{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BEVM7EFYW5OSKLHSXE66LRSZYO","short_pith_number":"pith:BEVM7EFY","schema_version":"1.0","canonical_sha256":"092acf90b8b75d252cf2b93de5c659c389f13149acbb2d6811adc83b16eda871","source":{"kind":"arxiv","id":"2405.00376","version":1},"attestation_state":"computed","paper":{"title":"EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Asa F. L. Bluck, Christopher J. Conselice, Daniel O. Bettaney, Dimitrios Irodotou, Duncan Austin, James Trussler, Joseph Caruana, Justin T.F. Basham, Katherine Ormerod, Leonardo Ferreira, Nathan Adams, Qiong Li, Thomas Harvey, William J. Roper","submitted_at":"2024-05-01T08:06:13Z","abstract_excerpt":"We measure the broad impact of galaxy structure on galaxy formation by examining the ongoing star formation and integrated star formation history as revealed through the stellar masses of galaxies at $z < 7$ based on JWST CEERS data from the Extended Groth Strip (EGS). Using the morphological catalog of 3965 visually classified JWST galaxies from Ferreira et al. (2023), we investigate the evolution of stars, and when they form, as a function of morphological type as well as galaxies classified as passive and starburst through spectral energy distributions. Although disk galaxies dominate the s"},"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":"2405.00376","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-05-01T08:06:13Z","cross_cats_sorted":[],"title_canon_sha256":"e0bddb6ae919f9b10e6efb30bc117634ac99edda6d3fe8697611c55c63157772","abstract_canon_sha256":"c692ff7c1921616eda57fec4b7f1f55b25d962dff7b89a97836d31bf0aaa7195"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:14:12.123425Z","signature_b64":"CMarUA+b6u+pvRKgkk1mmd1OBFpVuusQXB1PEXgwy0gq0S/l2IVloGYrT4kN+C2WD+mAJye5sBVR8KtIJa6sAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"092acf90b8b75d252cf2b93de5c659c389f13149acbb2d6811adc83b16eda871","last_reissued_at":"2026-07-05T08:14:12.122944Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:14:12.122944Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Asa F. L. Bluck, Christopher J. Conselice, Daniel O. Bettaney, Dimitrios Irodotou, Duncan Austin, James Trussler, Joseph Caruana, Justin T.F. Basham, Katherine Ormerod, Leonardo Ferreira, Nathan Adams, Qiong Li, Thomas Harvey, William J. Roper","submitted_at":"2024-05-01T08:06:13Z","abstract_excerpt":"We measure the broad impact of galaxy structure on galaxy formation by examining the ongoing star formation and integrated star formation history as revealed through the stellar masses of galaxies at $z < 7$ based on JWST CEERS data from the Extended Groth Strip (EGS). Using the morphological catalog of 3965 visually classified JWST galaxies from Ferreira et al. (2023), we investigate the evolution of stars, and when they form, as a function of morphological type as well as galaxies classified as passive and starburst through spectral energy distributions. Although disk galaxies dominate the s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.00376","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/2405.00376/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":"2405.00376","created_at":"2026-07-05T08:14:12.123000+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.00376v1","created_at":"2026-07-05T08:14:12.123000+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.00376","created_at":"2026-07-05T08:14:12.123000+00:00"},{"alias_kind":"pith_short_12","alias_value":"BEVM7EFYW5OS","created_at":"2026-07-05T08:14:12.123000+00:00"},{"alias_kind":"pith_short_16","alias_value":"BEVM7EFYW5OSKLHS","created_at":"2026-07-05T08:14:12.123000+00:00"},{"alias_kind":"pith_short_8","alias_value":"BEVM7EFY","created_at":"2026-07-05T08:14:12.123000+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/BEVM7EFYW5OSKLHSXE66LRSZYO","json":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO.json","graph_json":"https://pith.science/api/pith-number/BEVM7EFYW5OSKLHSXE66LRSZYO/graph.json","events_json":"https://pith.science/api/pith-number/BEVM7EFYW5OSKLHSXE66LRSZYO/events.json","paper":"https://pith.science/paper/BEVM7EFY"},"agent_actions":{"view_html":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO","download_json":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO.json","view_paper":"https://pith.science/paper/BEVM7EFY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.00376&json=true","fetch_graph":"https://pith.science/api/pith-number/BEVM7EFYW5OSKLHSXE66LRSZYO/graph.json","fetch_events":"https://pith.science/api/pith-number/BEVM7EFYW5OSKLHSXE66LRSZYO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO/action/storage_attestation","attest_author":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO/action/author_attestation","sign_citation":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO/action/citation_signature","submit_replication":"https://pith.science/pith/BEVM7EFYW5OSKLHSXE66LRSZYO/action/replication_record"}},"created_at":"2026-07-05T08:14:12.123000+00:00","updated_at":"2026-07-05T08:14:12.123000+00:00"}