{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:CYVA76HD4JDYKXZ7IRWOLAV7H3","short_pith_number":"pith:CYVA76HD","schema_version":"1.0","canonical_sha256":"162a0ff8e3e247855f3f446ce582bf3ee7dae257dae7a07079c16306444eca02","source":{"kind":"arxiv","id":"2410.14671","version":1},"attestation_state":"computed","paper":{"title":"Rapid Dust Formation in the Early Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrea Ferrara, Christa Gall, Danial Langeroodi, Jens Hjorth","submitted_at":"2024-10-18T17:59:04Z","abstract_excerpt":"Interstellar dust links the formation of the first stars to the rocky planet we inhabit by playing a pivotal role in the cooling and fragmentation of molecular clouds, and catalyzing the formation of water and organic molecules. Despite its central role, the origin of dust and its formation timescale remain unknown. Some models favor rapid production in supernova ejecta as the primary origin of dust, while others invoke slower production by evolved asymptotic giant branch stars or grain growth in the interstellar medium (ISM). The dust content of young early-universe galaxies is highly sensiti"},"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":"2410.14671","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-10-18T17:59:04Z","cross_cats_sorted":[],"title_canon_sha256":"83fd5dc59f9355f9e5fc945fb67d4ea6f0975e9c790eb15620cac1a517cbd45e","abstract_canon_sha256":"19bea46e07871a925c779bacbf9a6a67f19b8a5cda712a98da01130f34dfd045"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:22:35.119343Z","signature_b64":"TN4c6z0nl5OntBfwiELxQqgq65YAM8rCiB9bJq0xoJsf7wFtW6b4Hg01IvWtnPKP0fKedUVFRI0yP3WTHlfADg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"162a0ff8e3e247855f3f446ce582bf3ee7dae257dae7a07079c16306444eca02","last_reissued_at":"2026-07-05T09:22:35.118847Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:22:35.118847Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rapid Dust Formation in the Early Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrea Ferrara, Christa Gall, Danial Langeroodi, Jens Hjorth","submitted_at":"2024-10-18T17:59:04Z","abstract_excerpt":"Interstellar dust links the formation of the first stars to the rocky planet we inhabit by playing a pivotal role in the cooling and fragmentation of molecular clouds, and catalyzing the formation of water and organic molecules. Despite its central role, the origin of dust and its formation timescale remain unknown. Some models favor rapid production in supernova ejecta as the primary origin of dust, while others invoke slower production by evolved asymptotic giant branch stars or grain growth in the interstellar medium (ISM). The dust content of young early-universe galaxies is highly sensiti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.14671","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/2410.14671/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":"2410.14671","created_at":"2026-07-05T09:22:35.118905+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.14671v1","created_at":"2026-07-05T09:22:35.118905+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.14671","created_at":"2026-07-05T09:22:35.118905+00:00"},{"alias_kind":"pith_short_12","alias_value":"CYVA76HD4JDY","created_at":"2026-07-05T09:22:35.118905+00:00"},{"alias_kind":"pith_short_16","alias_value":"CYVA76HD4JDYKXZ7","created_at":"2026-07-05T09:22:35.118905+00:00"},{"alias_kind":"pith_short_8","alias_value":"CYVA76HD","created_at":"2026-07-05T09:22:35.118905+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.09829","citing_title":"Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies","ref_index":77,"is_internal_anchor":false},{"citing_arxiv_id":"2512.13778","citing_title":"Resolving dust and Ly{\\alpha} emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2605.09829","citing_title":"Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies","ref_index":77,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3","json":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3.json","graph_json":"https://pith.science/api/pith-number/CYVA76HD4JDYKXZ7IRWOLAV7H3/graph.json","events_json":"https://pith.science/api/pith-number/CYVA76HD4JDYKXZ7IRWOLAV7H3/events.json","paper":"https://pith.science/paper/CYVA76HD"},"agent_actions":{"view_html":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3","download_json":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3.json","view_paper":"https://pith.science/paper/CYVA76HD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.14671&json=true","fetch_graph":"https://pith.science/api/pith-number/CYVA76HD4JDYKXZ7IRWOLAV7H3/graph.json","fetch_events":"https://pith.science/api/pith-number/CYVA76HD4JDYKXZ7IRWOLAV7H3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3/action/storage_attestation","attest_author":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3/action/author_attestation","sign_citation":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3/action/citation_signature","submit_replication":"https://pith.science/pith/CYVA76HD4JDYKXZ7IRWOLAV7H3/action/replication_record"}},"created_at":"2026-07-05T09:22:35.118905+00:00","updated_at":"2026-07-05T09:22:35.118905+00:00"}