{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:J43CMTDFQZMNKY3HFSFYKW2CA2","short_pith_number":"pith:J43CMTDF","schema_version":"1.0","canonical_sha256":"4f36264c658658d563672c8b855b4206a4021fd5d51c3b64c15b8430439fdda9","source":{"kind":"arxiv","id":"1405.1425","version":1},"attestation_state":"computed","paper":{"title":"Modeling the connection between ultraviolet and infrared galaxy populations across cosmic times","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2), (2) The University of Sheffield), E. Bernhard (1, E. Daddi ((1) CEA Saclay, J.R. Mullaney, M. B\\'ethermin, M. Pannella, M. Sargent, S. Heinis, V. Buat","submitted_at":"2014-05-06T20:00:23Z","abstract_excerpt":"Using a phenomenological approach, we self-consistently model the redshift evolution of the ultraviolet (UV) and infrared (IR) luminosity functions across cosmic time, as well as a range of observed IR properties of UV-selected galaxy population. This model is an extension of the 2SFM (2 star-formation modes) formalism, which is based on the observed \"main-sequence\" of star-forming galaxies, i.e. a strong correlation between their stellar mass and their star formation rate (SFR), and a secondary population of starbursts with an excess of star formation. The balance between the UV light from yo"},"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":"1405.1425","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-05-06T20:00:23Z","cross_cats_sorted":[],"title_canon_sha256":"4cdcb0c140b5f0033c003222cd24a73560464782ecd74880bd3de4aad1dcb797","abstract_canon_sha256":"c76e62890bd727cfcd727a298b4f0b207399dfab3b2630b788c6f9a74617ed72"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:17.010692Z","signature_b64":"jV4uV5oKy03mBFIxdKXDG2jaLAS9xxsi+1AhvhCzh9ru40UnP1vGGAhi2TN0mg1dFMfgygmSHDvZM8TWqn9kAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f36264c658658d563672c8b855b4206a4021fd5d51c3b64c15b8430439fdda9","last_reissued_at":"2026-05-18T01:43:17.009800Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:17.009800Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling the connection between ultraviolet and infrared galaxy populations across cosmic times","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2), (2) The University of Sheffield), E. Bernhard (1, E. Daddi ((1) CEA Saclay, J.R. Mullaney, M. B\\'ethermin, M. Pannella, M. Sargent, S. Heinis, V. Buat","submitted_at":"2014-05-06T20:00:23Z","abstract_excerpt":"Using a phenomenological approach, we self-consistently model the redshift evolution of the ultraviolet (UV) and infrared (IR) luminosity functions across cosmic time, as well as a range of observed IR properties of UV-selected galaxy population. This model is an extension of the 2SFM (2 star-formation modes) formalism, which is based on the observed \"main-sequence\" of star-forming galaxies, i.e. a strong correlation between their stellar mass and their star formation rate (SFR), and a secondary population of starbursts with an excess of star formation. The balance between the UV light from yo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.1425","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":"1405.1425","created_at":"2026-05-18T01:43:17.009916+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.1425v1","created_at":"2026-05-18T01:43:17.009916+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.1425","created_at":"2026-05-18T01:43:17.009916+00:00"},{"alias_kind":"pith_short_12","alias_value":"J43CMTDFQZMN","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_16","alias_value":"J43CMTDFQZMNKY3H","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_8","alias_value":"J43CMTDF","created_at":"2026-05-18T12:28:33.132498+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/J43CMTDFQZMNKY3HFSFYKW2CA2","json":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2.json","graph_json":"https://pith.science/api/pith-number/J43CMTDFQZMNKY3HFSFYKW2CA2/graph.json","events_json":"https://pith.science/api/pith-number/J43CMTDFQZMNKY3HFSFYKW2CA2/events.json","paper":"https://pith.science/paper/J43CMTDF"},"agent_actions":{"view_html":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2","download_json":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2.json","view_paper":"https://pith.science/paper/J43CMTDF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.1425&json=true","fetch_graph":"https://pith.science/api/pith-number/J43CMTDFQZMNKY3HFSFYKW2CA2/graph.json","fetch_events":"https://pith.science/api/pith-number/J43CMTDFQZMNKY3HFSFYKW2CA2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2/action/storage_attestation","attest_author":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2/action/author_attestation","sign_citation":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2/action/citation_signature","submit_replication":"https://pith.science/pith/J43CMTDFQZMNKY3HFSFYKW2CA2/action/replication_record"}},"created_at":"2026-05-18T01:43:17.009916+00:00","updated_at":"2026-05-18T01:43:17.009916+00:00"}