{"as_of":"2026-08-07T18:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f2e39bb26a9907cc5da4c5129cfea5e734a53100a581396ddc7313491b231387","coverage":[{"denominator":98,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":98,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T19:40:06.008799Z","state":"measured"},{"denominator":99,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":99,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T16:18:19.429640Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-06T16:18:32.417568Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"cited_work":{"arxiv_id":"2507.05202","doi":null,"metadata_source":"pith","pith_arxiv_id":"2507.05202","snapshot_observed_at":"2026-08-06T16:18:32.417568Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","venue":"astro-ph.EP","work_id":"af15d4a2-dbe5-4aee-be48-96e8e31cd9cc","year":2025},"citing_paper":{"arxiv_id":"2507.13991","last_updated":"2025-07-24T13:56:45Z","snapshot_observed_at":"2026-08-06T16:09:29.789863Z","submitted_at":"2025-07-18T14:58:03Z","title":"Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-06T16:18:19.429640Z"},"links":{"cited_paper":"/paper/2507.05202","citing_paper":"/paper/2507.13991"},"observation_digest":"sha256:05eee7fbf676e0c7ee42e0e753976079840e8fd4fd2defe0bf81046e1712df53","observation_id":"64719da7-6228-4511-b025-ec44a158f4c9","resolution":{"observed_at":"2026-08-06T16:18:32.476918Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.05202/citation-record","integrity":"/paper/2507.05202/integrity","json":"/paper/2507.05202/citation-record.json","paper":"/paper/2507.05202"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:39:58.238688Z","title":"2006, ApJ, 650, 394, doi: 10.1086/506011","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.238688Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:e80a666aef872c60de6c40d4e1ab424bc681834a0141d3fbe16775c9e1d2cbbd","observation_id":"b86a0176-3a4e-4f33-be4a-38f64680d6e8","resolution":{"observed_at":"2026-08-06T19:39:58.238688Z","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":"2026-08-06T19:39:58.335653Z","title":"S., Dulk, G","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.335653Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2dce9599e03386686a26e9fbb7be91e3bcf9080413dad6cb54c2dcf409bdde98","observation_id":"510e53b8-021a-47b9-a3e0-4883d3b959ed","resolution":{"observed_at":"2026-08-06T19:39:58.335653Z","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":"2026-08-06T19:39:58.441147Z","title":"2018, AJ, 155, 178, doi: 10.3847/1538-3881/aab54e","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.441147Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:8a91df78e7b4f3657920cfc88a03ec0315d89db3d7b15b7bb62b1c2be0f38794","observation_id":"ecc64fa2-db9f-4d74-8a95-24504ec6ebfb","resolution":{"observed_at":"2026-08-06T19:39:58.441147Z","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":"2026-08-06T19:39:58.554083Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.554083Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2f419ff6baec37499399f595097e8568ec935bf37d7ed96310305ceac0561e44","observation_id":"c181aa83-1972-4e6e-a4f3-4031eac90f04","resolution":{"observed_at":"2026-08-06T19:39:58.554083Z","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":"2026-08-06T19:39:58.688372Z","title":"J., & Bodenheimer, P","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.688372Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:7aeef31b29c150a1f30d13b14e11eb398eaff32d7f367e4f39c106683795feb5","observation_id":"c2289392-55e5-47d0-b2a4-5ba3abe50ffd","resolution":{"observed_at":"2026-08-06T19:39:58.688372Z","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":"2026-08-06T19:39:58.853266Z","title":"2024, Physics of Plasmas, 31, 110501, doi: 10.1063/5.0219405","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.853266Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:bf11560e0cc3878785d42f08ac1ece0210d640a50824a101c661b687df78e941","observation_id":"970a6083-dada-440f-9db6-5ddaed51f3a8","resolution":{"observed_at":"2026-08-06T19:39:58.853266Z","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":"2026-08-06T19:39:58.970358Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:58.970358Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:023579714868629f86069c84dd18d3e373ec69079303eeb4574d88522441027d","observation_id":"63c9d3b4-d6da-4d2d-a102-ed3d85635b57","resolution":{"observed_at":"2026-08-06T19:39:58.970358Z","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":"2026-08-06T19:39:59.123056Z","title":"R., Shimwell, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.123056Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:e7f5a64a61ca5543f975baccd34a79c3ac2145d4ec2b84a81b1351515c54dc8a","observation_id":"e62d4beb-8791-46e1-9d30-35330b280255","resolution":{"observed_at":"2026-08-06T19:39:59.123056Z","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":"2026-08-06T19:39:59.279875Z","title":"W., & Ostlie, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.279875Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:1cb5151b35d73224b74d8fa65ee6d652a1d9aa07591ef489bcf01971b6c5b218","observation_id":"d1aa10cc-0e0b-43b3-bd56-ceda68ce3146","resolution":{"observed_at":"2026-08-06T19:39:59.279875Z","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":"2026-08-06T19:39:59.356272Z","title":"W., Shkolnik, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.356272Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:cf560bf126d0f61632d85615ef89402c22e43a65990769accb8ef9e360fa5b00","observation_id":"01cee139-1f24-4bf6-a686-044c92baa73c","resolution":{"observed_at":"2026-08-06T19:39:59.356272Z","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":"2026-08-06T19:39:59.466346Z","title":"2007, ApJL, 