{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:G2B3A2B6Y6OB53K6QBPDSTIL7A","short_pith_number":"pith:G2B3A2B6","schema_version":"1.0","canonical_sha256":"3683b0683ec79c1eed5e805e394d0bf8375da422b467d55ced573987a6673a9a","source":{"kind":"arxiv","id":"1005.1511","version":2},"attestation_state":"computed","paper":{"title":"Herschel-PACS spectroscopy of IR-bright galaxies at high redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Contursi, A. Poglitsch, A. Sternberg, A. Verma, D. Lutz, E. Gonz\\'alez-Alfonso, E. Sturm, J. de Jong, J. Fischer, J. Graci\\'a-Carpio, L. Tacconi, N. Christopher, R. Genzel, S. Hailey-Dunsheath","submitted_at":"2010-05-10T12:07:07Z","abstract_excerpt":"We present Herschel-PACS observations of rest-frame mid-infrared and far-infrared spectral line emissions from two lensed, ultra-luminous infrared galaxies at high redshift: MIPS J142824.0+352619 (MIPS J1428), a starburst-dominated system at z = 1.3, and IRAS F10214+4724 (F10214), a source at z = 2.3 hosting both star-formation and a luminous AGN. We have detected [OI]63 micron and [OIII]52 micron in MIPS J1428, and tentatively [OIII]52 micron in F10214. Together with the recent ZEUS-CSO [CII]158 micron detection in MIPS J1428 we can for the first time combine [OI], [CII] and far-IR (FIR) cont"},"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":"1005.1511","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-05-10T12:07:07Z","cross_cats_sorted":[],"title_canon_sha256":"787ec7a2fdb1f38e61ccf8a840ce9b57c25794df309c08a9aec5f6d7cf4d468d","abstract_canon_sha256":"b940819a6e4191434e3f71ef9747aee0aca9239e59416b6328de98984ea37d7c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:34.877458Z","signature_b64":"a6mz2ld3kAPsPAqwCl0gu20n0Q9nsW4+0LnR6krZpdfMCZy8UATUIJyV9mbaBkGYfnMpP7ZACA/nq7NIexB8Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3683b0683ec79c1eed5e805e394d0bf8375da422b467d55ced573987a6673a9a","last_reissued_at":"2026-05-18T02:07:34.876908Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:34.876908Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel-PACS spectroscopy of IR-bright galaxies at high redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Contursi, A. Poglitsch, A. Sternberg, A. Verma, D. Lutz, E. Gonz\\'alez-Alfonso, E. Sturm, J. de Jong, J. Fischer, J. Graci\\'a-Carpio, L. Tacconi, N. Christopher, R. Genzel, S. Hailey-Dunsheath","submitted_at":"2010-05-10T12:07:07Z","abstract_excerpt":"We present Herschel-PACS observations of rest-frame mid-infrared and far-infrared spectral line emissions from two lensed, ultra-luminous infrared galaxies at high redshift: MIPS J142824.0+352619 (MIPS J1428), a starburst-dominated system at z = 1.3, and IRAS F10214+4724 (F10214), a source at z = 2.3 hosting both star-formation and a luminous AGN. We have detected [OI]63 micron and [OIII]52 micron in MIPS J1428, and tentatively [OIII]52 micron in F10214. Together with the recent ZEUS-CSO [CII]158 micron detection in MIPS J1428 we can for the first time combine [OI], [CII] and far-IR (FIR) cont"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1511","kind":"arxiv","version":2},"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":"1005.1511","created_at":"2026-05-18T02:07:34.876966+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1511v2","created_at":"2026-05-18T02:07:34.876966+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1511","created_at":"2026-05-18T02:07:34.876966+00:00"},{"alias_kind":"pith_short_12","alias_value":"G2B3A2B6Y6OB","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"G2B3A2B6Y6OB53K6","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"G2B3A2B6","created_at":"2026-05-18T12:26:07.630475+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/G2B3A2B6Y6OB53K6QBPDSTIL7A","json":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A.json","graph_json":"https://pith.science/api/pith-number/G2B3A2B6Y6OB53K6QBPDSTIL7A/graph.json","events_json":"https://pith.science/api/pith-number/G2B3A2B6Y6OB53K6QBPDSTIL7A/events.json","paper":"https://pith.science/paper/G2B3A2B6"},"agent_actions":{"view_html":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A","download_json":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A.json","view_paper":"https://pith.science/paper/G2B3A2B6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1511&json=true","fetch_graph":"https://pith.science/api/pith-number/G2B3A2B6Y6OB53K6QBPDSTIL7A/graph.json","fetch_events":"https://pith.science/api/pith-number/G2B3A2B6Y6OB53K6QBPDSTIL7A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A/action/storage_attestation","attest_author":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A/action/author_attestation","sign_citation":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A/action/citation_signature","submit_replication":"https://pith.science/pith/G2B3A2B6Y6OB53K6QBPDSTIL7A/action/replication_record"}},"created_at":"2026-05-18T02:07:34.876966+00:00","updated_at":"2026-05-18T02:07:34.876966+00:00"}