{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:YI3YQGGOGFNGP54ZW5ENEA354T","short_pith_number":"pith:YI3YQGGO","schema_version":"1.0","canonical_sha256":"c2378818ce315a67f799b748d2037de4f6522f3cc8ce66ac826b71f1d4a829d5","source":{"kind":"arxiv","id":"astro-ph/0512382","version":1},"attestation_state":"computed","paper":{"title":"Large Area Mapping at 850 Microns. IV. Analysis of the Clump Distribution in the Orion B South Molecular Cloud","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Doug Johnstone, George F. Mitchell, Henry Matthews","submitted_at":"2005-12-15T00:18:28Z","abstract_excerpt":"We present results from a survey of a 1300 arcmin^2 region of the Orion B South molecular cloud, including NGC 2024, NGC 2023, and the Horsehead Nebula (B33), obtained using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope. Submillimeter continuum observations at 450 microns and 850 microns are discussed. Using an automated algorithm, 57 discrete emission features (``clumps'') are identified in the 850 micron map. The physical conditions within these clumps are investigated under the assumption that the objects are in quasi-hydrostatic equilibrium. The"},"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":"astro-ph/0512382","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-12-15T00:18:28Z","cross_cats_sorted":[],"title_canon_sha256":"9546c81c4d4b9dc1fb4603ff41141aff624a5472e7f3074dcded6dfb33f8ee6f","abstract_canon_sha256":"25917272a83fdf809e4993c9c06462bd8c3ec3cfbad5ffb901965a7eb570f463"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:14:44.213608Z","signature_b64":"nqKhaIsmaBDka7TVq6wnDAzyevy+DV/tHZ1IsWmzhqy+zvUNHMnWx5LDwBtOnNmUZXq/M48cBEcU3AhyiXhnBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c2378818ce315a67f799b748d2037de4f6522f3cc8ce66ac826b71f1d4a829d5","last_reissued_at":"2026-07-04T17:14:44.213127Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:14:44.213127Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large Area Mapping at 850 Microns. IV. Analysis of the Clump Distribution in the Orion B South Molecular Cloud","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Doug Johnstone, George F. Mitchell, Henry Matthews","submitted_at":"2005-12-15T00:18:28Z","abstract_excerpt":"We present results from a survey of a 1300 arcmin^2 region of the Orion B South molecular cloud, including NGC 2024, NGC 2023, and the Horsehead Nebula (B33), obtained using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope. Submillimeter continuum observations at 450 microns and 850 microns are discussed. Using an automated algorithm, 57 discrete emission features (``clumps'') are identified in the 850 micron map. The physical conditions within these clumps are investigated under the assumption that the objects are in quasi-hydrostatic equilibrium. The"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0512382","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/astro-ph/0512382/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":"astro-ph/0512382","created_at":"2026-07-04T17:14:44.213182+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0512382v1","created_at":"2026-07-04T17:14:44.213182+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0512382","created_at":"2026-07-04T17:14:44.213182+00:00"},{"alias_kind":"pith_short_12","alias_value":"YI3YQGGOGFNG","created_at":"2026-07-04T17:14:44.213182+00:00"},{"alias_kind":"pith_short_16","alias_value":"YI3YQGGOGFNGP54Z","created_at":"2026-07-04T17:14:44.213182+00:00"},{"alias_kind":"pith_short_8","alias_value":"YI3YQGGO","created_at":"2026-07-04T17:14:44.213182+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/YI3YQGGOGFNGP54ZW5ENEA354T","json":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T.json","graph_json":"https://pith.science/api/pith-number/YI3YQGGOGFNGP54ZW5ENEA354T/graph.json","events_json":"https://pith.science/api/pith-number/YI3YQGGOGFNGP54ZW5ENEA354T/events.json","paper":"https://pith.science/paper/YI3YQGGO"},"agent_actions":{"view_html":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T","download_json":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T.json","view_paper":"https://pith.science/paper/YI3YQGGO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0512382&json=true","fetch_graph":"https://pith.science/api/pith-number/YI3YQGGOGFNGP54ZW5ENEA354T/graph.json","fetch_events":"https://pith.science/api/pith-number/YI3YQGGOGFNGP54ZW5ENEA354T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T/action/storage_attestation","attest_author":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T/action/author_attestation","sign_citation":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T/action/citation_signature","submit_replication":"https://pith.science/pith/YI3YQGGOGFNGP54ZW5ENEA354T/action/replication_record"}},"created_at":"2026-07-04T17:14:44.213182+00:00","updated_at":"2026-07-04T17:14:44.213182+00:00"}