{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:3SC6J6XB7CIS4TDSTXJ6B6P3RF","short_pith_number":"pith:3SC6J6XB","schema_version":"1.0","canonical_sha256":"dc85e4fae1f8912e4c729dd3e0f9fb896ede7b9de766f7e5df5f8e777a597251","source":{"kind":"arxiv","id":"1211.1430","version":2},"attestation_state":"computed","paper":{"title":"A mapping study of L1174 with 13CO J=2-1 and 12CO J=3-2: star formation triggered by a Herbig Ae/Be star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Peking University, (3) Universit\\\"at zu K\\\"oln), J. H. Yuan (1), J. Z. Li (1), M. Miller (3) ((1) NAOC, W. Yu (2), Y. Wu (2)","submitted_at":"2012-11-07T00:53:34Z","abstract_excerpt":"We have carried out a comprehensive study of the molecular conditions and star-forming activities in dark cloud L1174 with multi-wavelength data. Mapping observations of L1174 in $^{13}$CO $J=2-1$ and $^{12}$CO $J=3-2$ were performed using the KOSMA 3-meter telescope. Six molecular cores with masses ranging from 5 to 31 $M_\\odot$ and sizes ranging from 0.17 to 0.39 pc are resolved. Large area ahead of a Herbig Be star, HD 200775, is in expanding and core 1 is with collapse signature. Large line widths of $^{13}$CO $J=2-1$ indicate the ubiquity of turbulent motions in this region. Spectra of $^"},"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":"1211.1430","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-11-07T00:53:34Z","cross_cats_sorted":[],"title_canon_sha256":"9e6de5f771a5b3106b98ce305c99fc409de0070b0eb827bce780e38597c4da62","abstract_canon_sha256":"1d40092b5b5914928f447749faa3c1e57aca243159ca0c8c304753f06cda3874"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:24.653066Z","signature_b64":"dmhJ3b7bksBFfbUj46hb3DXS6kDUNkdTgOKkfq/fH/o3j3K7idMcszNY9gkeFKIoDh7rYLnWWvNMDIBAYI1bCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc85e4fae1f8912e4c729dd3e0f9fb896ede7b9de766f7e5df5f8e777a597251","last_reissued_at":"2026-05-18T01:53:24.652565Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:24.652565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A mapping study of L1174 with 13CO J=2-1 and 12CO J=3-2: star formation triggered by a Herbig Ae/Be star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Peking University, (3) Universit\\\"at zu K\\\"oln), J. H. Yuan (1), J. Z. Li (1), M. Miller (3) ((1) NAOC, W. Yu (2), Y. Wu (2)","submitted_at":"2012-11-07T00:53:34Z","abstract_excerpt":"We have carried out a comprehensive study of the molecular conditions and star-forming activities in dark cloud L1174 with multi-wavelength data. Mapping observations of L1174 in $^{13}$CO $J=2-1$ and $^{12}$CO $J=3-2$ were performed using the KOSMA 3-meter telescope. Six molecular cores with masses ranging from 5 to 31 $M_\\odot$ and sizes ranging from 0.17 to 0.39 pc are resolved. Large area ahead of a Herbig Be star, HD 200775, is in expanding and core 1 is with collapse signature. Large line widths of $^{13}$CO $J=2-1$ indicate the ubiquity of turbulent motions in this region. Spectra of $^"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.1430","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":"1211.1430","created_at":"2026-05-18T01:53:24.652640+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.1430v2","created_at":"2026-05-18T01:53:24.652640+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.1430","created_at":"2026-05-18T01:53:24.652640+00:00"},{"alias_kind":"pith_short_12","alias_value":"3SC6J6XB7CIS","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"3SC6J6XB7CIS4TDS","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"3SC6J6XB","created_at":"2026-05-18T12:26:53.410803+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/3SC6J6XB7CIS4TDSTXJ6B6P3RF","json":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF.json","graph_json":"https://pith.science/api/pith-number/3SC6J6XB7CIS4TDSTXJ6B6P3RF/graph.json","events_json":"https://pith.science/api/pith-number/3SC6J6XB7CIS4TDSTXJ6B6P3RF/events.json","paper":"https://pith.science/paper/3SC6J6XB"},"agent_actions":{"view_html":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF","download_json":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF.json","view_paper":"https://pith.science/paper/3SC6J6XB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.1430&json=true","fetch_graph":"https://pith.science/api/pith-number/3SC6J6XB7CIS4TDSTXJ6B6P3RF/graph.json","fetch_events":"https://pith.science/api/pith-number/3SC6J6XB7CIS4TDSTXJ6B6P3RF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF/action/storage_attestation","attest_author":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF/action/author_attestation","sign_citation":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF/action/citation_signature","submit_replication":"https://pith.science/pith/3SC6J6XB7CIS4TDSTXJ6B6P3RF/action/replication_record"}},"created_at":"2026-05-18T01:53:24.652640+00:00","updated_at":"2026-05-18T01:53:24.652640+00:00"}