661, L81, doi: 10.1086/518473","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.466346Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:8fe164ef1fdf665ca13596bfea86fdb3666b6145a2aa05c36a13d5466955369b","observation_id":"e6745973-b50f-4fa3-bedd-6af26ca6088c","resolution":{"observed_at":"2026-08-06T19:39:59.466346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.03009","last_updated":"2020-06-04T16:56:47Z","snapshot_observed_at":"2026-08-06T04:58:50.423444Z","submitted_at":"2020-06-04T16:56:47Z","title":"List-three-coloring $ P_t $-free graphs with no induced 1-subdivision of $ K_{1,s} $","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.03009","snapshot_observed_at":"2026-08-06T19:39:59.528663Z","title":"R., & Aubert, J","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.528663Z"},"links":{"cited_paper":"/paper/2006.03009","citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:d8fc117dcbe0fd3d5b43a8070345281589edaa7148b8d361d29ddf533a6667ea","observation_id":"d0f53e5e-9d44-4ab5-892d-26d4512789e0","resolution":{"observed_at":"2026-08-06T19:39:59.528663Z","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":"2026-08-06T19:39:59.606477Z","title":"R., Holzwarth, V., & Reiners, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.606477Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:35d7d3d97abcaeea4ed80b5595db6323e9e1f06f5cbdbdd5c8d8cd97ac22bc3b","observation_id":"ee2f2d7c-55fd-426e-8d8e-e71a56587c55","resolution":{"observed_at":"2026-08-06T19:39:59.606477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.03299","last_updated":"2025-06-03T18:36:52Z","snapshot_observed_at":"2026-08-07T11:04:15.900189Z","submitted_at":"2025-06-03T18:36:52Z","title":"The NASA Exoplanet Archive and Exoplanet Follow-up Observing Program: Data, Tools, and Usage","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.03299","snapshot_observed_at":"2026-08-06T19:39:59.657391Z","title":"L., McElroy, D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.657391Z"},"links":{"cited_paper":"/paper/2506.03299","citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:3ec6546c3f2d620aace52a040af5b10f564a3fca47456453b0efcc12328d10ec","observation_id":"f0ec6290-48cf-47cb-a9c0-e5470c67b3a3","resolution":{"observed_at":"2026-08-06T19:39:59.657391Z","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":"2026-08-06T19:39:59.719260Z","title":"P., & Giuli, R","venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.719260Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:d980cee94bfcfa62470e843096e55bfe98761bd01f78ae24ae7150c2c714891f","observation_id":"0351ab39-10bd-4ae9-8107-7bff21750c7d","resolution":{"observed_at":"2026-08-06T19:39:59.719260Z","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":"2026-08-06T19:39:59.806443Z","title":"H., & Musielak, Z","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.806443Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:1bf6c118ddc9a54a9eb8a03a7cbb2740e23e0abba045e83b81a62cee302c86e8","observation_id":"db344744-1051-4c1b-ac28-c46c384bafb8","resolution":{"observed_at":"2026-08-06T19:39:59.806443Z","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":"2026-08-06T19:39:59.872361Z","title":"B., Schwartz, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T19:39:59.872361Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2e58ed1771d2b7ca8bec7123fe9f88db6c88de37e38cd6a8da71cbdf134e75bf","observation_id":"fd6a25e4-1b1f-4c2b-b51c-4dd4d4f92ffc","resolution":{"observed_at":"2026-08-06T19:39:59.872361Z","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":"2026-08-06T19:40:00.028026Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.028026Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:099b2e7b4f0640cce06d9d1ff8d1069b7fd80f7da327454e36c15ee14ec70876","observation_id":"682981fd-370f-4ec6-86f0-b00b20dafcdf","resolution":{"observed_at":"2026-08-06T19:40:00.028026Z","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":"2026-08-06T19:40:00.144285Z","title":"J., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.144285Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:72dcff824e69b5a118bb38941e22df7e33a7192523391ebd81c01598f0f99df8","observation_id":"900be536-7771-4a1f-a0ea-7eab7069584b","resolution":{"observed_at":"2026-08-06T19:40:00.144285Z","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":"2026-08-06T19:40:00.207096Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.207096Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:9095620fd544cf4da567c8bb9792c8a309541489295f4151496abb03fb778dd3","observation_id":"b1657f73-3173-4dd8-8e00-58d593ce53b3","resolution":{"observed_at":"2026-08-06T19:40:00.207096Z","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":"2026-08-06T19:40:00.290258Z","title":"P., Vogt, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.290258Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:e6b2696ee297cb21ec4377e39df6be61e9ff84f09e63afbc51ee9a3646b3d541","observation_id":"d1b543e1-f192-4cc5-912a-13d3f7e07e48","resolution":{"observed_at":"2026-08-06T19:40:00.290258Z","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":"2026-08-06T19:40:00.339368Z","title":"J., Dawson, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.339368Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:f7b5d801921291d412eb23fdb1ff230e26eab1013702bef2092ea76a6d632cd5","observation_id":"822cc461-5aa6-453e-8ab7-8d3d4fe85e69","resolution":{"observed_at":"2026-08-06T19:40:00.339368Z","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":"2026-08-06T19:40:00.384410Z","title":"J., Marley, M","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.384410Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2893b6b9e72c7d35cdc6bbae97c9ee1ed6d95d3ee68e7174b88247bf1cf49c24","observation_id":"189ae8a3-5f7c-497a-89c1-b8704794399d","resolution":{"observed_at":"2026-08-06T19:40:00.384410Z","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":"2026-08-06T19:40:00.435376Z","title":"2012, The