{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:QEUFMXXKTEIDVC7PHMPB2GV3QV","short_pith_number":"pith:QEUFMXXK","schema_version":"1.0","canonical_sha256":"8128565eea99103a8bef3b1e1d1abb8562fcb713fbdcd656940a7394c19c4259","source":{"kind":"arxiv","id":"1304.0565","version":2},"attestation_state":"computed","paper":{"title":"SABOCA 350-micron and LABOCA 870-micron dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Oskari Miettinen, Stella S. R. Offner","submitted_at":"2013-04-02T09:01:13Z","abstract_excerpt":"We present a 350 micron APEX/SABOCA map of IRAS 05399-0121/SMM 1, which is a dense double-core system in Orion B9. We combined these data with our previous LABOCA 870-micron data. The spatial resolution of the new SABOCA image, ~3400 AU, is about 2.6 times better than provided by LABOCA. We also make use of Spitzer infrared observations to characterise the star-formation activity in the source. The source is filamentary and remains a double-core system on the 3400 AU scale probed here, where the projected separation between IRAS 05399 and SMM 1 is 0.14 pc. The broadband spectral energy distrib"},"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":"1304.0565","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-04-02T09:01:13Z","cross_cats_sorted":[],"title_canon_sha256":"0018c8914b4d447ec31f30d744f0e042261cf6d6c41cae15b05e4e9fa13a97ab","abstract_canon_sha256":"1faa218d4cb85c846b18cde9396bbc394772966f948979f649370bada9d192c2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:50.132670Z","signature_b64":"RoMzfZw59usCQHGUukR/TazI7sA/x5yjaFfX2bfAPPdytmNXdgbm1Ys1WLySas8CQqUUSRgFairh2G+/HUvPCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8128565eea99103a8bef3b1e1d1abb8562fcb713fbdcd656940a7394c19c4259","last_reissued_at":"2026-05-18T01:50:50.132095Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:50.132095Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SABOCA 350-micron and LABOCA 870-micron dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Oskari Miettinen, Stella S. R. Offner","submitted_at":"2013-04-02T09:01:13Z","abstract_excerpt":"We present a 350 micron APEX/SABOCA map of IRAS 05399-0121/SMM 1, which is a dense double-core system in Orion B9. We combined these data with our previous LABOCA 870-micron data. The spatial resolution of the new SABOCA image, ~3400 AU, is about 2.6 times better than provided by LABOCA. We also make use of Spitzer infrared observations to characterise the star-formation activity in the source. The source is filamentary and remains a double-core system on the 3400 AU scale probed here, where the projected separation between IRAS 05399 and SMM 1 is 0.14 pc. The broadband spectral energy distrib"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.0565","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":""},"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":"1304.0565","created_at":"2026-05-18T01:50:50.132187+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.0565v2","created_at":"2026-05-18T01:50:50.132187+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.0565","created_at":"2026-05-18T01:50:50.132187+00:00"},{"alias_kind":"pith_short_12","alias_value":"QEUFMXXKTEID","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"QEUFMXXKTEIDVC7P","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"QEUFMXXK","created_at":"2026-05-18T12:27:57.521954+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/QEUFMXXKTEIDVC7PHMPB2GV3QV","json":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV.json","graph_json":"https://pith.science/api/pith-number/QEUFMXXKTEIDVC7PHMPB2GV3QV/graph.json","events_json":"https://pith.science/api/pith-number/QEUFMXXKTEIDVC7PHMPB2GV3QV/events.json","paper":"https://pith.science/paper/QEUFMXXK"},"agent_actions":{"view_html":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV","download_json":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV.json","view_paper":"https://pith.science/paper/QEUFMXXK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.0565&json=true","fetch_graph":"https://pith.science/api/pith-number/QEUFMXXKTEIDVC7PHMPB2GV3QV/graph.json","fetch_events":"https://pith.science/api/pith-number/QEUFMXXKTEIDVC7PHMPB2GV3QV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV/action/storage_attestation","attest_author":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV/action/author_attestation","sign_citation":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV/action/citation_signature","submit_replication":"https://pith.science/pith/QEUFMXXKTEIDVC7PHMPB2GV3QV/action/replication_record"}},"created_at":"2026-05-18T01:50:50.132187+00:00","updated_at":"2026-05-18T01:50:50.132187+00:00"}