{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:IYZTNL7DNTRAUH3TCJVR2GDI7I","short_pith_number":"pith:IYZTNL7D","schema_version":"1.0","canonical_sha256":"463336afe36ce20a1f73126b1d1868fa119e311d59fadf5e809db6f162524584","source":{"kind":"arxiv","id":"2201.00463","version":1},"attestation_state":"computed","paper":{"title":"The APEX Large CO Heterodyne Orion Legacy Survey (ALCOHOLS). I. Survey overview","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Ginsburg, A. Stutz, B. Duffy, B. J. Swift, B. Peters, C. De Breuck, C. J. Davis, C. Kulesa, C. Walker, D. Froebrich, D. Johnstone, D. Mardones, F. Nakamura, H. G. Arce, H. Zinnecker, J. Bally, J. Carpenter, J. Di Francesco, J. Eisl\\\"offel, J. Kloosterman, J. L. Pineda, J. P. Williams, K. Tatematsu, M. D. Smith, M. Heyer, M. J. McCaughrean, P. Bergman, S. T. Megeath, Th. Klein, Thomas Stanke, U. A. Y{\\i}ld{\\i}z, W. Dent","submitted_at":"2022-01-03T03:28:10Z","abstract_excerpt":"The Orion molecular cloud complex harbours the nearest GMCs and site of high-mass star formation. Its YSO populations are thoroughly characterized. The region is therefore a prime target for the study of star formation.\n  Here, we verify the performance of the SuperCAM 64 pixel heterodyne array on APEX. We give a descriptive overview of a set of wide-field CO(3-2) spectral cubes obtained towards the Orion GMC complex, aimed at characterizing the dynamics and structure of the extended molecular gas in diverse regions of the clouds, ranging from very active sites of clustered star formation in 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":"2201.00463","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-01-03T03:28:10Z","cross_cats_sorted":[],"title_canon_sha256":"11a924374217514bb60d3e0c3c8dc51aed2e7b244ac0b3fc81a7ba66b8a66991","abstract_canon_sha256":"eb6789e214b533a27f1d1006fc4118c94b7547981127b091249d20791d923e9a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:04:29.431164Z","signature_b64":"B25sp1KT3zbvz2FwlvMyI1h7Z8Cq8srIiBB1EZvxCHlqUtWx9xhhj/6SAhh7h9Vus3M1Y524C4TsoOLtjl6WAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"463336afe36ce20a1f73126b1d1868fa119e311d59fadf5e809db6f162524584","last_reissued_at":"2026-07-05T04:04:29.430682Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:04:29.430682Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The APEX Large CO Heterodyne Orion Legacy Survey (ALCOHOLS). I. Survey overview","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Ginsburg, A. Stutz, B. Duffy, B. J. Swift, B. Peters, C. De Breuck, C. J. Davis, C. Kulesa, C. Walker, D. Froebrich, D. Johnstone, D. Mardones, F. Nakamura, H. G. Arce, H. Zinnecker, J. Bally, J. Carpenter, J. Di Francesco, J. Eisl\\\"offel, J. Kloosterman, J. L. Pineda, J. P. Williams, K. Tatematsu, M. D. Smith, M. Heyer, M. J. McCaughrean, P. Bergman, S. T. Megeath, Th. Klein, Thomas Stanke, U. A. Y{\\i}ld{\\i}z, W. Dent","submitted_at":"2022-01-03T03:28:10Z","abstract_excerpt":"The Orion molecular cloud complex harbours the nearest GMCs and site of high-mass star formation. Its YSO populations are thoroughly characterized. The region is therefore a prime target for the study of star formation.\n  Here, we verify the performance of the SuperCAM 64 pixel heterodyne array on APEX. We give a descriptive overview of a set of wide-field CO(3-2) spectral cubes obtained towards the Orion GMC complex, aimed at characterizing the dynamics and structure of the extended molecular gas in diverse regions of the clouds, ranging from very active sites of clustered star formation in O"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.00463","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/2201.00463/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":"2201.00463","created_at":"2026-07-05T04:04:29.430739+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.00463v1","created_at":"2026-07-05T04:04:29.430739+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.00463","created_at":"2026-07-05T04:04:29.430739+00:00"},{"alias_kind":"pith_short_12","alias_value":"IYZTNL7DNTRA","created_at":"2026-07-05T04:04:29.430739+00:00"},{"alias_kind":"pith_short_16","alias_value":"IYZTNL7DNTRAUH3T","created_at":"2026-07-05T04:04:29.430739+00:00"},{"alias_kind":"pith_short_8","alias_value":"IYZTNL7D","created_at":"2026-07-05T04:04:29.430739+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/IYZTNL7DNTRAUH3TCJVR2GDI7I","json":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I.json","graph_json":"https://pith.science/api/pith-number/IYZTNL7DNTRAUH3TCJVR2GDI7I/graph.json","events_json":"https://pith.science/api/pith-number/IYZTNL7DNTRAUH3TCJVR2GDI7I/events.json","paper":"https://pith.science/paper/IYZTNL7D"},"agent_actions":{"view_html":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I","download_json":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I.json","view_paper":"https://pith.science/paper/IYZTNL7D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.00463&json=true","fetch_graph":"https://pith.science/api/pith-number/IYZTNL7DNTRAUH3TCJVR2GDI7I/graph.json","fetch_events":"https://pith.science/api/pith-number/IYZTNL7DNTRAUH3TCJVR2GDI7I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I/action/storage_attestation","attest_author":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I/action/author_attestation","sign_citation":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I/action/citation_signature","submit_replication":"https://pith.science/pith/IYZTNL7DNTRAUH3TCJVR2GDI7I/action/replication_record"}},"created_at":"2026-07-05T04:04:29.430739+00:00","updated_at":"2026-07-05T04:04:29.430739+00:00"}