Astrophysical Journal Supplement Series, 202, 5, doi: 10.1088/0067-0049/202/1/5","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.435376Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:6a9199bb933d17074787232987f80fcaaeb92031ed90951a079d0e62f868d47a","observation_id":"fce1c2f8-1d1b-47a0-a148-cbe930a8c55d","resolution":{"observed_at":"2026-08-06T19:40:00.435376Z","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":"2026-08-06T19:40:00.469915Z","title":"2023, in AAS/Division for Planetary Sciences Meeting","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.469915Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:394eff4407479eacf260479e0819e0e9e4d67be991504105c7080238f07a4989","observation_id":"778a6dc8-8398-438d-bc3c-e7a9025f73a3","resolution":{"observed_at":"2026-08-06T19:40:00.469915Z","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":"2026-08-06T19:40:00.528125Z","title":"X., Wang, S., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.528125Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:57b6f79e9309ee4b68641466886fa091e0b730f66bc9e989eeb4383208053491","observation_id":"8d93ce7e-59cc-4285-acfc-2df5e8926e71","resolution":{"observed_at":"2026-08-06T19:40:00.528125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/803/2/111","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:07.831379Z","title":"2015, ApJ, 803, 111, doi: 10.1088/0004-637X/803/2/111 18 —","venue":null,"work_id":"a3dc72b3-21a7-407b-a528-5167c14ab97e","year":2015},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.590997Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:afa3ba8f55036fb986beebcbc65bc262b15506a3ac26509f1feaa5d3f8e5f88f","observation_id":"d92190ea-376a-4db2-a3cc-f2cfdc900671","resolution":{"observed_at":"2026-08-06T19:40:07.890490Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:00.667418Z","title":"1966, Icarus, 5, 375, doi: 10.1016/0019-1035(66)90051-0 Grießmeier, J","venue":null,"work_id":null,"year":1966},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.667418Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:7b741e30c99588ac773820513169f43c725fee406021f59437391662b9009fc6","observation_id":"f3a76211-1d5f-4044-85ee-76ea17a3cbad","resolution":{"observed_at":"2026-08-06T19:40:00.667418Z","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":"2026-08-06T19:40:00.740453Z","title":"1996, ApJL, 459, L35, doi: 10.1086/309935","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.740453Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:bf0633328dcbe9ea15b9c3b4aecf175ffab0c2262fff74429957afab38fbc887","observation_id":"60372da4-0cd0-49d4-b372-1cdc08e2cbec","resolution":{"observed_at":"2026-08-06T19:40:00.740453Z","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":"2026-08-06T19:40:00.787027Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.787027Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:3dc60295eb8e366d53bd887d69694a59f3522c250ad3a5038694cf89f3e91ec5","observation_id":"d1a3d651-fb6a-41bf-9d2c-90fd241a3a82","resolution":{"observed_at":"2026-08-06T19:40:00.787027Z","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":"2026-08-06T19:40:00.823723Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.823723Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:1ce24a3a41f6f9058b2e5717cc6d18c772f6d6d34091672b0b01c785714af9a9","observation_id":"85e023fc-ec3c-4cd1-81af-b90fcb5331dc","resolution":{"observed_at":"2026-08-06T19:40:00.823723Z","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":"2026-08-06T19:40:00.863033Z","title":"2021, ApJ, 908, 77, doi: 10.3847/1538-4357/abd8d1","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.863033Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:183e06665897b95471a778c17a2f0610c6e82e2db03621c3586d5a6ad62f48cb","observation_id":"aaa1d41b-8824-4b0e-abba-07b840a5b560","resolution":{"observed_at":"2026-08-06T19:40:00.863033Z","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":"2026-08-06T19:40:00.908141Z","title":"A., Rubie, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.908141Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:833f23065ecd14d016244a1c52682e17db8d02f8ec92beac5dcf9c8a13068f77","observation_id":"50593036-b8b7-4f95-8e68-fc3dd8a081ca","resolution":{"observed_at":"2026-08-06T19:40:00.908141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab9e70","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:07.593350Z","title":"S., & Cantiello, M","venue":null,"work_id":"3479b2c9-6ad4-4c26-8345-3dfffa1b604a","year":2020},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.945448Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:fc24ca7fd5373952cfa089313381b3a18726ac8a78410c3b489f8cdf6c9e4dfe","observation_id":"19b20f15-149b-4b29-a94b-718065346ad8","resolution":{"observed_at":"2026-08-06T19:40:07.702033Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:00.982840Z","title":"S., Bauer, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:00.982840Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:c79c517f0f2d9b0401cc9a0a286603c239bf49419115ef5a53ed18cff78c5732","observation_id":"0a4b924e-e441-4623-ac70-1f8a25908eb4","resolution":{"observed_at":"2026-08-06T19:40:00.982840Z","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":"2026-08-06T19:40:01.033168Z","title":"2015, A&A, 