{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SCO7VM3UJ66A6W7ZQHEKGKPBD2","short_pith_number":"pith:SCO7VM3U","schema_version":"1.0","canonical_sha256":"909dfab3744fbc0f5bf981c8a329e11e9acba9c0af1104ec064100857feb0804","source":{"kind":"arxiv","id":"1310.4147","version":1},"attestation_state":"computed","paper":{"title":"The suppression of star formation by powerful active galactic nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Blain, A. Boselli, A. Cava, A. Conley, A. Cooray, A. Franceschini, A.J. Smith, A. Omont, A. Papageorgiou, B. Altieri, B. Maffei, B. O'Halloran, B. Schulz, C.D. Dowell, C.K. Xu, C.P. Pearson, D. Elbaz, D. Farrah, D.L. Clements, D.L. Shupe, Douglas Scott, D. Rigopoulou, D. Rizzo, E. Dwek, E. Hatziminaoglou, E. Ibar, E.N. Dubois, G. Lagache, G. Mainetti, G. Rodighiero, G. Wright, H. Aussel, H.T. Nguyen, I.G. Roseboom, I. Perez-Fournon, I. Valtchanov, J.A. Stevens, J. Bock, J.D. Vieira, J. Glenn, J.I. Rawlings, J.S. Dunlop, K.E. Tugwell, K. Isaak, L. Conversi, L. Levenson, L. Marchetti, L. Riguccini, L. Vigroux, L. Wang, M. Fox, M. Griffin, M. Halpern, M.J. Page, M. Pohlen, M. Rowan-Robinson, M. Sanchez Portal, M. Symeonidis, M. Trichas, M. Vaccari, M. Viero, M. Zemcov, N. Castro-Rodr'iguez, N. Lu, N. Seymour, P. Chanial, P. Panuzzo, R.J. Ivison, R. Ward, S. Dye, S. Eales, S.J. Oliver, S. Madden, T. Babbedge, V. Arumugam, V. Buat, W. Gear","submitted_at":"2013-10-15T18:58:42Z","abstract_excerpt":"The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly from accretion onto black holes. It is widely suspected, but unproven, that the tight correlation in mass of the black hole and stellar components results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, while powerful star-forming galaxies are usually dust-obscure"},"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":"1310.4147","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-15T18:58:42Z","cross_cats_sorted":[],"title_canon_sha256":"17631865c3e64050a0bc16a155a32b4df26877959083dc81dbe65aa4e995fedd","abstract_canon_sha256":"2ab72f597ad15c5a568bd03d639b04996c9d1079127ba4912beca256371bff57"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:10:24.936610Z","signature_b64":"BrtJ3IdSyui37Nhvlh0zcmRJJOgG+SgGpbbE34YbqeJMyv7jNETBMwHxSl7sEJD6yCktpmdEfk5UnQmdwuUnCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"909dfab3744fbc0f5bf981c8a329e11e9acba9c0af1104ec064100857feb0804","last_reissued_at":"2026-05-18T03:10:24.936016Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:10:24.936016Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The suppression of star formation by powerful active galactic nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amblard, A. Blain, A. Boselli, A. Cava, A. Conley, A. Cooray, A. Franceschini, A.J. Smith, A. Omont, A. Papageorgiou, B. Altieri, B. Maffei, B. O'Halloran, B. Schulz, C.D. Dowell, C.K. Xu, C.P. Pearson, D. Elbaz, D. Farrah, D.L. Clements, D.L. Shupe, Douglas Scott, D. Rigopoulou, D. Rizzo, E. Dwek, E. Hatziminaoglou, E. Ibar, E.N. Dubois, G. Lagache, G. Mainetti, G. Rodighiero, G. Wright, H. Aussel, H.T. Nguyen, I.G. Roseboom, I. Perez-Fournon, I. Valtchanov, J.A. Stevens, J. Bock, J.D. Vieira, J. Glenn, J.I. Rawlings, J.S. Dunlop, K.E. Tugwell, K. Isaak, L. Conversi, L. Levenson, L. Marchetti, L. Riguccini, L. Vigroux, L. Wang, M. Fox, M. Griffin, M. Halpern, M.J. Page, M. Pohlen, M. Rowan-Robinson, M. Sanchez Portal, M. Symeonidis, M. Trichas, M. Vaccari, M. Viero, M. Zemcov, N. Castro-Rodr'iguez, N. Lu, N. Seymour, P. Chanial, P. Panuzzo, R.J. Ivison, R. Ward, S. Dye, S. Eales, S.J. Oliver, S. Madden, T. Babbedge, V. Arumugam, V. Buat, W. Gear","submitted_at":"2013-10-15T18:58:42Z","abstract_excerpt":"The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly from accretion onto black holes. It is widely suspected, but unproven, that the tight correlation in mass of the black hole and stellar components results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, while powerful star-forming galaxies are usually dust-obscure"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4147","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":"1310.4147","created_at":"2026-05-18T03:10:24.936117+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.4147v1","created_at":"2026-05-18T03:10:24.936117+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4147","created_at":"2026-05-18T03:10:24.936117+00:00"},{"alias_kind":"pith_short_12","alias_value":"SCO7VM3UJ66A","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SCO7VM3UJ66A6W7Z","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SCO7VM3U","created_at":"2026-05-18T12:27:59.945178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.19658","citing_title":"The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs","ref_index":41,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2","json":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2.json","graph_json":"https://pith.science/api/pith-number/SCO7VM3UJ66A6W7ZQHEKGKPBD2/graph.json","events_json":"https://pith.science/api/pith-number/SCO7VM3UJ66A6W7ZQHEKGKPBD2/events.json","paper":"https://pith.science/paper/SCO7VM3U"},"agent_actions":{"view_html":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2","download_json":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2.json","view_paper":"https://pith.science/paper/SCO7VM3U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.4147&json=true","fetch_graph":"https://pith.science/api/pith-number/SCO7VM3UJ66A6W7ZQHEKGKPBD2/graph.json","fetch_events":"https://pith.science/api/pith-number/SCO7VM3UJ66A6W7ZQHEKGKPBD2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2/action/storage_attestation","attest_author":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2/action/author_attestation","sign_citation":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2/action/citation_signature","submit_replication":"https://pith.science/pith/SCO7VM3UJ66A6W7ZQHEKGKPBD2/action/replication_record"}},"created_at":"2026-05-18T03:10:24.936117+00:00","updated_at":"2026-05-18T03:10:24.936117+00:00"}