{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:3YKRXIJDBSHJV2B77NI7L3RTGP","short_pith_number":"pith:3YKRXIJD","schema_version":"1.0","canonical_sha256":"de151ba1230c8e9ae83ffb51f5ee3333cb55b9d53e33d8a3fb76f0f7ceca97a5","source":{"kind":"arxiv","id":"2212.02522","version":1},"attestation_state":"computed","paper":{"title":"Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adele Plat, Alba Vidal-Garcia, Anna Feltre, Christophe Morisset, Dylan Nelson, Emma Curtis-Lake, Ena Choi, Jacopo Chevallard, Michaela Hirschmann, Rachel S. Somerville, Stephane Charlot","submitted_at":"2022-12-05T19:00:03Z","abstract_excerpt":"We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z$\\approx$0 to z=8 in a full cosmological framework. We achieve this by coupling, in post-processing, the cosmological IllustrisTNG simulations with new-generation nebular-emission models, accounting for line emission from young stars, post-asymptotic-giant-branch (PAGB) stars, accreting black holes (BHs) and, for the first time, fast radiative shocks. The optical emission-line properties of simulated galaxies dominated by different ionizing sources are largely consist"},"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":"2212.02522","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-12-05T19:00:03Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"73a8883573a0ea5ea16034a0e0c8566b5cb35d3333293a935fb17ed9e6a8aa4e","abstract_canon_sha256":"25815a2af411b17f694e96de36f5089b40f7a76a4d43a32659cf78ab88eed42a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:22:31.908356Z","signature_b64":"gzO4sDZmlB459RcHN+74puv0ZqcfN+vklge6+JkrsxV51yoGRXMwFSDGwWifyTxBuWd8c7MxyFNGYAcBcLjtDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de151ba1230c8e9ae83ffb51f5ee3333cb55b9d53e33d8a3fb76f0f7ceca97a5","last_reissued_at":"2026-07-05T05:22:31.907876Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:22:31.907876Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Adele Plat, Alba Vidal-Garcia, Anna Feltre, Christophe Morisset, Dylan Nelson, Emma Curtis-Lake, Ena Choi, Jacopo Chevallard, Michaela Hirschmann, Rachel S. Somerville, Stephane Charlot","submitted_at":"2022-12-05T19:00:03Z","abstract_excerpt":"We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z$\\approx$0 to z=8 in a full cosmological framework. We achieve this by coupling, in post-processing, the cosmological IllustrisTNG simulations with new-generation nebular-emission models, accounting for line emission from young stars, post-asymptotic-giant-branch (PAGB) stars, accreting black holes (BHs) and, for the first time, fast radiative shocks. The optical emission-line properties of simulated galaxies dominated by different ionizing sources are largely consist"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.02522","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2212.02522/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2212.02522","created_at":"2026-07-05T05:22:31.907934+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.02522v1","created_at":"2026-07-05T05:22:31.907934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.02522","created_at":"2026-07-05T05:22:31.907934+00:00"},{"alias_kind":"pith_short_12","alias_value":"3YKRXIJDBSHJ","created_at":"2026-07-05T05:22:31.907934+00:00"},{"alias_kind":"pith_short_16","alias_value":"3YKRXIJDBSHJV2B7","created_at":"2026-07-05T05:22:31.907934+00:00"},{"alias_kind":"pith_short_8","alias_value":"3YKRXIJD","created_at":"2026-07-05T05:22:31.907934+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17146","citing_title":"MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon","ref_index":160,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP","json":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP.json","graph_json":"https://pith.science/api/pith-number/3YKRXIJDBSHJV2B77NI7L3RTGP/graph.json","events_json":"https://pith.science/api/pith-number/3YKRXIJDBSHJV2B77NI7L3RTGP/events.json","paper":"https://pith.science/paper/3YKRXIJD"},"agent_actions":{"view_html":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP","download_json":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP.json","view_paper":"https://pith.science/paper/3YKRXIJD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.02522&json=true","fetch_graph":"https://pith.science/api/pith-number/3YKRXIJDBSHJV2B77NI7L3RTGP/graph.json","fetch_events":"https://pith.science/api/pith-number/3YKRXIJDBSHJV2B77NI7L3RTGP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP/action/storage_attestation","attest_author":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP/action/author_attestation","sign_citation":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP/action/citation_signature","submit_replication":"https://pith.science/pith/3YKRXIJDBSHJV2B77NI7L3RTGP/action/replication_record"}},"created_at":"2026-07-05T05:22:31.907934+00:00","updated_at":"2026-07-05T05:22:31.907934+00:00"}