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants","version":1},"cited_work":{"arxiv_id":"0908.3087","doi":null,"metadata_source":"pith","pith_arxiv_id":"0908.3087","snapshot_observed_at":"2026-08-12T14:37:36.816705Z","title":"Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants","venue":"astro-ph.SR","work_id":"fc79c2ec-47ef-4c2c-bcea-694ccac2c27c","year":2009},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.117636Z"},"links":{"cited_paper":"/paper/0908.3087","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:4c3f4a69cbdc608d61a85fda8de878bd7d8ebdf4ed79a7572c8b98790dac7059","observation_id":"ce4bef51-53e1-40a6-bb35-a785742d6660","resolution":{"observed_at":"2026-08-12T14:37:36.821378Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.08330","last_updated":"2024-10-10T19:40:14Z","snapshot_observed_at":"2026-08-12T22:25:57.922971Z","submitted_at":"2024-10-10T19:40:14Z","title":"Connecting integrated RGB mass loss from asteroseismology and globular clusters","version":1},"cited_work":{"arxiv_id":"2410.08330","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.08330","snapshot_observed_at":"2026-08-12T14:37:36.796156Z","title":"Connecting integrated RGB mass loss from asteroseismology and globular clusters","venue":"astro-ph.SR","work_id":"cb2599b7-24eb-493b-a35d-292dff652a20","year":2024},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.122438Z"},"links":{"cited_paper":"/paper/2410.08330","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:356336be7cdd24f2137e18f5b00b0ba0d1510f450348438c8fbf50aaf74c3e12","observation_id":"99587992-8ad3-43cd-953a-aa35b3d3ae95","resolution":{"observed_at":"2026-08-12T14:37:36.801531Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.18714","last_updated":"2025-03-15T00:46:29Z","snapshot_observed_at":"2026-08-07T17:48:39.710798Z","submitted_at":"2025-02-26T00:19:02Z","title":"Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses","version":2},"cited_work":{"arxiv_id":"2502.18714","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.18714","snapshot_observed_at":"2026-08-12T14:37:36.774555Z","title":"Asteroseismic Study of Subgiants and Giants of the Open Cluster M67 using Kepler/K2: Expanded Sample and Precise Masses","venue":"astro-ph.SR","work_id":"b35c25ee-37f8-42a6-be26-8fe99782b24a","year":2025},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.128043Z"},"links":{"cited_paper":"/paper/2502.18714","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:a8406434857c8709ed44d9bbcc043961b771c57f165c5d8c2a433ea64cddb67b","observation_id":"5bfeb0b8-8935-40e8-9a94-bb7bcb6b8301","resolution":{"observed_at":"2026-08-12T14:37:36.780333Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03753","last_updated":"2017-11-10T10:12:29Z","snapshot_observed_at":"2026-07-06T06:08:45.897135Z","submitted_at":"2017-11-10T10:12:29Z","title":"Theoretical investigation on the mass loss impact on asteroseismic grid-based estimates of mass, radius, and age for RGB stars","version":1},"cited_work":{"arxiv_id":"1711.03753","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.03753","snapshot_observed_at":"2026-08-12T14:37:36.754348Z","title":"Theoretical investigation on the mass loss impact on asteroseismic grid-based estimates of mass, radius, and age for RGB stars","venue":"astro-ph.SR","work_id":"37414e02-ceb2-4a43-addf-3b026a32cbe4","year":2017},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.132847Z"},"links":{"cited_paper":"/paper/1711.03753","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:31940448c0e6a576cd60a94c8f6f603ea8ac654aabf96a46ea8b619d72afca58","observation_id":"757d5341-6e4c-4a70-beb8-b76073a95a18","resolution":{"observed_at":"2026-08-12T14:37:36.759106Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.137548Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.137548Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:64beda71a05964acbdce5ce089baeca782e5e03992c32bccb4103ebc50ba599b","observation_id":"c3fef32c-35fa-4ba7-96fa-8418432c6138","resolution":{"observed_at":"2026-08-12T14:37:35.137548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.142043Z","title":"Memoires of the Societe Royale des Sciences de Liege , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.142043Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:e1c2be604f7c721c8540dccb58f7af8f968b44401578c1352cc1c47bda0bb1a3","observation_id":"a3e9d900-29e4-4352-8fb6-6fb81e98cdd5","resolution":{"observed_at":"2026-08-12T14:37:35.142043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0007139","last_updated":"2000-07-11T14:36:12Z","snapshot_observed_at":"2026-08-06T07:52:01.567564Z","submitted_at":"2000-07-11T14:36:12Z","title":"The evolution of AGB stars with convective overshoot","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0007139","snapshot_observed_at":"2026-08-12T14:37:35.146531Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.146531Z"},"links":{"cited_paper":"/paper/astro-ph/0007139","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:868d6f257cde29dbf9344094d1f11faac0b312842986d5f8c465396a103a2a7d","observation_id":"613ed5f9-41c2-41e9-88b6-51164e484018","resolution":{"observed_at":"2026-08-12T14:37:35.146531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405087","last_updated":"2004-05-05T15:30:48Z","snapshot_observed_at":"2026-07-07T00:42:19.442022Z","submitted_at":"2004-05-05T15:30:48Z","title":"New Grids of ATLAS9 Model Atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405087","snapshot_observed_at":"2026-08-12T14:37:35.151320Z","title":"Modelling of Stellar Atmospheres , year = 2003, editor =","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.151320Z"},"links":{"cited_paper":"/paper/astro-ph/0405087","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:be891fdd7b39b5c4e6752de4a1327d3dad6f24140f553e27a3daa71564017334","observation_id":"37a707d7-acd7-4288-8063-72b39e1ae53e","resolution":{"observed_at":"2026-08-12T14:37:35.151320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-12T14:37:35.155970Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.155970Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:0eba6a42879f6c9db40c85746392024a75c3d50cb1f49f9c2826aafc38fe0d99","observation_id":"2df42163-618b-43b9-96f2-723a92059b07","resolution":{"observed_at":"2026-08-12T14:37:35.155970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.03651","last_updated":"2022-12-30T22:06:41Z","snapshot_observed_at":"2026-08-04T01:17:19.112305Z","submitted_at":"2022-08-07T06:17:23Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.03651","snapshot_observed_at":"2026-08-12T14:37:35.160675Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.160675Z"},"links":{"cited_paper":"/paper/2208.03651","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:1d92fd3900fd82f6f837637e98d245ddc05f2e826a679e936856416d0cf308f1","observation_id":"88f82d53-56be-48e8-a5aa-51f14e4f266a","resolution":{"observed_at":"2026-08-12T14:37:35.160675Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.01426","last_updated":"2019-05-16T08:59:53Z","snapshot_observed_at":"2026-08-09T21:08:34.617339Z","submitted_at":"2019-03-04T18:38:11Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.01426","snapshot_observed_at":"2026-08-12T14:37:35.165434Z","title":", keywords =","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.165434Z"},"links":{"cited_paper":"/paper/1903.01426","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:6d968bc89ea15c223a955eaf206c6f526764eef5d10770761386e8224d4399ea","observation_id":"57c5be9c-bf41-4996-9bce-aa31bde45f24","resolution":{"observed_at":"2026-08-12T14:37:35.165434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.08424","last_updated":"2018-01-04T00:21:17Z","snapshot_observed_at":"2026-07-06T06:05:34.407208Z","submitted_at":"2017-10-23T18:00:02Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.08424","snapshot_observed_at":"2026-08-12T14:37:35.171133Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.171133Z"},"links":{"cited_paper":"/paper/1710.08424","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:893cdde3052a89f6a1725e27a8e8a8fba9686d8c4f7db804ae2392d75963f07b","observation_id":"a3c1d7b2-b2de-4d72-b225-1ea1f2adbfd3","resolution":{"observed_at":"2026-08-12T14:37:35.171133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.175797Z","title":", year = 2016, month = mar, volume =","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.175797Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:b0002fc460a77b58c45a1bafde1ca017ea7a610e15d28db8adb41465e08e3b83","observation_id":"1cac9454-03f6-4941-9a04-81aa791765e0","resolution":{"observed_at":"2026-08-12T14:37:35.175797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.03146","last_updated":"2017-01-08T05:04:31Z","snapshot_observed_at":"2026-08-09T12:28:11.007796Z","submitted_at":"2015-06-10T02:23:18Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.03146","snapshot_observed_at":"2026-08-12T14:37:35.180862Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.180862Z"},"links":{"cited_paper":"/paper/1506.03146","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:fd0bdd9e5d7fa416ed183d4cb6f912696945e891fb5ec84051f2900b06083e86","observation_id":"684bed69-d383-4ea0-886f-3fd54576186f","resolution":{"observed_at":"2026-08-12T14:37:35.180862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.0319","last_updated":"2013-06-12T19:42:55Z","snapshot_observed_at":"2026-08-12T19:03:26.795307Z","submitted_at":"2013-01-02T21:00:00Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.0319","snapshot_observed_at":"2026-08-12T14:37:35.185749Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.185749Z"},"links":{"cited_paper":"/paper/1301.0319","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:fce20a5c689c3e3246dcf3db712394ceceee84ad49efabbc662688b5bd28b7ab","observation_id":"d0128cb6-aed4-4308-8057-9f25fb696713","resolution":{"observed_at":"2026-08-12T14:37:35.185749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1009.1622","last_updated":"2010-09-08T20:00:05Z","snapshot_observed_at":"2026-08-12T19:03:26.192943Z","submitted_at":"2010-09-08T20:00:05Z","title":"Modules for Experiments in Stellar Astrophysics (MESA)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.1622","snapshot_observed_at":"2026-08-12T14:37:35.190062Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.190062Z"},"links":{"cited_paper":"/paper/1009.1622","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:f37f6fa923d88f4cc3281360305325d2d48b1bca6429f5e6735af75f714ee1b6","observation_id":"4929153d-7f1b-479b-8eac-6ab4705fa6ae","resolution":{"observed_at":"2026-08-12T14:37:35.190062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07136","last_updated":"2024-08-13T18:10:57Z","snapshot_observed_at":"2026-08-12T23:04:06.089020Z","submitted_at":"2024-08-13T18:10:57Z","title":"Toward a Comprehensive Grid of Cepheid Models with MESA I. Uncertainties of the Evolutionary Tracks of Intermediate-Mass Stars","version":1},"cited_work":{"arxiv_id":"2408.07136","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.07136","snapshot_observed_at":"2026-08-12T14:37:36.630833Z","title":"Toward a Comprehensive Grid of Cepheid Models with MESA I. Uncertainties of the Evolutionary Tracks of Intermediate-Mass Stars","venue":"astro-ph.SR","work_id":"b2ce2311-15d6-4d22-91d0-2d8e487f7cb1","year":2024},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.194418Z"},"links":{"cited_paper":"/paper/2408.07136","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d7d9ed1e9587b852fa9663be1d98ece580c85beaa31229402673aebd96a8727e","observation_id":"038b2d84-0c21-40e6-a583-8e99eb970b08","resolution":{"observed_at":"2026-08-12T14:37:36.635485Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.198578Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.198578Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:c72398e3efb7970e7de2cef6724c5303e15d1732bbf9b8d52b887b336a18656f","observation_id":"445f2d2e-9b95-4fa9-a03e-713c713b542f","resolution":{"observed_at":"2026-08-12T14:37:35.198578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0808.2210","last_updated":"2008-10-06T13:55:45Z","snapshot_observed_at":"2026-07-06T01:43:41.463165Z","submitted_at":"2008-08-15T22:17:01Z","title":"The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. I. Classical Cepheids in the Large Magellanic Cloud","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.2210","snapshot_observed_at":"2026-08-12T14:37:35.202981Z","title":"The OGLE-III Catalog of Variable Stars","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.202981Z"},"links":{"cited_paper":"/paper/0808.2210","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:075fbbef547bb0245bc7f6a1a421e84878501cb5e5371ea93f61075de9a35636","observation_id":"b0f910e6-939f-4d6e-8e6e-24672410cb40","resolution":{"observed_at":"2026-08-12T14:37:35.202981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03104","last_updated":"2021-11-04T18:51:48Z","snapshot_observed_at":"2026-08-06T19:53:50.570637Z","submitted_at":"2021-11-04T18:51:48Z","title":"Non-radial modes in classical Cepheids. What to look for in