{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:XXPJXXOVGMZPYMFATTMSZRUTCT","short_pith_number":"pith:XXPJXXOV","schema_version":"1.0","canonical_sha256":"bdde9bddd53332fc30a09cd92cc69314d405b6dd14e873ebc0ac2374e4e977fa","source":{"kind":"arxiv","id":"1307.6224","version":1},"attestation_state":"computed","paper":{"title":"Diagnostics of AGN-driven Molecular Outflows in ULIRGs from Herschel-PACS Observations of OH at 119um","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Efstathiou, A. Verma, C. Borys, C. Pearson, D. Cormier, D. Farrah, D.L. Clements, D. Rigopoulou, E. Gonzalez-Alfonso, H.A. Smith, H.W.W. Spoon, J. Afonso, J. Bernard-Salas, M. Etxaluze, M.S. Westmoquette, T. Urrutia, V. Lebouteiller","submitted_at":"2013-07-23T20:03:27Z","abstract_excerpt":"We report on our observations of the 79 and 119um doublet transitions of OH for 24 local (z<0.262) ULIRGs observed with Herschel-PACS as part of the Herschel ULIRG Survey (HERUS). Some OH119 profiles display a clear P-Cygni shape and therefore imply outflowing OH gas, other profiles are predominantly in absorption or are completely in emission. We find that the relative strength of the OH emission component decreases as the silicate absorption increases. This locates the OH outflows inside the obscured nuclei. The maximum outflow velocities for our sources range from less than 100 to 2000 km/s"},"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":"1307.6224","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-23T20:03:27Z","cross_cats_sorted":[],"title_canon_sha256":"e9d2748fb2d9fc677ea082a0d874a82a04dc12c702cac00c4cce1334ce64ac4f","abstract_canon_sha256":"117353818671c47664d2593d77bf617b508ae269bc0d9195bc45d0d92d8b5f0c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:40.930218Z","signature_b64":"kL5y2ASbXkOBF98scAp1yFYdFV0G0SpzWRvpC2yKx4qJGwib1q4/eymUePlEn5Tuh6v4Mm39qOcHwDgFopqzAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bdde9bddd53332fc30a09cd92cc69314d405b6dd14e873ebc0ac2374e4e977fa","last_reissued_at":"2026-05-18T01:48:40.929535Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:40.929535Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Diagnostics of AGN-driven Molecular Outflows in ULIRGs from Herschel-PACS Observations of OH at 119um","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Efstathiou, A. Verma, C. Borys, C. Pearson, D. Cormier, D. Farrah, D.L. Clements, D. Rigopoulou, E. Gonzalez-Alfonso, H.A. Smith, H.W.W. Spoon, J. Afonso, J. Bernard-Salas, M. Etxaluze, M.S. Westmoquette, T. Urrutia, V. Lebouteiller","submitted_at":"2013-07-23T20:03:27Z","abstract_excerpt":"We report on our observations of the 79 and 119um doublet transitions of OH for 24 local (z<0.262) ULIRGs observed with Herschel-PACS as part of the Herschel ULIRG Survey (HERUS). Some OH119 profiles display a clear P-Cygni shape and therefore imply outflowing OH gas, other profiles are predominantly in absorption or are completely in emission. We find that the relative strength of the OH emission component decreases as the silicate absorption increases. This locates the OH outflows inside the obscured nuclei. The maximum outflow velocities for our sources range from less than 100 to 2000 km/s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.6224","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":"1307.6224","created_at":"2026-05-18T01:48:40.929657+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.6224v1","created_at":"2026-05-18T01:48:40.929657+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.6224","created_at":"2026-05-18T01:48:40.929657+00:00"},{"alias_kind":"pith_short_12","alias_value":"XXPJXXOVGMZP","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"XXPJXXOVGMZPYMFA","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"XXPJXXOV","created_at":"2026-05-18T12:28:06.772260+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/XXPJXXOVGMZPYMFATTMSZRUTCT","json":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT.json","graph_json":"https://pith.science/api/pith-number/XXPJXXOVGMZPYMFATTMSZRUTCT/graph.json","events_json":"https://pith.science/api/pith-number/XXPJXXOVGMZPYMFATTMSZRUTCT/events.json","paper":"https://pith.science/paper/XXPJXXOV"},"agent_actions":{"view_html":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT","download_json":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT.json","view_paper":"https://pith.science/paper/XXPJXXOV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.6224&json=true","fetch_graph":"https://pith.science/api/pith-number/XXPJXXOVGMZPYMFATTMSZRUTCT/graph.json","fetch_events":"https://pith.science/api/pith-number/XXPJXXOVGMZPYMFATTMSZRUTCT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT/action/storage_attestation","attest_author":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT/action/author_attestation","sign_citation":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT/action/citation_signature","submit_replication":"https://pith.science/pith/XXPJXXOVGMZPYMFATTMSZRUTCT/action/replication_record"}},"created_at":"2026-05-18T01:48:40.929657+00:00","updated_at":"2026-05-18T01:48:40.929657+00:00"}