{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:JZNAY4QCONYLHGA2W33CSMZE3X","short_pith_number":"pith:JZNAY4QC","schema_version":"1.0","canonical_sha256":"4e5a0c72027370b3981ab6f6293324dde76439e13bc907f939b3e5ea6af82c6e","source":{"kind":"arxiv","id":"2310.11999","version":1},"attestation_state":"computed","paper":{"title":"IRAS4A1: Multi-wavelength continuum analysis of a very flared Class 0 disk","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"C. Carrasco-Gonz\\'alez, D. J. Wilner, E. G. Cox, E. Mac\\'ias, J. Di Francesco, J. J. Tobin, L. W. Looney, N. Van der Marel, O. M. Guerra-Alvarado, P. D. Sheehan","submitted_at":"2023-10-18T14:31:08Z","abstract_excerpt":"Understanding the formation of substructures in protoplanetary disks is vital for gaining insights into dust growth and the process of planet formation. Studying these substructures in highly embedded Class 0 objects using the Atacama Large Millimeter/submillimeter Array (ALMA), however, poses significant challenges. Nonetheless, it is imperative to do so to unravel the mechanisms and timing behind the formation of these substructures. In this study, we present high-resolution ALMA data at Bands 6 and 4 of the NGC1333 IRAS4A Class 0 protobinary system. This system consists of two components, A"},"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":"2310.11999","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-10-18T14:31:08Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"4fdf5df30e6bff9b71b29b53d11f98613ef61507b04a1a8215b7af8c18ae1800","abstract_canon_sha256":"8bc52e20a6adf2d7837f48c30e11832cf0c7721fb4e159358602bd1ea95ea3dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:36:44.234530Z","signature_b64":"kF9CyvqTgf8fQOuiFRJxcCCnu9rAmytD0s+n7q2l1nSBw7k9F7GrCpxJhjevgMn8RS035oEOPP5WD8zMRDJOAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e5a0c72027370b3981ab6f6293324dde76439e13bc907f939b3e5ea6af82c6e","last_reissued_at":"2026-07-05T07:36:44.233977Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:36:44.233977Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"IRAS4A1: Multi-wavelength continuum analysis of a very flared Class 0 disk","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"C. Carrasco-Gonz\\'alez, D. J. Wilner, E. G. Cox, E. Mac\\'ias, J. Di Francesco, J. J. Tobin, L. W. Looney, N. Van der Marel, O. M. Guerra-Alvarado, P. D. Sheehan","submitted_at":"2023-10-18T14:31:08Z","abstract_excerpt":"Understanding the formation of substructures in protoplanetary disks is vital for gaining insights into dust growth and the process of planet formation. Studying these substructures in highly embedded Class 0 objects using the Atacama Large Millimeter/submillimeter Array (ALMA), however, poses significant challenges. Nonetheless, it is imperative to do so to unravel the mechanisms and timing behind the formation of these substructures. In this study, we present high-resolution ALMA data at Bands 6 and 4 of the NGC1333 IRAS4A Class 0 protobinary system. This system consists of two components, A"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.11999","kind":"arxiv","version":1},"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/2310.11999/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":"2310.11999","created_at":"2026-07-05T07:36:44.234050+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.11999v1","created_at":"2026-07-05T07:36:44.234050+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.11999","created_at":"2026-07-05T07:36:44.234050+00:00"},{"alias_kind":"pith_short_12","alias_value":"JZNAY4QCONYL","created_at":"2026-07-05T07:36:44.234050+00:00"},{"alias_kind":"pith_short_16","alias_value":"JZNAY4QCONYLHGA2","created_at":"2026-07-05T07:36:44.234050+00:00"},{"alias_kind":"pith_short_8","alias_value":"JZNAY4QC","created_at":"2026-07-05T07:36:44.234050+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X","json":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X.json","graph_json":"https://pith.science/api/pith-number/JZNAY4QCONYLHGA2W33CSMZE3X/graph.json","events_json":"https://pith.science/api/pith-number/JZNAY4QCONYLHGA2W33CSMZE3X/events.json","paper":"https://pith.science/paper/JZNAY4QC"},"agent_actions":{"view_html":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X","download_json":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X.json","view_paper":"https://pith.science/paper/JZNAY4QC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.11999&json=true","fetch_graph":"https://pith.science/api/pith-number/JZNAY4QCONYLHGA2W33CSMZE3X/graph.json","fetch_events":"https://pith.science/api/pith-number/JZNAY4QCONYLHGA2W33CSMZE3X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X/action/storage_attestation","attest_author":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X/action/author_attestation","sign_citation":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X/action/citation_signature","submit_replication":"https://pith.science/pith/JZNAY4QCONYLHGA2W33CSMZE3X/action/replication_record"}},"created_at":"2026-07-05T07:36:44.234050+00:00","updated_at":"2026-07-05T07:36:44.234050+00:00"}