{"schema":"pith.reference-change-event.v1","doi":"10.3847/2041-8213/ab43d0","canonical_url":"https://pith.science/event/10.3847/2041-8213/ab43d0","json_url":"https://pith.science/event/10.3847/2041-8213/ab43d0.json","not_a_judgment":"This page records that a citing paper's bibliography includes a work with a published notice. It is not a judgment on the citing paper.","primary":{"event_id":234430,"doi":"10.3847/2041-8213/ab43d0","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2020-02-04","title":"Erratum: “The Intrinsic Temperature and Radiative–Convective Boundary Depth in the Atmospheres of Hot Jupiters” (ApJL, 2018, 884, L6)","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","work_arxiv_id":null,"notice_doi":"10.3847/2041-8213/ab6d6c","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.3847/2041-8213/ab43d0","json_href":"/event/10.3847/2041-8213/ab43d0.json"},"events":[{"event_id":234430,"doi":"10.3847/2041-8213/ab43d0","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2020-02-04","title":"Erratum: “The Intrinsic Temperature and Radiative–Convective Boundary Depth in the Atmospheres of Hot Jupiters” (ApJL, 2018, 884, L6)","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","work_arxiv_id":null,"notice_doi":"10.3847/2041-8213/ab6d6c","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.3847/2041-8213/ab43d0","json_href":"/event/10.3847/2041-8213/ab43d0.json"}],"flags":[{"id":2741,"status":"open","status_label":"Open","citing_arxiv_id":"2605.08752","citing_title":"Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes","ref_index":43,"evidence_raw":"The Intrinsic Temperature and Radiative-Convective Boundary Depth in the Atmospheres of Hot Jupiters. , keywords =. doi:10.3847/2041-8213/ab43d0 , archivePrefix =. 1907.07777 , primaryClass =","evidence_cleaned":"The Intrinsic Temperature and Radiative-Convective Boundary Depth in the Atmospheres of Hot Jupiters., keywords =. doi:10.3847/2041-8213/ab43d0, archivePrefix =. 1907.07777, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2020-02-04","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","event_doi":"10.3847/2041-8213/ab43d0","flag_href":"/flags/2741","event_href":"/event/10.3847/2041-8213/ab43d0","paper_href":"/paper/2605.08752","created_at":"2026-07-11T03:19:00.057274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":2744,"status":"open","status_label":"Open","citing_arxiv_id":"2606.00177","citing_title":"Magnesium Silicate Clouds in the Atmosphere of HD 209458b from a Rule-Based Tree-Structured Data Reduction","ref_index":248,"evidence_raw":"doi:10.3847/2041-8213/ab43d0 , eid =. arXiv , author =:1907.07777 , journal =","evidence_cleaned":"doi:10.3847/2041-8213/ab43d0, eid =. arXiv, author =:1907.07777, journal =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2020-02-04","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","event_doi":"10.3847/2041-8213/ab43d0","flag_href":"/flags/2744","event_href":"/event/10.3847/2041-8213/ab43d0","paper_href":"/paper/2606.00177","created_at":"2026-07-11T03:19:00.057274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":2743,"status":"open","status_label":"Open","citing_arxiv_id":"2606.07497","citing_title":"The Roasting Marshmallows Program with IGRINS on Gemini South V: Atmosphere of MASCARA-1b is Enriched in Refractory Elements","ref_index":101,"evidence_raw":"Thorngren, D., Gao, P., & Fortney, J. J. 2019, ApJL, 884, L6, doi: 10.3847/2041-8213/ab43d0","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2020-02-04","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","event_doi":"10.3847/2041-8213/ab43d0","flag_href":"/flags/2743","event_href":"/event/10.3847/2041-8213/ab43d0","paper_href":"/paper/2606.07497","created_at":"2026-07-11T03:19:00.057274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":2742,"status":"open","status_label":"Open","citing_arxiv_id":"2606.22455","citing_title":"Magnetic field strengths of hot giant exoplanets consistent with Solar System values","ref_index":39,"evidence_raw":"The. The Astrophysical Journal , author =. 2019 , pages =. doi:10.3847/2041-8213/ab43d0 , abstract =","evidence_cleaned":"The. The Astrophysical Journal, author =. 2019, pages =. doi:10.3847/2041-8213/ab43d0, abstract =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2020-02-04","work_title":"arXiv , author =:1907.07777 , journal =","work_doi":"10.3847/2041-8213/ab43d0","event_doi":"10.3847/2041-8213/ab43d0","flag_href":"/flags/2742","event_href":"/event/10.3847/2041-8213/ab43d0","paper_href":"/paper/2606.22455","created_at":"2026-07-11T03:19:00.057274Z","dispute_note":null,"disputed_at":null,"disputed_by":null}],"flag_count":4,"flags_open":4,"flags_disputed":0,"desk_url":"https://pith.science/flags"}