{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:5KXON6UYLWEFWPT7455HUEIR57","short_pith_number":"pith:5KXON6UY","schema_version":"1.0","canonical_sha256":"eaaee6fa985d885b3e7fe77a7a1111efdeddff822b229c59067e736122e1b9dd","source":{"kind":"arxiv","id":"1005.3409","version":3},"attestation_state":"computed","paper":{"title":"Star Forming Dense Cloud Cores in the TeV {\\gamma}-ray SNR RX J1713.7-3946","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Kawamura, A. Mizuno, A. O. Benz, B. -C. Koo, F. Bertoldi, H. Horachi, H. Maezawa, H. Matsumoto, H. Ogawa, H. Sano, H. Yamamoto, J. Sato, J. Stutzki, K. Torii, L. Bronfman, M. G. Burton, N. Mizuno, N. Moribe, S. Anderl, S. Inutsuka, T. Hayakawa, T. Inoue, T. Okuda, T. Onishi, T. Tanaka, Y. Fukui","submitted_at":"2010-05-19T10:48:31Z","abstract_excerpt":"RX J1713.7-3946 is one of the TeV {\\gamma}-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular observations toward the dense cloud cores, peaks A, C and D, in the SNR in the 12CO(J=2-1) and 13CO(J=2-1) transitions at angular resolution of 90\". The most intense core in 13CO, peak C, was also mapped in the 12CO(J=4-3) transition at angular resolution of 38\". Peak C shows strong signs of active star formation including bipolar outflow and a far-infrared protostellar source and has a steep gradient with a r^{-"},"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":"1005.3409","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-05-19T10:48:31Z","cross_cats_sorted":[],"title_canon_sha256":"1a747f0e7726383b06c5021317856488bebe3e45366542c1d009fadb7d1d034b","abstract_canon_sha256":"2ba500ddfb51a2fc6a190771bf8041d1fa7bff7d8b65827e5ffd5b6fee6d2b05"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:17.014915Z","signature_b64":"NwVLfrcgvAtVXehYsQzJP0aernsstvRU2LXdsfwz28kBMmdcRCPCqag3JMIJsx01j1nwxje7THO5hcu8lARQDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eaaee6fa985d885b3e7fe77a7a1111efdeddff822b229c59067e736122e1b9dd","last_reissued_at":"2026-05-18T02:07:17.013594Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:17.013594Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star Forming Dense Cloud Cores in the TeV {\\gamma}-ray SNR RX J1713.7-3946","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Kawamura, A. Mizuno, A. O. Benz, B. -C. Koo, F. Bertoldi, H. Horachi, H. Maezawa, H. Matsumoto, H. Ogawa, H. Sano, H. Yamamoto, J. Sato, J. Stutzki, K. Torii, L. Bronfman, M. G. Burton, N. Mizuno, N. Moribe, S. Anderl, S. Inutsuka, T. Hayakawa, T. Inoue, T. Okuda, T. Onishi, T. Tanaka, Y. Fukui","submitted_at":"2010-05-19T10:48:31Z","abstract_excerpt":"RX J1713.7-3946 is one of the TeV {\\gamma}-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular observations toward the dense cloud cores, peaks A, C and D, in the SNR in the 12CO(J=2-1) and 13CO(J=2-1) transitions at angular resolution of 90\". The most intense core in 13CO, peak C, was also mapped in the 12CO(J=4-3) transition at angular resolution of 38\". Peak C shows strong signs of active star formation including bipolar outflow and a far-infrared protostellar source and has a steep gradient with a r^{-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.3409","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":"1005.3409","created_at":"2026-05-18T02:07:17.014169+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.3409v3","created_at":"2026-05-18T02:07:17.014169+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.3409","created_at":"2026-05-18T02:07:17.014169+00:00"},{"alias_kind":"pith_short_12","alias_value":"5KXON6UYLWEF","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"5KXON6UYLWEFWPT7","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"5KXON6UY","created_at":"2026-05-18T12:26:04.259169+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/5KXON6UYLWEFWPT7455HUEIR57","json":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57.json","graph_json":"https://pith.science/api/pith-number/5KXON6UYLWEFWPT7455HUEIR57/graph.json","events_json":"https://pith.science/api/pith-number/5KXON6UYLWEFWPT7455HUEIR57/events.json","paper":"https://pith.science/paper/5KXON6UY"},"agent_actions":{"view_html":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57","download_json":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57.json","view_paper":"https://pith.science/paper/5KXON6UY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.3409&json=true","fetch_graph":"https://pith.science/api/pith-number/5KXON6UYLWEFWPT7455HUEIR57/graph.json","fetch_events":"https://pith.science/api/pith-number/5KXON6UYLWEFWPT7455HUEIR57/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57/action/storage_attestation","attest_author":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57/action/author_attestation","sign_citation":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57/action/citation_signature","submit_replication":"https://pith.science/pith/5KXON6UYLWEFWPT7455HUEIR57/action/replication_record"}},"created_at":"2026-05-18T02:07:17.014169+00:00","updated_at":"2026-05-18T02:07:17.014169+00:00"}