{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:AMWMKAO7DWHQPH6UYHWBVZKMML","short_pith_number":"pith:AMWMKAO7","schema_version":"1.0","canonical_sha256":"032cc501df1d8f079fd4c1ec1ae54c62d50f423ff1f84cbd6d822ecebae04ad5","source":{"kind":"arxiv","id":"1007.4226","version":1},"attestation_state":"computed","paper":{"title":"The distribution of water in the high-mass star-forming region NGC 6334I","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bacmann, A. Baudry, A. Boogert, A. Castets, A. Coutens, A. Fuente, A. Klotz, A. Loose, A. Lorenzani, A. Walters, B. Lefloch, B. Nisini, B. Parise, C. Ceccarelli, C. Codella, C. Comito, C. Dominik, C. Kahane, C. Risacher, C. Vastel, D. C. Lis, D. Neufeld, E.A. Bergin, E. Caux, E. Falgarone, E. Herbst, F. Helmich, F. van der Tak, F. Wyrowski, G. Blake, G. Melnick, H. Aarts, H. Yorke, J. Cernicharo, J. Kooi, J. Pearson, J. Stutzki, K. Demyk, K. Schuster, L. Pagani, M. Benedettini, M. Emprechtinger, M. Gerin, M. Kama, M. Salez, M. van der Wiel, N. Crimier, P. Caselli, P. Encrenaz, P. Goldsmith, P. Hennebelle, P. Hily-Blant, P. Saraceno, P. Schilke, R. Rolffs, S. Bottinelli, S. Cabrit, S. Lord, S. Maret, S. Pacheco, S. Viti, T. Bell, T. G. Phillips, T. Henning, T. Jacq, V. Ossenkopf, V. Wakelam, W. Langer, X. Tielens","submitted_at":"2010-07-23T22:24:34Z","abstract_excerpt":"We present observations of twelve rotational transitions of H2O-16, H2O-18, and H2O-17 toward the massive star-forming region NGC 6334 I, carried out with Herschel/HIFI as part of the guaranteed time key program Chemical HErschel Surveys of Star forming regions (CHESS). We analyze these observations to obtain insights into physical processes in this region.\n  We identify three main gas components (hot core, cold foreground, and outflow) in NGC 6334 I and derive the physical conditions in these components.\n  The hot core, identified by the emission in highly excited lines, shows a high excitati"},"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":"1007.4226","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-07-23T22:24:34Z","cross_cats_sorted":[],"title_canon_sha256":"22423416884d82e29e5fd1c4c08d65422d3df9b95d906060dab64260cba6ac4f","abstract_canon_sha256":"deae9d73cf10744d6ddf8ef4558a6f32317cf559b8dd2c32c51657cb8874dcd9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:10.867407Z","signature_b64":"W4G3SW4Z+gOWAzLoCmbmLKsyvA/MWkxPZCFzSAQSmDwQqpl80q//yHOV5vSBdWk7eh9woAY0b67nPDg+cOgDCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"032cc501df1d8f079fd4c1ec1ae54c62d50f423ff1f84cbd6d822ecebae04ad5","last_reissued_at":"2026-05-18T02:06:10.866831Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:10.866831Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The distribution of water in the high-mass star-forming region NGC 6334I","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bacmann, A. Baudry, A. Boogert, A. Castets, A. Coutens, A. Fuente, A. Klotz, A. Loose, A. Lorenzani, A. Walters, B. Lefloch, B. Nisini, B. Parise, C. Ceccarelli, C. Codella, C. Comito, C. Dominik, C. Kahane, C. Risacher, C. Vastel, D. C. Lis, D. Neufeld, E.A. Bergin, E. Caux, E. Falgarone, E. Herbst, F. Helmich, F. van der Tak, F. Wyrowski, G. Blake, G. Melnick, H. Aarts, H. Yorke, J. Cernicharo, J. Kooi, J. Pearson, J. Stutzki, K. Demyk, K. Schuster, L. Pagani, M. Benedettini, M. Emprechtinger, M. Gerin, M. Kama, M. Salez, M. van der Wiel, N. Crimier, P. Caselli, P. Encrenaz, P. Goldsmith, P. Hennebelle, P. Hily-Blant, P. Saraceno, P. Schilke, R. Rolffs, S. Bottinelli, S. Cabrit, S. Lord, S. Maret, S. Pacheco, S. Viti, T. Bell, T. G. Phillips, T. Henning, T. Jacq, V. Ossenkopf, V. Wakelam, W. Langer, X. Tielens","submitted_at":"2010-07-23T22:24:34Z","abstract_excerpt":"We present observations of twelve rotational transitions of H2O-16, H2O-18, and H2O-17 toward the massive star-forming region NGC 6334 I, carried out with Herschel/HIFI as part of the guaranteed time key program Chemical HErschel Surveys of Star forming regions (CHESS). We analyze these observations to obtain insights into physical processes in this region.\n  We identify three main gas components (hot core, cold foreground, and outflow) in NGC 6334 I and derive the physical conditions in these components.\n  The hot core, identified by the emission in highly excited lines, shows a high excitati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.4226","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":""},"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":"1007.4226","created_at":"2026-05-18T02:06:10.866925+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.4226v1","created_at":"2026-05-18T02:06:10.866925+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.4226","created_at":"2026-05-18T02:06:10.866925+00:00"},{"alias_kind":"pith_short_12","alias_value":"AMWMKAO7DWHQ","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"AMWMKAO7DWHQPH6U","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"AMWMKAO7","created_at":"2026-05-18T12:26:05.355336+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/AMWMKAO7DWHQPH6UYHWBVZKMML","json":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML.json","graph_json":"https://pith.science/api/pith-number/AMWMKAO7DWHQPH6UYHWBVZKMML/graph.json","events_json":"https://pith.science/api/pith-number/AMWMKAO7DWHQPH6UYHWBVZKMML/events.json","paper":"https://pith.science/paper/AMWMKAO7"},"agent_actions":{"view_html":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML","download_json":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML.json","view_paper":"https://pith.science/paper/AMWMKAO7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.4226&json=true","fetch_graph":"https://pith.science/api/pith-number/AMWMKAO7DWHQPH6UYHWBVZKMML/graph.json","fetch_events":"https://pith.science/api/pith-number/AMWMKAO7DWHQPH6UYHWBVZKMML/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML/action/storage_attestation","attest_author":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML/action/author_attestation","sign_citation":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML/action/citation_signature","submit_replication":"https://pith.science/pith/AMWMKAO7DWHQPH6UYHWBVZKMML/action/replication_record"}},"created_at":"2026-05-18T02:06:10.866925+00:00","updated_at":"2026-05-18T02:06:10.866925+00:00"}