spectroscopy?","version":1},"cited_work":{"arxiv_id":"2111.03104","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.03104","snapshot_observed_at":"2026-08-12T14:37:36.529395Z","title":"Non-radial modes in classical Cepheids. What to look for in spectroscopy?","venue":"astro-ph.SR","work_id":"14578f4c-6e70-4ead-b23f-447cc3b77a6f","year":2021},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.207634Z"},"links":{"cited_paper":"/paper/2111.03104","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:23b7268975960ade5cc46574c97f373fd5e8ea08d75400c1bf739b9927a8974f","observation_id":"7bc2a729-6ba2-4025-ba82-73b81b9ae4cd","resolution":{"observed_at":"2026-08-12T14:37:36.533759Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00447","last_updated":"2019-12-19T20:13:12Z","snapshot_observed_at":"2026-07-06T08:11:48.623117Z","submitted_at":"2019-08-01T15:01:51Z","title":"Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Str\\\"omgren photometry","version":2},"cited_work":{"arxiv_id":"1908.00447","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.00447","snapshot_observed_at":"2026-08-12T14:37:36.508551Z","title":"Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Str\\\"omgren photometry","venue":"astro-ph.SR","work_id":"570a3dd6-cbcf-43c2-adc9-70d055fab6f7","year":2019},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.212313Z"},"links":{"cited_paper":"/paper/1908.00447","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:bd5518c794275e2e0325f109414fc92b9b1a8bf1d413a1ab5590f41bb0d4bde5","observation_id":"b7c3a8af-5b71-4047-82c7-30b036b94669","resolution":{"observed_at":"2026-08-12T14:37:36.513599Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T14:37:35.216774Z","title":"Stellar Populations and the Distance Scale , year = 2018, editor =","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.216774Z"},"links":{"citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d1b6c69353337c41fe9dce2237d5ac0b7d8eeed7fe87709c8860aacf460c40b8","observation_id":"408ec0d3-b229-4cd6-9990-50063a4535f2","resolution":{"observed_at":"2026-08-12T14:37:35.216774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01683","last_updated":"2016-01-07T21:00:01Z","snapshot_observed_at":"2026-07-06T04:42:11.317805Z","submitted_at":"2016-01-07T21:00:01Z","title":"Eclipsing Binaries with Classical Cepheid Component in the Magellanic System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01683","snapshot_observed_at":"2026-08-12T14:37:35.221244Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.221244Z"},"links":{"cited_paper":"/paper/1601.01683","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:a161be1c3fbd38bf72570cfde1de7da9e60a8ce283507013e8b4ba967814ba97","observation_id":"0a682472-bb11-41d7-b684-18bcff1d68ff","resolution":{"observed_at":"2026-08-12T14:37:35.221244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.09851","last_updated":"2017-09-23T06:52:50Z","snapshot_observed_at":"2026-08-04T06:26:17.470134Z","submitted_at":"2017-08-31T17:59:12Z","title":"Observational calibration of the projection factor of Cepheids IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.09851","snapshot_observed_at":"2026-08-12T14:37:35.225864Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.225864Z"},"links":{"cited_paper":"/paper/1708.09851","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d51ed72530b817cab3d669ad15303f9a14cf2d3a6e37e9edebcf1bb286e67dfa","observation_id":"0c146459-a989-44b7-93db-88d317930e1e","resolution":{"observed_at":"2026-08-12T14:37:35.225864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.04814","last_updated":"2016-04-17T00:36:55Z","snapshot_observed_at":"2026-07-06T04:53:06.316815Z","submitted_at":"2016-04-17T00:36:55Z","title":"The influential effect of blending, bump, changing period and eclipsing Cepheids on the Leavitt law","version":1},"cited_work":{"arxiv_id":"1604.04814","doi":null,"metadata_source":"pith","pith_arxiv_id":"1604.04814","snapshot_observed_at":"2026-08-12T14:37:36.473275Z","title":"The influential effect of blending, bump, changing period and eclipsing Cepheids on the Leavitt