{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:JOFCN4CYEZU3GJG7MVJ5EIDJC7","short_pith_number":"pith:JOFCN4CY","schema_version":"1.0","canonical_sha256":"4b8a26f0582669b324df6553d2206917fa9cfd13aa38483a536396e4f4448c9c","source":{"kind":"arxiv","id":"1209.0670","version":1},"attestation_state":"computed","paper":{"title":"Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Cooray, A. Dariush, C. Hoyos, D. J. B. Smith, D. L. Clements, E. Ibar, E. Valiante, G. de Zotti, J. A. Stevens, J. M. Cao Orjales, K. Coppin, L. Dunne, M. Baes, M. J. Hardcastle, M. J. Jarvis, M. J. Page, R. Auld, R. Hopwood, R. J. Ivison, S. Dye, S. Eales, S. Maddox","submitted_at":"2012-09-04T15:25:59Z","abstract_excerpt":"We have used data from the Herschel-ATLAS at 250, 350 and 500 \\mu m to determine the far-infrared (FIR) properties of 50 Broad Absorption Line Quasars (BAL QSOs). Our sample contains 49 high-ionization BAL QSOs (HiBALs) and 1 low-ionization BAL QSO (LoBAL) which are compared against a sample of 329 non-BAL QSOs. These samples are matched over the redshift range 1.5 \\leq z < 2.3 and in absolute i-band magnitude over the range -28 \\leq M_{i} \\leq -24. Of these, 3 BAL QSOs (HiBALs) and 27 non-BAL QSOs are detected at the > 5 sigma level. We calculate star-formation rates (SFR) for our individuall"},"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":"1209.0670","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-09-04T15:25:59Z","cross_cats_sorted":[],"title_canon_sha256":"85ec873e3e65d015d01d35a33b1c2a32a49f93fade6ebb00476cc516d7534dd8","abstract_canon_sha256":"7f7046e8c5e6ad04c946bf4158ad033a2a531274f2df06f8b6d4d8979e252662"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:40.804676Z","signature_b64":"eEOJaLabAhMsmAKy/ucaCrXzPeTdH5QvUAPkFeA3B1MKO1b25+11n0btlWrz4Z0sMXCKfVDcMnUv7g/0QmDFBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4b8a26f0582669b324df6553d2206917fa9cfd13aa38483a536396e4f4448c9c","last_reissued_at":"2026-05-18T01:54:40.803861Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:40.803861Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Cava, A. Cooray, A. Dariush, C. Hoyos, D. J. B. Smith, D. L. Clements, E. Ibar, E. Valiante, G. de Zotti, J. A. Stevens, J. M. Cao Orjales, K. Coppin, L. Dunne, M. Baes, M. J. Hardcastle, M. J. Jarvis, M. J. Page, R. Auld, R. Hopwood, R. J. Ivison, S. Dye, S. Eales, S. Maddox","submitted_at":"2012-09-04T15:25:59Z","abstract_excerpt":"We have used data from the Herschel-ATLAS at 250, 350 and 500 \\mu m to determine the far-infrared (FIR) properties of 50 Broad Absorption Line Quasars (BAL QSOs). Our sample contains 49 high-ionization BAL QSOs (HiBALs) and 1 low-ionization BAL QSO (LoBAL) which are compared against a sample of 329 non-BAL QSOs. These samples are matched over the redshift range 1.5 \\leq z < 2.3 and in absolute i-band magnitude over the range -28 \\leq M_{i} \\leq -24. Of these, 3 BAL QSOs (HiBALs) and 27 non-BAL QSOs are detected at the > 5 sigma level. We calculate star-formation rates (SFR) for our individuall"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.0670","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":"1209.0670","created_at":"2026-05-18T01:54:40.803992+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.0670v1","created_at":"2026-05-18T01:54:40.803992+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.0670","created_at":"2026-05-18T01:54:40.803992+00:00"},{"alias_kind":"pith_short_12","alias_value":"JOFCN4CYEZU3","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"JOFCN4CYEZU3GJG7","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"JOFCN4CY","created_at":"2026-05-18T12:27:11.947152+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/JOFCN4CYEZU3GJG7MVJ5EIDJC7","json":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7.json","graph_json":"https://pith.science/api/pith-number/JOFCN4CYEZU3GJG7MVJ5EIDJC7/graph.json","events_json":"https://pith.science/api/pith-number/JOFCN4CYEZU3GJG7MVJ5EIDJC7/events.json","paper":"https://pith.science/paper/JOFCN4CY"},"agent_actions":{"view_html":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7","download_json":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7.json","view_paper":"https://pith.science/paper/JOFCN4CY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.0670&json=true","fetch_graph":"https://pith.science/api/pith-number/JOFCN4CYEZU3GJG7MVJ5EIDJC7/graph.json","fetch_events":"https://pith.science/api/pith-number/JOFCN4CYEZU3GJG7MVJ5EIDJC7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7/action/storage_attestation","attest_author":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7/action/author_attestation","sign_citation":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7/action/citation_signature","submit_replication":"https://pith.science/pith/JOFCN4CYEZU3GJG7MVJ5EIDJC7/action/replication_record"}},"created_at":"2026-05-18T01:54:40.803992+00:00","updated_at":"2026-05-18T01:54:40.803992+00:00"}