577, A27, doi: 10.1051/0004-6361/201425300","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.033168Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:d9aec97d1f93f8011ab7bb6a0e85c4ba2f3642e3797c4a68e4f6f813701f76c5","observation_id":"8986d583-9ddd-438a-9f1a-c996e1d5fbbf","resolution":{"observed_at":"2026-08-06T19:40:01.033168Z","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":"2026-08-06T19:40:01.135580Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.135580Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:749c02604b8a37f9328398fda14f33e1623f62056e8d099ecdeed3a23a2d3059","observation_id":"d129a15b-bd55-4872-993a-0ef6e1bb10f7","resolution":{"observed_at":"2026-08-06T19:40:01.135580Z","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":"2026-08-06T19:40:01.229200Z","title":"M., Hallinan, G., Pineda, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.229200Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:efd3d10130d423776baa8c93c206132ddecbdfb42c0215631c8a509d31a783f0","observation_id":"02845c45-b138-41e4-b76b-80c53ddaa4de","resolution":{"observed_at":"2026-08-06T19:40:01.229200Z","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":"2026-08-06T19:40:01.297341Z","title":"2018, ApJS, 237, 25, doi: 10.3847/1538-4365/aac2d5","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.297341Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:72d8f68ef257da8820e5e3625c7ca97c0662dd67020616500855754851512af6","observation_id":"42949a5e-cf4d-4274-a82a-e0bc9a0fae58","resolution":{"observed_at":"2026-08-06T19:40:01.297341Z","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":"2026-08-06T19:40:01.364175Z","title":"A., Allan, A., & Kubyshkina, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.364175Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:318ba6c8e20c976784205380e07b8158b6f74de3d40484d667612d2447a71a58","observation_id":"b7fc63d7-cf6a-49f7-9938-72a2b4dab61e","resolution":{"observed_at":"2026-08-06T19:40:01.364175Z","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":"2026-08-06T19:40:01.417114Z","title":"2022, A&A, 658, L7, doi: 10.1051/0004-6361/202142588","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.417114Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:b65aadacf38b2234a90029c7a8466988e6130f8cd47427efd6edc41d7564af63","observation_id":"ce1e4eca-c5ed-4179-b227-6b62a627c027","resolution":{"observed_at":"2026-08-06T19:40:01.417114Z","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":"2026-08-06T19:40:01.492865Z","title":"A., Charbonneau, D., Allen, L","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.492865Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:5db849aff807432bcf1286a952721a3f2fa2f990cfbd94f144c6784fbb5110cb","observation_id":"2c736f95-1225-44e5-baf7-c1503fd1cd28","resolution":{"observed_at":"2026-08-06T19:40:01.492865Z","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":"2026-08-06T19:40:01.558353Z","title":"2020, ApJ, 893, 36, doi: 10.3847/1538-4357/ab7eb4","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.558353Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:918ec448c08f53d0de002c602ee1a847a271dcf864685b48bb211ea48de42495","observation_id":"3bb92d19-4e17-42fa-b5ad-18cbfa6cdda5","resolution":{"observed_at":"2026-08-06T19:40:01.558353Z","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":"2026-08-06T19:40:01.629531Z","title":"D., & Youdin, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.629531Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:cd7da70a4b7aeffd3b9587f8d6d586979d9d98908d62fa9ce6ea7e569e99c2ba","observation_id":"3b72594a-77b1-43b5-a84d-3230a2f979b3","resolution":{"observed_at":"2026-08-06T19:40:01.629531Z","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":"2026-08-06T19:40:01.713821Z","title":"1986, A&A, 160, 116","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.713821Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:64d519febbf1799c22013daceb092db66f773659e1da2126aed7391d4d721c19","observation_id":"d23c5d4d-67f8-4b91-8db6-760c94e82b83","resolution":{"observed_at":"2026-08-06T19:40:01.713821Z","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":"10.1103/physreve.103.063203","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:07.351623Z","title":"J., Sch¨ ottler, M., et al","venue":null,"work_id":"77a89903-b985-40f9-bd9f-fb72878994a0","year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.779893Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:d533f779e1dee1a56b4e7c4afbe5dfc5882d1e9d205468b10d4f67e78704b010","observation_id":"d6501708-2556-4dfd-8ffb-b1d686b112b5","resolution":{"observed_at":"2026-08-06T19:40:07.423219Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:01.840333Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.840333Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:89e7afb379bf139feee14381f990a0cdfa72e419058f428cd9139951990eb3f2","observation_id":"b1a4f468-8e0d-46f3-ab42-9bbeb66a9038","resolution":{"observed_at":"2026-08-06T19:40:01.840333Z","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":"2026-08-06T19:40:01.907982Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.907982Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:3c0035d96f0055d0f044d096b79a6a57533522fa49dded2796a32a48e8113b61","observation_id":"acf6a370-3169-4ca8-bf0b-048cdca04b01","resolution":{"observed_at":"2026-08-06T19:40:01.907982Z","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":"2026-08-06T19:40:01.974948Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:01.974948Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:230a5c039aba7df994415d6ba8df3c96077534ad32c38d81a19a14adf75299b7","observation_id":"ecab7cae-7202-41f6-bb2e-45127dba5253","resolution":{"observed_at":"2026-08-06T19:40:01.974948Z","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":"2026-08-06T19:40:02.062478Z","title":"2010, ApJ, 