{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:2K7RLZI2YACCB263TAILGUFKKI","short_pith_number":"pith:2K7RLZI2","schema_version":"1.0","canonical_sha256":"d2bf15e51ac00420ebdb9810b350aa5208586ef38ec5694c279fc8a04550dca5","source":{"kind":"arxiv","id":"1706.04871","version":3},"attestation_state":"computed","paper":{"title":"ALMA observations of N83C in the early stage of star formation in the Small Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akiko Kawamura, Alberto D. Bolatto, Aya Homma, Erik Muller, Kazuki Tokuda, Kazuya Saigo, Kazuyuki Muraoka, Margaret Meixner, Marta Sewi{\\l}o, Norikazu Mizuno, Remy Indebetouw, Ryohei Harada, Sarolta Zahorecz, Tetsuhiro Minamidani, Toshikazu Onishi, Yasuo Fukui, Yuuki Morioka","submitted_at":"2017-06-15T13:58:19Z","abstract_excerpt":"We have performed Atacama Large Millimeter/submillimeter Array (ALMA) observations in $^{12}$CO($J=2-1$), $^{13}$CO($J=2-1$), C$^{18}$O($J=2-1$), $^{12}$CO($J=3-2$), $^{13}$CO($J=3-2$), and CS($J=7-6$) lines toward the active star-forming region N83C in the Small Magellanic Cloud (SMC), whose metallicity is $\\sim$ 1/5 of the Milky Way (MW). The ALMA observations first reveal sub-pc scale molecular structures in $^{12}$CO($J=2-1$) and $^{13}$CO($J=2-1$) emission. We found strong CO peaks associated with young stellar objects (YSOs) identified by the $Spitzer$ Space Telescope, and also found tha"},"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":"1706.04871","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-15T13:58:19Z","cross_cats_sorted":[],"title_canon_sha256":"54153f2307a95ec4e8f5baa75ecf391172b00ca5217709f9269af44d9efae17b","abstract_canon_sha256":"cc5d19801f2497ed666a93e13349bcf55cbb14d35326c49f147bfa8a1e7df890"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:50.996882Z","signature_b64":"1JzN/nKsPoz7XAhPXuJPFAueBTKo7T+DNc9Rnr04xEj+ruBj4gyGvmX0Eqlj0enSnqsQH+iapZL9ESLagLwNBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d2bf15e51ac00420ebdb9810b350aa5208586ef38ec5694c279fc8a04550dca5","last_reissued_at":"2026-05-18T00:38:50.996161Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:50.996161Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA observations of N83C in the early stage of star formation in the Small Magellanic Cloud","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Akiko Kawamura, Alberto D. Bolatto, Aya Homma, Erik Muller, Kazuki Tokuda, Kazuya Saigo, Kazuyuki Muraoka, Margaret Meixner, Marta Sewi{\\l}o, Norikazu Mizuno, Remy Indebetouw, Ryohei Harada, Sarolta Zahorecz, Tetsuhiro Minamidani, Toshikazu Onishi, Yasuo Fukui, Yuuki Morioka","submitted_at":"2017-06-15T13:58:19Z","abstract_excerpt":"We have performed Atacama Large Millimeter/submillimeter Array (ALMA) observations in $^{12}$CO($J=2-1$), $^{13}$CO($J=2-1$), C$^{18}$O($J=2-1$), $^{12}$CO($J=3-2$), $^{13}$CO($J=3-2$), and CS($J=7-6$) lines toward the active star-forming region N83C in the Small Magellanic Cloud (SMC), whose metallicity is $\\sim$ 1/5 of the Milky Way (MW). The ALMA observations first reveal sub-pc scale molecular structures in $^{12}$CO($J=2-1$) and $^{13}$CO($J=2-1$) emission. We found strong CO peaks associated with young stellar objects (YSOs) identified by the $Spitzer$ Space Telescope, and also found tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.04871","kind":"arxiv","version":3},"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":"1706.04871","created_at":"2026-05-18T00:38:50.996264+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.04871v3","created_at":"2026-05-18T00:38:50.996264+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.04871","created_at":"2026-05-18T00:38:50.996264+00:00"},{"alias_kind":"pith_short_12","alias_value":"2K7RLZI2YACC","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_16","alias_value":"2K7RLZI2YACCB263","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_8","alias_value":"2K7RLZI2","created_at":"2026-05-18T12:30:55.937587+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/2K7RLZI2YACCB263TAILGUFKKI","json":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI.json","graph_json":"https://pith.science/api/pith-number/2K7RLZI2YACCB263TAILGUFKKI/graph.json","events_json":"https://pith.science/api/pith-number/2K7RLZI2YACCB263TAILGUFKKI/events.json","paper":"https://pith.science/paper/2K7RLZI2"},"agent_actions":{"view_html":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI","download_json":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI.json","view_paper":"https://pith.science/paper/2K7RLZI2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.04871&json=true","fetch_graph":"https://pith.science/api/pith-number/2K7RLZI2YACCB263TAILGUFKKI/graph.json","fetch_events":"https://pith.science/api/pith-number/2K7RLZI2YACCB263TAILGUFKKI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI/action/storage_attestation","attest_author":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI/action/author_attestation","sign_citation":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI/action/citation_signature","submit_replication":"https://pith.science/pith/2K7RLZI2YACCB263TAILGUFKKI/action/replication_record"}},"created_at":"2026-05-18T00:38:50.996264+00:00","updated_at":"2026-05-18T00:38:50.996264+00:00"}