law","venue":"astro-ph.SR","work_id":"11577b75-78be-4da9-a8c6-1a87cae3ec71","year":2016},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.230463Z"},"links":{"cited_paper":"/paper/1604.04814","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:196de7ce0728f6700b46a8fe304c9ee61cb12961869ce2e848503f68e65c73ed","observation_id":"6010608d-5c50-4f11-829b-b8245ca32179","resolution":{"observed_at":"2026-08-12T14:37:36.477853Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1210.1219","last_updated":"2012-11-09T15:13:01Z","snapshot_observed_at":"2026-08-10T09:41:32.118608Z","submitted_at":"2012-10-03T20:00:03Z","title":"The Optical Gravitational Lensing Experiment. Gaia South Ecliptic Pole Field as Seen by OGLE-IV","version":2},"cited_work":{"arxiv_id":"1210.1219","doi":"10.48550/arxiv.1210.1219","metadata_source":"pith","pith_arxiv_id":"1210.1219","snapshot_observed_at":"2026-08-12T18:16:22.223912Z","title":"The Optical Gravitational Lensing Experiment. Gaia South Ecliptic Pole Field as Seen by OGLE-IV","venue":"astro-ph.SR","work_id":"aec6dca5-c461-4af9-8a1f-03a49ef6f3a8","year":2012},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.234953Z"},"links":{"cited_paper":"/paper/1210.1219","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:34efaee0167f0e2c397a909ea828235d8c96c3cee1d33a6de62f0a3737f8af76","observation_id":"e682bfa1-9298-4fff-9c76-f0f29f59474d","resolution":{"observed_at":"2026-08-12T14:37:35.642534Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.02826","last_updated":"2015-11-09T20:15:59Z","snapshot_observed_at":"2026-08-01T15:42:04.364972Z","submitted_at":"2015-11-09T20:15:59Z","title":"The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic Cloud","version":1},"cited_work":{"arxiv_id":"1511.02826","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.02826","snapshot_observed_at":"2026-08-12T14:37:36.453411Z","title":"The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic Cloud","venue":"astro-ph.SR","work_id":"317c7165-f27d-4f71-ac19-308ae93c3ab8","year":2015},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.240180Z"},"links":{"cited_paper":"/paper/1511.02826","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:eef4e115bc41798b7c438e91366e19386c6ac0140a70a7fa96cc0ad8b1899998","observation_id":"ef6bd687-7f29-4f32-b0f4-d047d527af04","resolution":{"observed_at":"2026-08-12T14:37:36.458410Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03503","last_updated":"2021-11-05T13:47:01Z","snapshot_observed_at":"2026-07-30T16:16:35.348756Z","submitted_at":"2021-11-05T13:47:01Z","title":"Period Change Rates in Large Magellanic Cloud Cepheids Revisited","version":1},"cited_work":{"arxiv_id":"2111.03503","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.03503","snapshot_observed_at":"2026-08-12T14:37:36.433262Z","title":"Period Change Rates in Large Magellanic Cloud Cepheids Revisited","venue":"astro-ph.SR","work_id":"dabd834f-cc9d-4161-ac9c-d89effa8c582","year":2021},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.244870Z"},"links":{"cited_paper":"/paper/2111.03503","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:0a80073cf24052732585c51cc97be9aa0a3ff4a8029935d17881dd049f1b6498","observation_id":"4086704e-f013-4bb5-a1d8-06ddadeb39ef","resolution":{"observed_at":"2026-08-12T14:37:36.438240Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.00661","last_updated":"2025-03-01T23:25:30Z","snapshot_observed_at":"2026-08-07T17:36:43.854626Z","submitted_at":"2025-03-01T23:25:30Z","title":"Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes","version":1},"cited_work":{"arxiv_id":"2503.00661","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.00661","snapshot_observed_at":"2026-08-12T14:37:36.411707Z","title":"Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes","venue":"astro-ph.SR","work_id":"4617d882-5005-4eb5-8041-cce4cd3ea768","year":2025},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.249589Z"},"links":{"cited_paper":"/paper/2503.00661","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:d6948017575c9e2e2438d270d756e7531713d78f0dd789d0b38665c14f5e7b5c","observation_id":"d58bbe07-d918-488e-be4d-b33b8a23ed7b","resolution":{"observed_at":"2026-08-12T14:37:36.417036Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.14039","last_updated":"2024-03-27T14:38:36Z","snapshot_observed_at":"2026-08-04T18:41:04.138341Z","submitted_at":"2024-03-20T23:28:11Z","title":"Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect","version":2},"cited_work":{"arxiv_id":"2403.14039","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.14039","snapshot_observed_at":"2026-08-12T14:37:36.390580Z","title