{"schema":"pith.reference-change-event.v1","doi":"10.1007/s11433-023-2179-9","canonical_url":"https://pith.science/event/10.1007/s11433-023-2179-9","json_url":"https://pith.science/event/10.1007/s11433-023-2179-9.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":438245,"doi":"10.1007/s11433-023-2179-9","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-12-13","title":"Erratum to: Detecting gravitational wave with an interferometric seismometer array on lunar nearside","work_title":null,"work_doi":"10.1007/s11433-023-2179-9","work_arxiv_id":null,"notice_doi":"10.1007/s11433-023-2250-y","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1007/s11433-023-2179-9","json_href":"/event/10.1007/s11433-023-2179-9.json"},"events":[{"event_id":438245,"doi":"10.1007/s11433-023-2179-9","event_type":"correction","event_type_label":"Correction","source":"crossref","source_label":"Crossref","event_date":"2023-12-13","title":"Erratum to: Detecting gravitational wave with an interferometric seismometer array on lunar nearside","work_title":null,"work_doi":"10.1007/s11433-023-2179-9","work_arxiv_id":null,"notice_doi":"10.1007/s11433-023-2250-y","flag_count":0,"flags_open":0,"flags_disputed":0,"latest_flag_at":null,"human_href":"/event/10.1007/s11433-023-2179-9","json_href":"/event/10.1007/s11433-023-2179-9.json"}],"flags":[{"id":9347,"status":"open","status_label":"Open","citing_arxiv_id":"2502.02995","citing_title":"Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna","ref_index":18,"evidence_raw":"Li, J., Liu, F., Pan, Y ., Wang, Z., Cao, M., Wang, M., Zhang, F., Zhang, J., Zhu, Z.-H.: Detecting gravitational wave with an interferometric seismometer array on lunar nearside. Sci. China Phys. Mech. Astron. 66(10), 109513 (2023) https://doi.org/10.1007/s11433-023-2179-9 . [Erratum: Sci.China Phys.Mech.Astron. 67, 219551 (2024)] 7 101 103 105 m2 [M⊙] q < 1 q > 10 z = 0.05 z = 0.1 z = 0.5 102 103 104 105 m1 [M⊙] 101 103 105 m2 [M⊙] q < 1 q > 10 z = 1 102 103 104 105 m1 [M⊙] z = 5 102 103 104 105 m1 [M⊙] z = 10 10□310□210□1100101 ∆ z/(1 + z) Fig. 5 Same as Fig. 2, but for the angle-averaged relative error of the redshift, ∆z/(1 + z)","evidence_cleaned":null,"evidence_source_label":"bibliography line","event_type":"correction","event_type_label":"Correction","source_label":"Crossref","event_date":"2023-12-13","work_title":null,"work_doi":"10.1007/s11433-023-2179-9","event_doi":"10.1007/s11433-023-2179-9","flag_href":"/flags/9347","event_href":"/event/10.1007/s11433-023-2179-9","paper_href":"/paper/2502.02995","created_at":"2026-08-09T12:17:52.938498Z","dispute_note":null,"disputed_at":null,"disputed_by":null}],"flag_count":1,"flags_open":1,"flags_disputed":0,"desk_url":"https://pith.science/flags"}