{"schema":"pith.reference-change-event.v1","doi":"10.3847/1538-4357/aaf473","canonical_url":"https://pith.science/event/10.3847/1538-4357/aaf473","json_url":"https://pith.science/event/10.3847/1538-4357/aaf473.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":302964,"doi":"10.3847/1538-4357/aaf473","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2022-08-17","title":"Erratum: “AT2018cow: A Luminous Millimeter Transient” (2019, ApJ, 871, 73)","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","work_arxiv_id":null,"notice_doi":"10.3847/1538-4357/ac847b","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.3847/1538-4357/aaf473","json_href":"/event/10.3847/1538-4357/aaf473.json"},"events":[{"event_id":302964,"doi":"10.3847/1538-4357/aaf473","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2022-08-17","title":"Erratum: “AT2018cow: A Luminous Millimeter Transient” (2019, ApJ, 871, 73)","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","work_arxiv_id":null,"notice_doi":"10.3847/1538-4357/ac847b","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.3847/1538-4357/aaf473","json_href":"/event/10.3847/1538-4357/aaf473.json"}],"flags":[{"id":4138,"status":"open","status_label":"Open","citing_arxiv_id":"1907.05323","citing_title":"Extragalactic astrophysics with next-generation CMB experiments","ref_index":120,"evidence_raw":"Multiple detections per year are expected. Even a non-detection will place interesting constraints on the shock dynamics and on the energy budget of the unknown GRB progenitors. One example of unexpected phenomena that may show up at (sub-)mm wavelengths is the extraordinary extragalactic transient AT2018cow, with an estimated peak ﬂux density of 94 mJy at≃ 100 GHz [120]. This object may herald a new class of energetic transients which at early times are most readily observed at (sub-)mm wavelengths. 5 DETECTING SOURCES IN POLARIZATION Accurate simulations [121] showed that, for a tensor-to-scalar ratior≃ 10−3 (i.e. at levels predicted by models currently of special interest, such as Starobinsky'sR2 and Higgs inﬂation), the overall uncertainty","evidence_cleaned":null,"evidence_source_label":"citation context","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4138","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/1907.05323","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4137,"status":"open","status_label":"Open","citing_arxiv_id":"2601.00947","citing_title":"The Emission and Suppression of Line Features in Luminous Transients","ref_index":25,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4137","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2601.00947","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4145,"status":"open","status_label":"Open","citing_arxiv_id":"2606.09992","citing_title":"EP260321a/SN 2026gzf: The Faintest Shock Breakout Associated with a Broad-Lined Supernova","ref_index":80,"evidence_raw":"AT2018cow: A Luminous Millimeter Transient. , keywords =. doi:10.3847/1538-4357/aaf473 , archivePrefix =. 1810.10880 , primaryClass =","evidence_cleaned":"AT2018cow: A Luminous Millimeter Transient., keywords =. doi:10.3847/1538-4357/aaf473, archivePrefix =. 1810.10880, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4145","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.09992","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4147,"status":"open","status_label":"Open","citing_arxiv_id":"2606.09992","citing_title":"EP260321a/SN 2026gzf: The Faintest Shock Breakout Associated with a Broad-Lined Supernova","ref_index":88,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4147","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.09992","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4144,"status":"open","status_label":"Open","citing_arxiv_id":"2606.11307","citing_title":"Towards improved synchrotron self absorption energy estimates: accounting for inhomogeneous and non-spherical emitting regions","ref_index":22,"evidence_raw":"AT2018cow: A Luminous Millimeter Transient. , keywords =. doi:10.3847/1538-4357/aaf473 , archivePrefix =. 1810.10880 , primaryClass =","evidence_cleaned":"AT2018cow: A Luminous Millimeter Transient., keywords =. doi:10.3847/1538-4357/aaf473, archivePrefix =. 1810.10880, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4144","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.11307","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4143,"status":"open","status_label":"Open","citing_arxiv_id":"2606.12846","citing_title":"Constraining inhomogeneities and asymmetries in SNe, FBOTs, and other high-energy transients from unresolved radio observations","ref_index":114,"evidence_raw":"AT2018cow: A Luminous Millimeter Transient. , keywords =. doi:10.3847/1538-4357/aaf473 , archivePrefix =. 1810.10880 , primaryClass =","evidence_cleaned":"AT2018cow: A Luminous Millimeter Transient., keywords =. doi:10.3847/1538-4357/aaf473, archivePrefix =. 1810.10880, primaryClass =","evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4143","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.12846","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4142,"status":"open","status_label":"Open","citing_arxiv_id":"2606.17129","citing_title":"Constraints on Late-Time Flaring from Luminous Fast Blue Optical Transients using the Transiting Exoplanet Survey Satellite and the Zwicky Transient Facility","ref_index":28,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4142","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.17129","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4141,"status":"open","status_label":"Open","citing_arxiv_id":"2606.17136","citing_title":"The Lazuli Space Observatory: Opportunities for time-domain and multi-messenger astronomy","ref_index":77,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4141","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.17136","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4140,"status":"open","status_label":"Open","citing_arxiv_id":"2606.18842","citing_title":"\\texttt{TransFit-MAG}: Self-Consistent Modeling of Magnetar-Powered Transients from Shock Breakout to Spin-Down Heating","ref_index":19,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4140","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.18842","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4139,"status":"open","status_label":"Open","citing_arxiv_id":"2606.23786","citing_title":"A Collapsar-Disk Origin for GW190814","ref_index":34,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Kulkarni, S. R., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4139","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2606.23786","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null},{"id":4146,"status":"open","status_label":"Open","citing_arxiv_id":"2607.05778","citing_title":"Dependence of Particle Acceleration Efficiency on Shock Velocity in Weakly Magnetized Electron-Ion Shocks","ref_index":22,"evidence_raw":"Ho, A. Y. Q., Phinney, E. S., Ravi, V., et al. 2019, ApJ, 871, 73, doi: 10.3847/1538-4357/aaf473","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2022-08-17","work_title":", keywords =","work_doi":"10.3847/1538-4357/aaf473","event_doi":"10.3847/1538-4357/aaf473","flag_href":"/flags/4146","event_href":"/event/10.3847/1538-4357/aaf473","paper_href":"/paper/2607.05778","created_at":"2026-07-11T03:19:06.392014Z","dispute_note":null,"disputed_at":null,"disputed_by":null}],"flag_count":11,"flags_open":11,"flags_disputed":0,"desk_url":"https://pith.science/flags"}