{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:SVPWH4VLGEZHQPHYP2IJBG7JI7","short_pith_number":"pith:SVPWH4VL","schema_version":"1.0","canonical_sha256":"955f63f2ab3132783cf87e90909be947f4b2090458e6d6673a6e1761cb6e76a2","source":{"kind":"arxiv","id":"astro-ph/0105428","version":1},"attestation_state":"computed","paper":{"title":"The dusty SF history of high-z galaxies, modelling tools and future prospects","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Gian Luigi Granato, Laura Silva","submitted_at":"2001-05-24T08:57:25Z","abstract_excerpt":"We summarize recent advances in the determination of the cosmic history of star formation and other properties of high-z galaxies, and the relevance of this information in our understanding of the formation of structures. We emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data. This demand a panchromatic approach to observations and suitable modelling tools. We spend also some words on expectations from future instruments."},"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":"astro-ph/0105428","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-05-24T08:57:25Z","cross_cats_sorted":[],"title_canon_sha256":"34df1b0c2319a047ac681b2f7a4322617f2361f22466a09c236ce49c181f1762","abstract_canon_sha256":"a7c0f15936e5bd2b320127c3c64e49f2896bb08312c98513f4ef486566336eff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:21:50.518631Z","signature_b64":"lrrvAqiR3ioUaYFXVux6zxdRyerkNonVmzPK/SOkQo2Am1RFzyGVOX3pn2lf4gh+9xeUBQHtf4VzJ9/ir1WkCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"955f63f2ab3132783cf87e90909be947f4b2090458e6d6673a6e1761cb6e76a2","last_reissued_at":"2026-05-18T01:21:50.518136Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:21:50.518136Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The dusty SF history of high-z galaxies, modelling tools and future prospects","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Gian Luigi Granato, Laura Silva","submitted_at":"2001-05-24T08:57:25Z","abstract_excerpt":"We summarize recent advances in the determination of the cosmic history of star formation and other properties of high-z galaxies, and the relevance of this information in our understanding of the formation of structures. We emphasize the importance of dust reprocessing in the high--z universe, as demonstrated in particular by IR and sub-mm data. This demand a panchromatic approach to observations and suitable modelling tools. We spend also some words on expectations from future instruments."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0105428","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":""},"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":"astro-ph/0105428","created_at":"2026-05-18T01:21:50.518208+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0105428v1","created_at":"2026-05-18T01:21:50.518208+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0105428","created_at":"2026-05-18T01:21:50.518208+00:00"},{"alias_kind":"pith_short_12","alias_value":"SVPWH4VLGEZH","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"SVPWH4VLGEZHQPHY","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"SVPWH4VL","created_at":"2026-05-18T12:25:50.845339+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/SVPWH4VLGEZHQPHYP2IJBG7JI7","json":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7.json","graph_json":"https://pith.science/api/pith-number/SVPWH4VLGEZHQPHYP2IJBG7JI7/graph.json","events_json":"https://pith.science/api/pith-number/SVPWH4VLGEZHQPHYP2IJBG7JI7/events.json","paper":"https://pith.science/paper/SVPWH4VL"},"agent_actions":{"view_html":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7","download_json":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7.json","view_paper":"https://pith.science/paper/SVPWH4VL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0105428&json=true","fetch_graph":"https://pith.science/api/pith-number/SVPWH4VLGEZHQPHYP2IJBG7JI7/graph.json","fetch_events":"https://pith.science/api/pith-number/SVPWH4VLGEZHQPHYP2IJBG7JI7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7/action/storage_attestation","attest_author":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7/action/author_attestation","sign_citation":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7/action/citation_signature","submit_replication":"https://pith.science/pith/SVPWH4VLGEZHQPHYP2IJBG7JI7/action/replication_record"}},"created_at":"2026-05-18T01:21:50.518208+00:00","updated_at":"2026-05-18T01:21:50.518208+00:00"}