{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:S566MCTC4JYIT2YCTDNPMJNE2O","short_pith_number":"pith:S566MCTC","schema_version":"1.0","canonical_sha256":"977de60a62e27089eb0298daf625a4d382e3100686cd338cc7803a7efbd21388","source":{"kind":"arxiv","id":"1205.3801","version":3},"attestation_state":"computed","paper":{"title":"Constraining stellar assembly and AGN feedback at the peak epoch of star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adrianne Slyz, Joseph Silk, Julien Devriendt, Michael Dopita, Nimish Hathi, Robert O'Connell, Rogier Windhorst, Russell Ryan Jr, Seth Cohen, Sugata Kaviraj, Taysun Kimm, Yohan Dubois","submitted_at":"2012-05-16T20:28:02Z","abstract_excerpt":"We study stellar assembly and feedback from active galactic nuclei (AGN) around the epoch of peak star formation (1<z<2), by comparing hydrodynamic simulations to rest-frame UV-optical galaxy colours from the Wide Field Camera 3 (WFC3) Early-Release Science (ERS) Programme. Our Adaptive Mesh Refinement simulations include metal-dependent radiative cooling, star formation, kinetic outflows due to supernova explosions, and feedback from supermassive black holes. Our model assumes that when gas accretes onto black holes, a fraction of the energy is used to form either thermal winds or sub-relativ"},"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":"1205.3801","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-05-16T20:28:02Z","cross_cats_sorted":[],"title_canon_sha256":"403b0f993cd32d74b1d9dfec89f9990746aa8fa85027d6aa0329b38b2734495e","abstract_canon_sha256":"ddee9b58ab4ae3aaa322c93da7c9683876d479fe293386b172279ef7e80a8388"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:31.119904Z","signature_b64":"GEbxv2RXlqU5olPrSBIC0Yov/JqrcQfpmJSlJ8jlCCFcPbtD1YLEwgIsvhhwDMbiT3bHg8sDeJwb27IWSTJGDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"977de60a62e27089eb0298daf625a4d382e3100686cd338cc7803a7efbd21388","last_reissued_at":"2026-05-18T01:57:31.119276Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:31.119276Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining stellar assembly and AGN feedback at the peak epoch of star formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adrianne Slyz, Joseph Silk, Julien Devriendt, Michael Dopita, Nimish Hathi, Robert O'Connell, Rogier Windhorst, Russell Ryan Jr, Seth Cohen, Sugata Kaviraj, Taysun Kimm, Yohan Dubois","submitted_at":"2012-05-16T20:28:02Z","abstract_excerpt":"We study stellar assembly and feedback from active galactic nuclei (AGN) around the epoch of peak star formation (1<z<2), by comparing hydrodynamic simulations to rest-frame UV-optical galaxy colours from the Wide Field Camera 3 (WFC3) Early-Release Science (ERS) Programme. Our Adaptive Mesh Refinement simulations include metal-dependent radiative cooling, star formation, kinetic outflows due to supernova explosions, and feedback from supermassive black holes. Our model assumes that when gas accretes onto black holes, a fraction of the energy is used to form either thermal winds or sub-relativ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.3801","kind":"arxiv","version":3},"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":"1205.3801","created_at":"2026-05-18T01:57:31.119379+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.3801v3","created_at":"2026-05-18T01:57:31.119379+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.3801","created_at":"2026-05-18T01:57:31.119379+00:00"},{"alias_kind":"pith_short_12","alias_value":"S566MCTC4JYI","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"S566MCTC4JYIT2YC","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"S566MCTC","created_at":"2026-05-18T12:27:20.899486+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/S566MCTC4JYIT2YCTDNPMJNE2O","json":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O.json","graph_json":"https://pith.science/api/pith-number/S566MCTC4JYIT2YCTDNPMJNE2O/graph.json","events_json":"https://pith.science/api/pith-number/S566MCTC4JYIT2YCTDNPMJNE2O/events.json","paper":"https://pith.science/paper/S566MCTC"},"agent_actions":{"view_html":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O","download_json":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O.json","view_paper":"https://pith.science/paper/S566MCTC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.3801&json=true","fetch_graph":"https://pith.science/api/pith-number/S566MCTC4JYIT2YCTDNPMJNE2O/graph.json","fetch_events":"https://pith.science/api/pith-number/S566MCTC4JYIT2YCTDNPMJNE2O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O/action/storage_attestation","attest_author":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O/action/author_attestation","sign_citation":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O/action/citation_signature","submit_replication":"https://pith.science/pith/S566MCTC4JYIT2YCTDNPMJNE2O/action/replication_record"}},"created_at":"2026-05-18T01:57:31.119379+00:00","updated_at":"2026-05-18T01:57:31.119379+00:00"}