{"schema":"pith.reference-change-event.v1","doi":"10.1038/s41586-023-06499-2","canonical_url":"https://pith.science/event/10.1038/s41586-023-06499-2","json_url":"https://pith.science/event/10.1038/s41586-023-06499-2.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":272016,"doi":"10.1038/s41586-023-06499-2","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-10-20","title":"Author Correction: A super-massive Neptune-sized planet","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","work_arxiv_id":null,"notice_doi":"10.1038/s41586-023-06748-4","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1038/s41586-023-06499-2","json_href":"/event/10.1038/s41586-023-06499-2.json"},"events":[{"event_id":272016,"doi":"10.1038/s41586-023-06499-2","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-10-20","title":"Author Correction: A super-massive Neptune-sized planet","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","work_arxiv_id":null,"notice_doi":"10.1038/s41586-023-06748-4","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1038/s41586-023-06499-2","json_href":"/event/10.1038/s41586-023-06499-2.json"}],"flags":[{"id":3558,"status":"open","status_label":"Open","citing_arxiv_id":"2604.06029","citing_title":"The Cohesive Object Sequence: The Mass-Density Distribution of Astronomical Objects from Asteroids to Stars","ref_index":56,"evidence_raw":"Naponiello, L., Mancini, L., Sozzetti, A., et al. 2023, Nature, 622, 255–260, doi: 10.1038/s41586-023-06499-2 NASA Exoplanet Science Institute. 2020, Planetary Systems Table, IPAC, doi: 10.26133/NEA12 N¨ attil¨ a, J., Miller, M. C., Steiner, A. W., et al. 2017, Astronomy &; Astrophysics, 608, A31, doi: 10.1051/0004-6361/201731082","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3558","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2604.06029","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":3557,"status":"open","status_label":"Open","citing_arxiv_id":"2604.09834","citing_title":"Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune System","ref_index":98,"evidence_raw":"Naponiello, L., Mancini, L., Sozzetti, A., et al. 2023, Nature, 622, 255, doi: 10.1038/s41586-023-06499-2","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3557","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2604.09834","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":3556,"status":"open","status_label":"Open","citing_arxiv_id":"2604.19179","citing_title":"A tidally detached super Neptune on a strongly misaligned retrograde orbit","ref_index":240,"evidence_raw":"A super-massive Neptune-sized planet. , keywords =. doi:10.1038/s41586-023-06499-2 , archivePrefix =. 2309.01464 , primaryClass =","evidence_cleaned":"A super-massive Neptune-sized planet., keywords =. doi:10.1038/s41586-023-06499-2, archivePrefix =. 2309.01464, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3556","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2604.19179","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":3560,"status":"open","status_label":"Open","citing_arxiv_id":"2606.20789","citing_title":"Dynamical Tides during High-Eccentricity Migration produces the Hot Jupiter Pile-up, Neptune Ridge, and Neptune Desert","ref_index":79,"evidence_raw":"Naponiello, L., Mancini, L., Sozzetti, A., et al. 2023, Nature, 622, 255, doi: 10.1038/s41586-023-06499-2","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3560","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2606.20789","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":3559,"status":"open","status_label":"Open","citing_arxiv_id":"2606.21625","citing_title":"The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c","ref_index":71,"evidence_raw":"A super-massive Neptune-sized planet. , keywords =. doi:10.1038/s41586-023-06499-2 , archivePrefix =. 2309.01464 , primaryClass =","evidence_cleaned":"A super-massive Neptune-sized planet., keywords =. doi:10.1038/s41586-023-06499-2, archivePrefix =. 2309.01464, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3559","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2606.21625","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":3561,"status":"open","status_label":"Open","citing_arxiv_id":"2606.21625","citing_title":"The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c","ref_index":71,"evidence_raw":"A super-massive Neptune-sized planet. , keywords =. doi:10.1038/s41586-023-06499-2 , archivePrefix =. 2309.01464 , primaryClass =","evidence_cleaned":"A super-massive Neptune-sized planet., keywords =. doi:10.1038/s41586-023-06499-2, archivePrefix =. 2309.01464, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-10-20","work_title":", keywords =","work_doi":"10.1038/s41586-023-06499-2","event_doi":"10.1038/s41586-023-06499-2","flag_href":"/flags/3561","event_href":"/event/10.1038/s41586-023-06499-2","paper_href":"/paper/2606.21625","created_at":"2026-07-11T03:19:03.555274Z","dispute_note":null,"disputed_at":null,"disputed_by":null}],"flag_count":6,"flags_open":6,"flags_disputed":0,"desk_url":"https://pith.science/flags"}