{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:GL4ACZXINET62M5ETNQEGCKB2F","short_pith_number":"pith:GL4ACZXI","schema_version":"1.0","canonical_sha256":"32f80166e86927ed33a49b60430941d15c82dff491f81013b8db6b30075fd26a","source":{"kind":"arxiv","id":"2204.13797","version":1},"attestation_state":"computed","paper":{"title":"Interplay between Young Stars and Molecular Clouds in the Ophiuchus Star-forming Complex","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Aashish Gupta, Wen-Ping Chen","submitted_at":"2022-04-28T22:07:14Z","abstract_excerpt":"We present spatial and kinematic correlation between the young stellar population and the cloud clumps in the Ophiuchus star-forming region. The stellar sample consists of known young objects at various evolutionary stages, taken from the literature, some of which are diagnosed with Gaia EDR3 parallax and proper-motion measurements. The molecular gas is traced by the 850 $\\mu$m Submillimetre Common-User Bolometer Array-2 image, reaching $\\sim$2.3 mJy beam$^{-1}$, the deepest so far for the region, stacked from the James Clerk Maxwell Telescope/Transient program aiming to detect submillimeter o"},"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":"2204.13797","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-04-28T22:07:14Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"d6cf8db0a62c6fb0b5d91fb33d53f920105b7a42cf8e2a1dc2c6ac9b0025375e","abstract_canon_sha256":"6389c05d8addf9a4c6cf4cd49f0f5837c0e2f238c4633e1231c8ee284f28beb3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:18:53.657389Z","signature_b64":"rY0TzFgeTh5PzuH5IzsyLjaovmzj96xPfScukqgen1PvrZZWYaRdXXTByxr4Uux3EpPz3KigQ6NTqZ6XoAsuCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"32f80166e86927ed33a49b60430941d15c82dff491f81013b8db6b30075fd26a","last_reissued_at":"2026-07-05T04:18:53.656941Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:18:53.656941Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interplay between Young Stars and Molecular Clouds in the Ophiuchus Star-forming Complex","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Aashish Gupta, Wen-Ping Chen","submitted_at":"2022-04-28T22:07:14Z","abstract_excerpt":"We present spatial and kinematic correlation between the young stellar population and the cloud clumps in the Ophiuchus star-forming region. The stellar sample consists of known young objects at various evolutionary stages, taken from the literature, some of which are diagnosed with Gaia EDR3 parallax and proper-motion measurements. The molecular gas is traced by the 850 $\\mu$m Submillimetre Common-User Bolometer Array-2 image, reaching $\\sim$2.3 mJy beam$^{-1}$, the deepest so far for the region, stacked from the James Clerk Maxwell Telescope/Transient program aiming to detect submillimeter o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2204.13797","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/2204.13797/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":"2204.13797","created_at":"2026-07-05T04:18:53.657001+00:00"},{"alias_kind":"arxiv_version","alias_value":"2204.13797v1","created_at":"2026-07-05T04:18:53.657001+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2204.13797","created_at":"2026-07-05T04:18:53.657001+00:00"},{"alias_kind":"pith_short_12","alias_value":"GL4ACZXINET6","created_at":"2026-07-05T04:18:53.657001+00:00"},{"alias_kind":"pith_short_16","alias_value":"GL4ACZXINET62M5E","created_at":"2026-07-05T04:18:53.657001+00:00"},{"alias_kind":"pith_short_8","alias_value":"GL4ACZXI","created_at":"2026-07-05T04:18:53.657001+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/GL4ACZXINET62M5ETNQEGCKB2F","json":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F.json","graph_json":"https://pith.science/api/pith-number/GL4ACZXINET62M5ETNQEGCKB2F/graph.json","events_json":"https://pith.science/api/pith-number/GL4ACZXINET62M5ETNQEGCKB2F/events.json","paper":"https://pith.science/paper/GL4ACZXI"},"agent_actions":{"view_html":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F","download_json":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F.json","view_paper":"https://pith.science/paper/GL4ACZXI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2204.13797&json=true","fetch_graph":"https://pith.science/api/pith-number/GL4ACZXINET62M5ETNQEGCKB2F/graph.json","fetch_events":"https://pith.science/api/pith-number/GL4ACZXINET62M5ETNQEGCKB2F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F/action/storage_attestation","attest_author":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F/action/author_attestation","sign_citation":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F/action/citation_signature","submit_replication":"https://pith.science/pith/GL4ACZXINET62M5ETNQEGCKB2F/action/replication_record"}},"created_at":"2026-07-05T04:18:53.657001+00:00","updated_at":"2026-07-05T04:18:53.657001+00:00"}