725, 1146, doi: 10.1088/0004-637X/725/1/1146","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.062478Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:7612a2d5a98995582d5569401d1fb621674cd69f6104299916476d649ae6469e","observation_id":"b70ded2b-06ef-408b-b9f8-436d2e36f35e","resolution":{"observed_at":"2026-08-06T19:40:02.062478Z","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":"2026-08-06T19:40:02.126745Z","title":"D., & Fortney, J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.126745Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:ff25e08ab28f2695b940e7607a18740d307de64750fec93021d9463721e072cf","observation_id":"e9ec4f75-ab98-4578-b8a7-01fa7e8fd511","resolution":{"observed_at":"2026-08-06T19:40:02.126745Z","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":"2026-08-06T19:40:02.175091Z","title":"2012, ApJ, 745, 138, doi: 10.1088/0004-637X/745/2/138","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.175091Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:ad7abbf375a4cfde3e9e096fdcd048e8c0a9994e78cf143190f59d2500eea4b9","observation_id":"720d68cb-f9da-42d5-9f34-960684663b53","resolution":{"observed_at":"2026-08-06T19:40:02.175091Z","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":"2026-08-06T19:40:02.275309Z","title":"D., & Dermott, S","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.275309Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:7c483ec04c31f6f5243ee603b31e1e752d09d18a32ff09f51cdd6d17ab70a176","observation_id":"65d762c5-7fe5-4ef2-9115-4635da908b30","resolution":{"observed_at":"2026-08-06T19:40:02.275309Z","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":"2026-08-06T19:40:02.335203Z","title":"H., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.335203Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:cf0d881d837644deed5a9cf0287721283ade846e496814ee5de277ce5c00439e","observation_id":"3d2c7d81-6e89-47d0-ad98-0ade961d2a67","resolution":{"observed_at":"2026-08-06T19:40:02.335203Z","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":"10.1130/0091-","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:07.151576Z","title":"2002, Geology, 30, 987, doi: 10.1130/0091- 7613(2002)030⟨0987:WDVLAM⟩2.0.CO;2","venue":null,"work_id":"2feb6584-28e1-431e-a940-2521af5e889b","year":2002},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.420825Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:a410c8acf50a413b63565895502eb89190c2259e381ca28d28ce381f364f0732","observation_id":"badf253d-dc1a-4dbb-a7da-be18b5f54e6e","resolution":{"observed_at":"2026-08-06T19:40:07.191487Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:02.506804Z","title":null,"venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.506804Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:34c3b7ffc5b33d30749f9b4fb78e9315576c510f53b28bc6eda6c0701e806c78","observation_id":"9387ab17-97ad-4aeb-8ef3-e54c0cf5d1e8","resolution":{"observed_at":"2026-08-06T19:40:02.506804Z","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":"2026-08-06T19:40:02.575023Z","title":"2011, ApJS, 192, 3, doi: 10.1088/0067-0049/192/1/3","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.575023Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:29ca608aa92ea21cb21874f94497e9ad1fa82eb39cb2d959c2edf7b871afbc4f","observation_id":"62699f69-0303-4b8c-acdd-2cc0cfd99dc7","resolution":{"observed_at":"2026-08-06T19:40:02.575023Z","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":"2026-08-06T19:40:02.639859Z","title":"2013, ApJS, 208, 4, doi: 10.1088/0067-0049/208/1/4","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.639859Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2abd050454e77a5eae9847deffb045410459accbbb2d8b5039ecd234eb4b87af","observation_id":"8f5f9db4-0ca7-4712-945d-88c3d3764a80","resolution":{"observed_at":"2026-08-06T19:40:02.639859Z","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":"2026-08-06T19:40:02.722968Z","title":"2015, ApJS, 220, 15, doi: 10.1088/0067-0049/220/1/15","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.722968Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:dd8763e9c5c30be74f3f39c0203e16fcedba190dae70327a0307d20b945044af","observation_id":"2cc8d693-cc01-48ac-a1a1-76a16d832919","resolution":{"observed_at":"2026-08-06T19:40:02.722968Z","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":"2026-08-06T19:40:02.785150Z","title":"B., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.785150Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:4856540903d2929d7c3d30be2cd8af0fddecae8da58bf6732ea1fc52b338fd21","observation_id":"52f4460a-2028-46d9-baba-9d6087f5daa5","resolution":{"observed_at":"2026-08-06T19:40:02.785150Z","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":"2026-08-06T19:40:02.871632Z","title":"2019, ApJS, 243, 10, doi: 10.3847/1538-4365/ab2241 P´ erez-Torres, M., G´ omez, J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.871632Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:b0b594e4c293df12c560f8294174e7e7e716468a70bc92a6c97cd4e1fd9e597c","observation_id":"d03b2d46-bf3b-49a6-82bf-96f37f2b7a63","resolution":{"observed_at":"2026-08-06T19:40:02.871632Z","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":"2026-08-06T19:40:02.935459Z","title":"2010a, ApJ, 724, 313, doi: 10.1088/0004-637X/724/1/313 —","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.935459Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:237cd8b4dacd8223ab1626e0b2978ff47c4e8c48bb2cde88c9234075d4943e29","observation_id":"5fbd9c9a-1c48-4389-b29e-bcf5d39fee92","resolution":{"observed_at":"2026-08-06T19:40:02.935459Z","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":"2026-08-06T19:40:02.986822Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:02.986822Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:3450ec2c04efe83097b376cd9d32363554e64c1109e150e3335bf5ad8804f04d","observation_id":"e2391e0f-9743-4321-910f-20f3ddcf7987","resolution":{"observed_at":"2026-08-06T19:40:02.986822Z","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":"2026-08-06T19:40:03.033594Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.033594Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:7cdc985a79c0269205ab9fa074fc8043846eeb86393b0a55c7c7d0c17cc7e804","observation_id":"115b1a4a-5ae0-44dc-bf55-85c029cb7160","resolution":{"observed_at":"2026-08-06T19:40:03.033594Z","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":"2026-08-06T19:40:03.125010Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.125010Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2e0af32e977ae5d1cbc3e075700ca5d70b8716f9f8bb246c8adc679479cc95c7","observation_id":"940c7d51-6a5a-4a02-8be6-810bb016c925","resolution":{"observed_at":"2026-08-06T19:40:03.125010Z","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":"2026-08-06T19:40:03.203440Z","title":"J., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.203440Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:6d6b64cbe694578b8d93aaebd184593174d085f6d828c2fa29de5c499df8aac1","observation_id":"45afc640-c8a4-485d-8847-e892ffacb403","resolution":{"observed_at":"2026-08-06T19:40:03.203440Z","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":"2026-08-06T19:40:03.312074Z","title":"D., & Molli` ere, P","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.312074Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:3545f9844922dec48f8d82a84549c5bf68fdcf2afac7ecfb89d123e9ca0c9d1e","observation_id":"b6c61ed2-01e7-49fe-a1a7-9831186e7238","resolution":{"observed_at":"2026-08-06T19:40:03.312074Z","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":"2026-08-06T19:40:03.403435Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.403435Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:44c9e7cdd64003ebeaa6cd435a04aa851932197c5e59149249d0037fb1809280","observation_id":"7d7ceb14-32a1-4a57-8f52-ed317775f946","resolution":{"observed_at":"2026-08-06T19:40:03.403435Z","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":"2026-08-06T19:40:03.481033Z","title":"2013, A&A, 552, A119, doi: 10.1051/0004-6361/201118179","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.481033Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:a6ceeb5272bed5eb58539a44f52cf317b1fb5c636148fa30fa304e2231a6ac4e","observation_id":"6ddef670-728e-4b3d-88db-f3f867613523","resolution":{"observed_at":"2026-08-06T19:40:03.481033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/722/2/1547","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:06.877151Z","title":null,"venue":null,"work_id":"3da5c990-5d0b-4865-83a9-778106f7a27f","year":2010},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.578965Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:a461855fd817d44cbbb66759b8a5b1ae0eb08862f0b5bb38eda65788b21f4a85","observation_id":"788dbb8a-686b-4ad8-baad-42a461cea9e1","resolution":{"observed_at":"2026-08-06T19:40:06.955932Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:03.686348Z","title":"M., Marsden, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.686348Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:39cabfbd767f181c14f94e5c9ebd97abd4a0b3528d1c5eb6b34682a7ff240bbf","observation_id":"c54e6d14-4f93-4aba-abcf-c28165cf9673","resolution":{"observed_at":"2026-08-06T19:40:03.686348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201731454","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:06.729392Z","title":"2018, A&A, 616, A76, doi: 10.1051/0004-6361/201731454","venue":null,"work_id":"f386c389-f743-478b-8e0f-0f8041da286d","year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.792523Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:af012b3d1e0e6d458b63f8474f7124d0c4351def00cb7d8add1d496feed7a9aa","observation_id":"f42cdeaa-26a0-4862-967b-ea4013e654a8","resolution":{"observed_at":"2026-08-06T19:40:06.757667Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:03.912452Z","title":"A., Dalba, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.912452Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:49e655970266d5c44ff2d3815f455519b0bae779a27627efcd383ee7da4b2a78","observation_id":"7e5f39fe-40fd-48dd-baed-a56bbfe15592","resolution":{"observed_at":"2026-08-06T19:40:03.912452Z","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":"2026-08-06T19:40:03.992733Z","title":"P., Fortney, J","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:03.992733Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:548425e69d91cd0785cf3b949995624d8b36307a8b2a05775dd8c77ed37b03c1","observation_id":"9a53d2a5-59ad-46b6-9da3-aabfd5b30ee1","resolution":{"observed_at":"2026-08-06T19:40:03.992733Z","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":"2026-08-06T19:40:04.068676Z","title":"P., & Guillot, T","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.068676Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:a41a3b74d3fa0b25426aa94de8a1c178eebc00bc98c4bc676152e2520e29f9bd","observation_id":"9e777454-b7e2-456e-9221-3279673f8e4d","resolution":{"observed_at":"2026-08-06T19:40:04.068676Z","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":"2026-08-06T19:40:04.143855Z","title":"2023, MNRAS, 