{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:BWQR5DZYI32HEWU6GRCUR5NDWY","short_pith_number":"pith:BWQR5DZY","schema_version":"1.0","canonical_sha256":"0da11e8f3846f4725a9e344548f5a3b60ab21612b8cdf78f64004c22b5088bf3","source":{"kind":"arxiv","id":"1204.0397","version":1},"attestation_state":"computed","paper":{"title":"The massive protostar W43-MM1 as seen by Herschel-HIFI water spectra: high turbulence and accretion luminosity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Baudry, E. F. van Dishoeck, F. Herpin, F. van der Tak, F. Wyrowski, J. Braine, L. Chavarria, L. Kristensen, S. Bontemps, T. Jacq","submitted_at":"2012-04-02T13:03:16Z","abstract_excerpt":"We present Herschel/HIFI observations of fourteen water lines in W43-MM1, a massive protostellar object in the luminous star cluster-forming region W43. We analyze the gas dynamics from the line profiles using Herschel-HIFI observations (WISH-KP) of fourteen far-IR water lines (H2O, H217O, H218O), CS(11-10), and C18O(9-8) lines, and using our modeling of the continuum spectral energy distribution. As for lower mass protostellar objects, the molecular line profiles are a mix of emission and absorption, and can be decomposed into 'medium', and 'broad' velocity components. The broad component is "},"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":"1204.0397","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-04-02T13:03:16Z","cross_cats_sorted":[],"title_canon_sha256":"2284b35b2545e1c0b53033da85fe0a94535e69194c0b36932329d3f6d229ef2a","abstract_canon_sha256":"56c2e1cd19852436004b3ca705726935b154d8b004e03889eec7f1049e33b340"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:58.131029Z","signature_b64":"6M8eFzfNNGch1eJOf+wnS/ycn1oB8xonnjmfQ6Hg6wGuC3MRgrME9k4z7nG3CI1rgjlQpqlgQxqN20F5zCGoDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0da11e8f3846f4725a9e344548f5a3b60ab21612b8cdf78f64004c22b5088bf3","last_reissued_at":"2026-05-18T01:57:58.130532Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:58.130532Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The massive protostar W43-MM1 as seen by Herschel-HIFI water spectra: high turbulence and accretion luminosity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Baudry, E. F. van Dishoeck, F. Herpin, F. van der Tak, F. Wyrowski, J. Braine, L. Chavarria, L. Kristensen, S. Bontemps, T. Jacq","submitted_at":"2012-04-02T13:03:16Z","abstract_excerpt":"We present Herschel/HIFI observations of fourteen water lines in W43-MM1, a massive protostellar object in the luminous star cluster-forming region W43. We analyze the gas dynamics from the line profiles using Herschel-HIFI observations (WISH-KP) of fourteen far-IR water lines (H2O, H217O, H218O), CS(11-10), and C18O(9-8) lines, and using our modeling of the continuum spectral energy distribution. As for lower mass protostellar objects, the molecular line profiles are a mix of emission and absorption, and can be decomposed into 'medium', and 'broad' velocity components. The broad component is "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.0397","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":"1204.0397","created_at":"2026-05-18T01:57:58.130615+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.0397v1","created_at":"2026-05-18T01:57:58.130615+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.0397","created_at":"2026-05-18T01:57:58.130615+00:00"},{"alias_kind":"pith_short_12","alias_value":"BWQR5DZYI32H","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_16","alias_value":"BWQR5DZYI32HEWU6","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_8","alias_value":"BWQR5DZY","created_at":"2026-05-18T12:27:01.376967+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/BWQR5DZYI32HEWU6GRCUR5NDWY","json":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY.json","graph_json":"https://pith.science/api/pith-number/BWQR5DZYI32HEWU6GRCUR5NDWY/graph.json","events_json":"https://pith.science/api/pith-number/BWQR5DZYI32HEWU6GRCUR5NDWY/events.json","paper":"https://pith.science/paper/BWQR5DZY"},"agent_actions":{"view_html":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY","download_json":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY.json","view_paper":"https://pith.science/paper/BWQR5DZY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.0397&json=true","fetch_graph":"https://pith.science/api/pith-number/BWQR5DZYI32HEWU6GRCUR5NDWY/graph.json","fetch_events":"https://pith.science/api/pith-number/BWQR5DZYI32HEWU6GRCUR5NDWY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY/action/storage_attestation","attest_author":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY/action/author_attestation","sign_citation":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY/action/citation_signature","submit_replication":"https://pith.science/pith/BWQR5DZYI32HEWU6GRCUR5NDWY/action/replication_record"}},"created_at":"2026-05-18T01:57:58.130615+00:00","updated_at":"2026-05-18T01:57:58.130615+00:00"}