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We determine the masses to be $M(D_{sJ}^+(2317)) = 2317.2 \\pm 0.5(\\mathrm{stat}) \\pm 0.9(\\mathrm{syst}) \\mathrm{MeV}/c^2$ and $M(D_{sJ}^+(2457))=2456.5 \\pm 1.3(\\mathrm{stat}) \\pm 1.3(\\mathrm{syst}) \\mathrm{MeV}/c^2$. We observe the radiative decay mode $D_{sJ}^"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"hep-ex/0307052","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ex","submitted_at":"2003-07-18T02:18:26Z","cross_cats_sorted":[],"title_canon_sha256":"672a57b1caf4a8f482622c4c64b02184137f508db18bc5c66a006a134f8b492f","abstract_canon_sha256":"b0e498cab46c9334219372a5292b05ff5c1156fd3d16d1bce4e67cfb273f1005"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:24:11.711025Z","signature_b64":"e7PqfHcavQhXJzIM1FvdJScCW8lun5p2IlfWdLwxjDGXXvBB3fjsLhRZKDw0+3Y/xSu3PgpgSGynuSa8cqmQBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a302c012ed32b6ef1fb9730ac604a66f57c220eeaf5e228ca4107c4d5aa988af","last_reissued_at":"2026-07-04T17:24:11.710606Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:24:11.710606Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurements of the $D_{sJ}$ resonance properties","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"et al. (Belle Collaboration), Y. Mikami","submitted_at":"2003-07-18T02:18:26Z","abstract_excerpt":"We report measurements of the properties of the $D_{sJ}^+(2317)$ and $D_{sJ}^+(2457)$ resonances produced in continuum $e^+ e^-$ annihilation near $\\sqrt{s}=10.6 \\mathrm{GeV}$. The analysis is based on an $86.9 \\mathrm{fb^{-1}}$ data sample collected %at and 60 MeV below the $\\Upsilon(4S)$ resonance with with the Belle detector at KEKB. We determine the masses to be $M(D_{sJ}^+(2317)) = 2317.2 \\pm 0.5(\\mathrm{stat}) \\pm 0.9(\\mathrm{syst}) \\mathrm{MeV}/c^2$ and $M(D_{sJ}^+(2457))=2456.5 \\pm 1.3(\\mathrm{stat}) \\pm 1.3(\\mathrm{syst}) \\mathrm{MeV}/c^2$. We observe the radiative decay mode $D_{sJ}^"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ex/0307052","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ex/0307052/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"hep-ex/0307052","created_at":"2026-07-04T17:24:11.710664+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ex/0307052v2","created_at":"2026-07-04T17:24:11.710664+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ex/0307052","created_at":"2026-07-04T17:24:11.710664+00:00"},{"alias_kind":"pith_short_12","alias_value":"UMBMAEXNGK3O","created_at":"2026-07-04T17:24:11.710664+00:00"},{"alias_kind":"pith_short_16","alias_value":"UMBMAEXNGK3O6H5Z","created_at":"2026-07-04T17:24:11.710664+00:00"},{"alias_kind":"pith_short_8","alias_value":"UMBMAEXN","created_at":"2026-07-04T17:24:11.710664+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.05476","citing_title":"What can we learn from the radiative decays of the $D_{s1}(2460)$ meson?","ref_index":38,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5","json":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5.json","graph_json":"https://pith.science/api/pith-number/UMBMAEXNGK3O6H5ZOMFMMBFGN5/graph.json","events_json":"https://pith.science/api/pith-number/UMBMAEXNGK3O6H5ZOMFMMBFGN5/events.json","paper":"https://pith.science/paper/UMBMAEXN"},"agent_actions":{"view_html":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5","download_json":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5.json","view_paper":"https://pith.science/paper/UMBMAEXN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ex/0307052&json=true","fetch_graph":"https://pith.science/api/pith-number/UMBMAEXNGK3O6H5ZOMFMMBFGN5/graph.json","fetch_events":"https://pith.science/api/pith-number/UMBMAEXNGK3O6H5ZOMFMMBFGN5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5/action/storage_attestation","attest_author":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5/action/author_attestation","sign_citation":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5/action/citation_signature","submit_replication":"https://pith.science/pith/UMBMAEXNGK3O6H5ZOMFMMBFGN5/action/replication_record"}},"created_at":"2026-07-04T17:24:11.710664+00:00","updated_at":"2026-07-04T17:24:11.710664+00:00"}