525, 626, doi: 10.1093/mnras/stad2311","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.143855Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:06c03b0a6ce2c561ae71a88073d64def3790443207ff4c6013616325036531fb","observation_id":"52c0ccc1-0e9d-4fa9-b707-06be8ff981d4","resolution":{"observed_at":"2026-08-06T19:40:04.143855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.14342","last_updated":"2025-05-20T13:28:59Z","snapshot_observed_at":"2026-08-07T15:33:54.856857Z","submitted_at":"2025-05-20T13:28:59Z","title":"Non-ideal MHD simulations of hot Jupiter atmospheres","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.14342","snapshot_observed_at":"2026-08-06T19:40:04.197035Z","title":"2025, arXiv e-prints, arXiv:2505.14342, doi: 10.48550/arXiv.2505.14342","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.197035Z"},"links":{"cited_paper":"/paper/2505.14342","citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:8a7ca82a248683057fc8c3856b36126336a145029ff22474c7ebfb3edec0ce5a","observation_id":"585383fc-cfa0-4728-b372-a226ae23972c","resolution":{"observed_at":"2026-08-06T19:40:04.197035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/772/1/76","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:06.543575Z","title":"S., & Burrows, A","venue":null,"work_id":"ecf0708d-58dc-45a6-b2c0-8a0467d9ccf4","year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.282023Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:59ca74b42e6d79dc7535d948fe1b94b10e458c18f406b9836173b094ab992321","observation_id":"81755040-24dc-44d6-af9f-50aba3008290","resolution":{"observed_at":"2026-08-06T19:40:06.605588Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:04.378988Z","title":"G., Collins, K","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.378988Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:6eabab1e2e03e9b361b026b2fec2968f3be5684e91f9516ddaf482560a4bdf61","observation_id":"84ff3d8d-e76f-46a2-9b8a-133cb03f5718","resolution":{"observed_at":"2026-08-06T19:40:04.378988Z","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":"2026-08-06T19:40:04.447020Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.447020Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:11556e3d26ce3f023ae34274d3c6f90e5315e1e485a8ca2c307efd88cc7ad7ee","observation_id":"c3dcb25a-319f-41cc-a726-903673e73b6d","resolution":{"observed_at":"2026-08-06T19:40:04.447020Z","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":"2026-08-06T19:40:04.533173Z","title":"2016, ApJ, 833, 140, doi: 10.3847/1538-4357/833/2/140","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.533173Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:0e9c3fceb3afcb7f311a14534f49b662e0fe2a1f964519df5eacd11daae88acc","observation_id":"9e5d1bae-2739-435b-b446-e119248d8bcb","resolution":{"observed_at":"2026-08-06T19:40:04.533173Z","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":"2026-08-06T19:40:04.603828Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.603828Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2090512d7031f4cf3c6ca9422f8e8564471b7db3067f4f606342c7e1241d2e38","observation_id":"13b6bff3-0c91-4c8d-8577-63cb0eb79de0","resolution":{"observed_at":"2026-08-06T19:40:04.603828Z","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":"2026-08-06T19:40:04.683555Z","title":"P., & Fortney, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.683555Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:30ab92b14d299a37232d6cabc9924e883a37541a533deadcac1700df5f62783e","observation_id":"0dbe8ea0-6c1e-40cb-bbda-2fd7189b0fb4","resolution":{"observed_at":"2026-08-06T19:40:04.683555Z","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":"2026-08-06T19:40:04.816717Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.816717Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:8cccf26829c1fca77c19295f7203f01c29d53347ec5ae75370ed02884955c501","observation_id":"70f4898b-67f5-45fb-a4b4-74f4960bcc96","resolution":{"observed_at":"2026-08-06T19:40:04.816717Z","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":"2026-08-06T19:40:04.908839Z","title":"2024, A&A, 688, A66, doi: 10.1051/0004-6361/202450095","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:04.908839Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:f9980d31e8f5706fecaf08075fdd923e05cc1da3f8f57c3d59ca0631759ea1ae","observation_id":"2e3c58c6-544a-4cd9-bf70-de6789cc3f7e","resolution":{"observed_at":"2026-08-06T19:40:04.908839Z","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":"2026-08-06T19:40:05.007784Z","title":"D., Zarka, P., Grießmeier, J.