{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:OJTFLCKKS6L4UHE3FEYNNC2NFW","short_pith_number":"pith:OJTFLCKK","schema_version":"1.0","canonical_sha256":"726655894a9797ca1c9b2930d68b4d2d8357ce1bedf9f0fc1a14fe25f6bb0625","source":{"kind":"arxiv","id":"1008.0859","version":1},"attestation_state":"computed","paper":{"title":"Luminosity Functions of Local Infrared Galaxies with AKARI: Implications to the Cosmic Star Formation History and AGN Evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Chisato Yamauchi (JAXA), Chris Pearson (Rutherford), Chris Sedgwick (Open U.), Daisuke Ishihara (Nagoya), Emeric Le Floc'h (CEA), Ezequiel Treister (IfA, Hanae Inami, Hideo Matsuhara (JAXA), Hyung Mok Lee (SNU), Shinki Oyabu (Subaru), Stephane Arnouts (CFHT), Stephen Serjeant, Takao Nakagawa (JAXA), Takehiko Wada, Tomotsugu Goto (ifa, Toshinobu Takagi, Tsutomu T. Takeuchi (Nagoya), University of Hawaii), University of Hawaii/Subaru telescope), Woong-Seob Jeong (KASI)","submitted_at":"2010-08-04T20:00:13Z","abstract_excerpt":"Infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution. The AKARI IR space telescope performed all sky survey in 6 IR bands (9, 18, 65, 90, 140, and 160um) with 3-10 times better sensitivity than IRAS, covering the crucial far-IR wavelengths across the peak of the dust emission. Combined with a better spatial resolution, AKARI can much more precisely measure the total infrared luminosity (L_TIR) of individual galaxies, and thus, the total infrared luminosity density in the local Universe. By fitting IR SED models, we have re-measured L_TIR "},"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":"1008.0859","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-04T20:00:13Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"59b6e495e2e1dc7f0c3463e52091e7e9b83fe73092fcfbda548a69274ba85414","abstract_canon_sha256":"e04ed0c5647a8520e543e359051e4b078b4fb86f8c5fe0a66c43d484409fe18c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:59.208581Z","signature_b64":"7nVuUr0U4Wz+ukaI701i+MCrxVOYFnZEUU3gXYWEAyjYmfJVDvLkL7EnKreM0MemVHpj7I5uqiD4+I8wFrivAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"726655894a9797ca1c9b2930d68b4d2d8357ce1bedf9f0fc1a14fe25f6bb0625","last_reissued_at":"2026-05-18T02:05:59.207881Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:59.207881Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Luminosity Functions of Local Infrared Galaxies with AKARI: Implications to the Cosmic Star Formation History and AGN Evolution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Chisato Yamauchi (JAXA), Chris Pearson (Rutherford), Chris Sedgwick (Open U.), Daisuke Ishihara (Nagoya), Emeric Le Floc'h (CEA), Ezequiel Treister (IfA, Hanae Inami, Hideo Matsuhara (JAXA), Hyung Mok Lee (SNU), Shinki Oyabu (Subaru), Stephane Arnouts (CFHT), Stephen Serjeant, Takao Nakagawa (JAXA), Takehiko Wada, Tomotsugu Goto (ifa, Toshinobu Takagi, Tsutomu T. Takeuchi (Nagoya), University of Hawaii), University of Hawaii/Subaru telescope), Woong-Seob Jeong (KASI)","submitted_at":"2010-08-04T20:00:13Z","abstract_excerpt":"Infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution. The AKARI IR space telescope performed all sky survey in 6 IR bands (9, 18, 65, 90, 140, and 160um) with 3-10 times better sensitivity than IRAS, covering the crucial far-IR wavelengths across the peak of the dust emission. Combined with a better spatial resolution, AKARI can much more precisely measure the total infrared luminosity (L_TIR) of individual galaxies, and thus, the total infrared luminosity density in the local Universe. By fitting IR SED models, we have re-measured L_TIR "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.0859","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":"1008.0859","created_at":"2026-05-18T02:05:59.207988+00:00"},{"alias_kind":"arxiv_version","alias_value":"1008.0859v1","created_at":"2026-05-18T02:05:59.207988+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.0859","created_at":"2026-05-18T02:05:59.207988+00:00"},{"alias_kind":"pith_short_12","alias_value":"OJTFLCKKS6L4","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"OJTFLCKKS6L4UHE3","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"OJTFLCKK","created_at":"2026-05-18T12:26:12.377268+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/OJTFLCKKS6L4UHE3FEYNNC2NFW","json":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW.json","graph_json":"https://pith.science/api/pith-number/OJTFLCKKS6L4UHE3FEYNNC2NFW/graph.json","events_json":"https://pith.science/api/pith-number/OJTFLCKKS6L4UHE3FEYNNC2NFW/events.json","paper":"https://pith.science/paper/OJTFLCKK"},"agent_actions":{"view_html":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW","download_json":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW.json","view_paper":"https://pith.science/paper/OJTFLCKK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1008.0859&json=true","fetch_graph":"https://pith.science/api/pith-number/OJTFLCKKS6L4UHE3FEYNNC2NFW/graph.json","fetch_events":"https://pith.science/api/pith-number/OJTFLCKKS6L4UHE3FEYNNC2NFW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW/action/storage_attestation","attest_author":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW/action/author_attestation","sign_citation":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW/action/citation_signature","submit_replication":"https://pith.science/pith/OJTFLCKKS6L4UHE3FEYNNC2NFW/action/replication_record"}},"created_at":"2026-05-18T02:05:59.207988+00:00","updated_at":"2026-05-18T02:05:59.207988+00:00"}