{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:IOCFWY275443WMDOP3UKRCVTB3","short_pith_number":"pith:IOCFWY27","schema_version":"1.0","canonical_sha256":"43845b635fef39bb306e7ee8a88ab30ef4607544a668414b9154995df3017cca","source":{"kind":"arxiv","id":"1305.1881","version":1},"attestation_state":"computed","paper":{"title":"AGN in dusty hosts: implications for galaxy evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bongiorno, A. van der Wel, D. Sanders, J. Kartaltepe, M. Brusa, M. J. Page, M. Salvato, Myrto Symeonidis, O. Ilbert","submitted_at":"2013-05-08T16:51:41Z","abstract_excerpt":"We present strong empirical evidence for a physical connection between the occurrence of a starburst (SB) and a luminous AGN phase. Drawing infrared (IR), X-ray, and optically selected samples from COSMOS, we find that the locus of type-2 AGN hosts in the optical colour-magnitude (U-V/V) and colour-colour (U-V/V-J) space significantly overlaps with that of IR-luminous (L_IR > 10^10 L_sun) galaxies. Based on our observations, we propose that, when simultaneously building their black hole and stellar masses, type-2 AGN hosts are located in the same part of colour-colour space as dusty star-formi"},"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":"1305.1881","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-05-08T16:51:41Z","cross_cats_sorted":[],"title_canon_sha256":"b6d4c6ca29fe4787a10198cc84f2352b9e7b97a1f84cb69465f7e292e2487a87","abstract_canon_sha256":"c6c7117f1ab13ac9c371fa7b05e376135051e99dbb9420f4f4f5fcc72a522d9e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:04.666217Z","signature_b64":"L/VLl0aN0uDl1pgftCZVm0tICWrRpDCciXLbYRPbJHa3OEHjrC5OlhE/O3EPLvY5iiWuDblCABrNTxLbprLtDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"43845b635fef39bb306e7ee8a88ab30ef4607544a668414b9154995df3017cca","last_reissued_at":"2026-05-18T01:50:04.665573Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:04.665573Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"AGN in dusty hosts: implications for galaxy evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bongiorno, A. van der Wel, D. Sanders, J. Kartaltepe, M. Brusa, M. J. Page, M. Salvato, Myrto Symeonidis, O. Ilbert","submitted_at":"2013-05-08T16:51:41Z","abstract_excerpt":"We present strong empirical evidence for a physical connection between the occurrence of a starburst (SB) and a luminous AGN phase. Drawing infrared (IR), X-ray, and optically selected samples from COSMOS, we find that the locus of type-2 AGN hosts in the optical colour-magnitude (U-V/V) and colour-colour (U-V/V-J) space significantly overlaps with that of IR-luminous (L_IR > 10^10 L_sun) galaxies. Based on our observations, we propose that, when simultaneously building their black hole and stellar masses, type-2 AGN hosts are located in the same part of colour-colour space as dusty star-formi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.1881","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":"1305.1881","created_at":"2026-05-18T01:50:04.665683+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.1881v1","created_at":"2026-05-18T01:50:04.665683+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.1881","created_at":"2026-05-18T01:50:04.665683+00:00"},{"alias_kind":"pith_short_12","alias_value":"IOCFWY275443","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"IOCFWY275443WMDO","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"IOCFWY27","created_at":"2026-05-18T12:27:46.883200+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/IOCFWY275443WMDOP3UKRCVTB3","json":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3.json","graph_json":"https://pith.science/api/pith-number/IOCFWY275443WMDOP3UKRCVTB3/graph.json","events_json":"https://pith.science/api/pith-number/IOCFWY275443WMDOP3UKRCVTB3/events.json","paper":"https://pith.science/paper/IOCFWY27"},"agent_actions":{"view_html":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3","download_json":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3.json","view_paper":"https://pith.science/paper/IOCFWY27","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.1881&json=true","fetch_graph":"https://pith.science/api/pith-number/IOCFWY275443WMDOP3UKRCVTB3/graph.json","fetch_events":"https://pith.science/api/pith-number/IOCFWY275443WMDOP3UKRCVTB3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3/action/storage_attestation","attest_author":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3/action/author_attestation","sign_citation":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3/action/citation_signature","submit_replication":"https://pith.science/pith/IOCFWY275443WMDOP3UKRCVTB3/action/replication_record"}},"created_at":"2026-05-18T01:50:04.665683+00:00","updated_at":"2026-05-18T01:50:04.665683+00:00"}