{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BMEF277ILANLPIMIQUGWETOSLS","short_pith_number":"pith:BMEF277I","schema_version":"1.0","canonical_sha256":"0b085d7fe8581ab7a188850d624dd25cb44af74e28a1da0b255658cbdc6ab4c2","source":{"kind":"arxiv","id":"2405.04598","version":1},"attestation_state":"computed","paper":{"title":"Cue: A Fast and Flexible Photoionization Emulator for Modeling Nebular Emission Powered By Almost Any Ionizing Source","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Benjamin D. Johnson, Joel Leja, Minjung Park, Razieh Emami, Rebecca Davies, Sandro Tacchella, Sirio Belli, Yijia Li","submitted_at":"2024-05-07T18:21:04Z","abstract_excerpt":"The complex physics governing nebular emission in galaxies, particularly in the early universe, often defy simple low-dimensional models. This has proven to be a significant barrier in understanding the (often diverse) ionizing sources powering this emission. We present Cue, a highly flexible tool for interpreting nebular emission across a wide range of abundances and ionizing conditions of galaxies at different redshifts. Unlike typical nebular models used to interpret extragalactic nebular emission, our model does not require a specific ionizing spectrum as a source, instead approximating th"},"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":"2405.04598","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-05-07T18:21:04Z","cross_cats_sorted":[],"title_canon_sha256":"66f05866f3d69099f2232052cfcc6974d7a15df5ecba667e2dcc99edc24e5cc0","abstract_canon_sha256":"ccbd44595c458f0faa756cdb2663452f88a62d0ebd7fe88008ccd9fdf462979a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:16:51.325035Z","signature_b64":"On8fInA18NWLJ9xFzR6PZntx1u/8hur3M8uTYqUQJWz0bi5mF/SByfcuJabWLG1uCfpeylQvEcuo7iR7shLbDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b085d7fe8581ab7a188850d624dd25cb44af74e28a1da0b255658cbdc6ab4c2","last_reissued_at":"2026-07-05T08:16:51.324568Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:16:51.324568Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cue: A Fast and Flexible Photoionization Emulator for Modeling Nebular Emission Powered By Almost Any Ionizing Source","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Benjamin D. Johnson, Joel Leja, Minjung Park, Razieh Emami, Rebecca Davies, Sandro Tacchella, Sirio Belli, Yijia Li","submitted_at":"2024-05-07T18:21:04Z","abstract_excerpt":"The complex physics governing nebular emission in galaxies, particularly in the early universe, often defy simple low-dimensional models. This has proven to be a significant barrier in understanding the (often diverse) ionizing sources powering this emission. We present Cue, a highly flexible tool for interpreting nebular emission across a wide range of abundances and ionizing conditions of galaxies at different redshifts. Unlike typical nebular models used to interpret extragalactic nebular emission, our model does not require a specific ionizing spectrum as a source, instead approximating th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.04598","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/2405.04598/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":"2405.04598","created_at":"2026-07-05T08:16:51.324629+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.04598v1","created_at":"2026-07-05T08:16:51.324629+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.04598","created_at":"2026-07-05T08:16:51.324629+00:00"},{"alias_kind":"pith_short_12","alias_value":"BMEF277ILANL","created_at":"2026-07-05T08:16:51.324629+00:00"},{"alias_kind":"pith_short_16","alias_value":"BMEF277ILANLPIMI","created_at":"2026-07-05T08:16:51.324629+00:00"},{"alias_kind":"pith_short_8","alias_value":"BMEF277I","created_at":"2026-07-05T08:16:51.324629+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.05424","citing_title":"Nebular emission from composite star-forming galaxies -- I. A novel modelling approach","ref_index":52,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS","json":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS.json","graph_json":"https://pith.science/api/pith-number/BMEF277ILANLPIMIQUGWETOSLS/graph.json","events_json":"https://pith.science/api/pith-number/BMEF277ILANLPIMIQUGWETOSLS/events.json","paper":"https://pith.science/paper/BMEF277I"},"agent_actions":{"view_html":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS","download_json":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS.json","view_paper":"https://pith.science/paper/BMEF277I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.04598&json=true","fetch_graph":"https://pith.science/api/pith-number/BMEF277ILANLPIMIQUGWETOSLS/graph.json","fetch_events":"https://pith.science/api/pith-number/BMEF277ILANLPIMIQUGWETOSLS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS/action/storage_attestation","attest_author":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS/action/author_attestation","sign_citation":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS/action/citation_signature","submit_replication":"https://pith.science/pith/BMEF277ILANLPIMIQUGWETOSLS/action/replication_record"}},"created_at":"2026-07-05T08:16:51.324629+00:00","updated_at":"2026-07-05T08:16:51.324629+00:00"}