":"Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect","venue":"astro-ph.SR","work_id":"e20eecd0-6296-438e-a423-fd7247678984","year":2024},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.254248Z"},"links":{"cited_paper":"/paper/2403.14039","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:9b75535b89b1f173ab7030c040fc4b08e647f47b2a50fbeab4b9dacaf46aadfd","observation_id":"5030e462-9765-4263-a244-5940e0610e1f","resolution":{"observed_at":"2026-08-12T14:37:36.395478Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.08860","last_updated":"2021-11-22T15:44:01Z","snapshot_observed_at":"2026-07-06T11:58:46.444354Z","submitted_at":"2021-10-17T16:10:24Z","title":"The iron and oxygen content of LMC Classical Cepheids and its implications for the Extragalactic Distance Scale and Hubble constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.08860","snapshot_observed_at":"2026-08-12T14:37:35.259005Z","title":"Equivalent width analysis with Kurucz stellar atmosphere models","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.259005Z"},"links":{"cited_paper":"/paper/2110.08860","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:bc97161ddf91c21db0f041edbb5d9e4158afa87e6a264862365cbe389f20eab7","observation_id":"348c7c9c-f957-476a-ac9b-924b28e423f0","resolution":{"observed_at":"2026-08-12T14:37:35.259005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.00229","last_updated":"2023-02-10T10:45:27Z","snapshot_observed_at":"2026-07-06T14:36:25.690733Z","submitted_at":"2022-12-31T15:47:43Z","title":"Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves","version":2},"cited_work":{"arxiv_id":"2301.00229","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.00229","snapshot_observed_at":"2026-08-12T14:37:36.353262Z","title":"Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves","venue":"astro-ph.SR","work_id":"7850ed9e-db37-4ce7-a1f0-fd7f92e8291f","year":2022},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.263820Z"},"links":{"cited_paper":"/paper/2301.00229","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:cd1030ffdc84f7250c44d988502ff0c185368547480b74a65ec84ebb49c3abc4","observation_id":"a6756497-e59a-474f-a2b9-b1cf63ca1f48","resolution":{"observed_at":"2026-08-12T14:37:36.358010Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.04759","last_updated":"2025-06-05T08:43:58Z","snapshot_observed_at":"2026-08-07T10:31:11.547079Z","submitted_at":"2025-06-05T08:43:58Z","title":"Implications of a turbulent convection model for classical Cepheids","version":1},"cited_work":{"arxiv_id":"2506.04759","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.04759","snapshot_observed_at":"2026-08-12T14:37:36.332046Z","title":"Implications of a turbulent convection model for classical Cepheids","venue":"astro-ph.SR","work_id":"14c71068-538a-4a1f-861f-f79e20d3a2c7","year":2025},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.269469Z"},"links":{"cited_paper":"/paper/2506.04759","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:244bb01b805b51544c9c7fc2eb7ac460c4a49d25641491177c417265ef9bd99d","observation_id":"c030acd2-cbe5-4b9c-a5fb-1ef4836b51d4","resolution":{"observed_at":"2026-08-12T14:37:36.337006Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.01391","last_updated":"2018-07-21T15:19:47Z","snapshot_observed_at":"2026-08-09T10:04:43.031650Z","submitted_at":"2018-06-04T21:09:31Z","title":"The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.01391","snapshot_observed_at":"2026-08-12T14:37:35.274600Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-12T14:37:35.274600Z"},"links":{"cited_paper":"/paper/1806.01391","citing_paper":"/paper/2608.10909"},"observation_digest":"sha256:21c4be2d3aaca2a91c5f705cf3abf67a3308b746521522e316de44ab3436c09a","observation_id":"c03b01de-1f99-4259-8e2c-3a91ad970cb7","resolution":{"observed_at":"2026-08-12T14:37:35.274600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2608.10909","last_updated":"2026-08-11T13:30:29Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-12T23:27:11.786397Z","submitted_at":"2026-08-11T13:30:29Z","title":"Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":78,"verified_exact":22,"verified_fuzzy":0},"total_outbound_references":125},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 100 of 125 outbound references and 0 inbound Pith citation observations for arXiv:2608.10909."}