-M., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.007784Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:096bbc87a79cae63f1d73eeb5339ec8adc1df5b6e6519126f2bb0155f91bb909","observation_id":"c294e306-3f0f-4419-b98d-0dd54051ad6e","resolution":{"observed_at":"2026-08-06T19:40:05.007784Z","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":"2026-08-06T19:40:05.092476Z","title":"M., Hubbard, W","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.092476Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:13c2422d61688bd0bb47460ec51ddb7b9204224c9ea91da95e61eeb64dc5eef0","observation_id":"4560b4a1-da08-4f86-ae49-95df6c75b42b","resolution":{"observed_at":"2026-08-06T19:40:05.092476Z","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":"2026-08-06T19:40:05.159214Z","title":"2025, ApJL, 979, L31, doi: 10.3847/2041-8213/ada954","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.159214Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:2492959044af4e6636a64e3d9600269114828ca0702f859233224356c15c632d","observation_id":"aa9dce14-ff6e-45b5-af11-d1086f3d4d02","resolution":{"observed_at":"2026-08-06T19:40:05.159214Z","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":"2026-08-06T19:40:05.230849Z","title":"M., Marcy, G","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.230849Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:4797145a5e614751e9257e5ab7038221ea6da4dc4346c254b575d2e0c3288f21","observation_id":"17b412c8-84c8-49ea-929e-5d3e59aceddf","resolution":{"observed_at":"2026-08-06T19:40:05.230849Z","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":"2026-08-06T19:40:05.317480Z","title":"2005, ApJL, 628, L143, doi: 10.1086/432716","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.317480Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:cca367b75d12e2a310566b8609bb1f03650d558cb0cbf7fffe85f4cfc1d67ce3","observation_id":"6726c6b7-8d68-42f6-9834-0b6e8363dc95","resolution":{"observed_at":"2026-08-06T19:40:05.317480Z","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":"2026-08-06T19:40:05.387951Z","title":"E., M¨ uller, H.-R., Redfield, S., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.387951Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:d5d2148f246d99780c5066771b223498c6865df5936bb34da2a608e66ce622a8","observation_id":"8bdaaca5-67f5-4774-bdd8-c05e5a3dbe55","resolution":{"observed_at":"2026-08-06T19:40:05.387951Z","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":"2026-08-06T19:40:05.475732Z","title":"2013, ApJ, 763, 13, doi: 10.1088/0004-637X/763/1/13","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.475732Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:b19584e10913bcfb2c147de16fe6409cf751bbf88154778c7aff482949853a5c","observation_id":"484c9c70-7880-4ef4-a505-446c436718e1","resolution":{"observed_at":"2026-08-06T19:40:05.475732Z","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":"2026-08-06T19:40:05.563434Z","title":"K., Gastine, T., Christensen, U","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.563434Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:26e5d3d6ce143b6431fb204743c1b89c48242eb782f6e691183d91f7fb6de174","observation_id":"69aa07fc-fde5-4a48-95ae-e928430f640d","resolution":{"observed_at":"2026-08-06T19:40:05.563434Z","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":"2026-08-06T19:40:05.646854Z","title":"K., & Thorngren, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.646854Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:b43d853f2dffe6d54e4f3291e1d79d327a0ce3fabc57fbf00f426c9adfdc09d8","observation_id":"a9a533b9-28ae-4e93-930d-b69def4934cb","resolution":{"observed_at":"2026-08-06T19:40:05.646854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/721/2/1113","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T19:40:06.157626Z","title":"N., & Mitchell, J","venue":null,"work_id":"9538725c-8c1b-447b-95b1-d7baf9c5bd6a","year":2010},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.719718Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:c2a78df15846efc8964a5b6a0acaa34a375bd56bee6769f35f5600da3d55232c","observation_id":"a78adc76-0211-4fba-90df-7ee492024dea","resolution":{"observed_at":"2026-08-06T19:40:06.227790Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T19:40:05.802601Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.802601Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:dd10cd93a8fcc102ebfc01d818b7df89e4da9acd4fae29a26586fe972aa1335d","observation_id":"9452e035-be5d-4439-91c6-c40b531d744d","resolution":{"observed_at":"2026-08-06T19:40:05.802601Z","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":"2026-08-06T19:40:05.916004Z","title":"A., Ryabov, B","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:05.916004Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:1c0ae3a50bf77b9743542b8d8adfef92d871a0f0b9507a01db8efb318e3854ec","observation_id":"11d47c38-3c1c-4e07-82d0-3ac755c63a55","resolution":{"observed_at":"2026-08-06T19:40:05.916004Z","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":"2026-08-06T19:40:06.008799Z","title":"K., & Howard, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T19:40:06.008799Z"},"links":{"citing_paper":"/paper/2507.05202"},"observation_digest":"sha256:9b1665ef024c3b8b27c1d240717ef6be822b30fd2b72c541c89bb05b6accb95c","observation_id":"717a4a39-4178-48d0-8a7d-93312a5dd9b5","resolution":{"observed_at":"2026-08-06T19:40:06.008799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.05202","last_updated":"2025-07-07T17:02:00Z","latest_version":1,"primary_category":"astro-ph.EP","snapshot_observed_at":"2026-08-06T19:27:33.109697Z","submitted_at":"2025-07-07T17:02:00Z","title":"Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters"},"reference_resolution":{"displayed":98,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":90,"verified_exact":7,"verified_fuzzy":0},"total_outbound_references":98},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 98 of 98 outbound references and 1 inbound Pith citation observation for arXiv:2507.05202."}