{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:NWTDXT64QKSDWDBB5JSNYZCSL3","short_pith_number":"pith:NWTDXT64","schema_version":"1.0","canonical_sha256":"6da63bcfdc82a43b0c21ea64dc64525ed845261f983fdb0f2bef0d9f70e88257","source":{"kind":"arxiv","id":"1509.04384","version":1},"attestation_state":"computed","paper":{"title":"Mid-Infrared Luminosity Function of Local Star-Forming Galaxies in the NEP-Wide Survey Field of AKARI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Hideo Matsuhara, Hyung Mok Lee, Hyunjin Shim, Min Gyu Kim, Myung Gyoon Lee, Myungshin Im, Seong Jin Kim, Tomotsugu Goto, Woong-Seob Jeong","submitted_at":"2015-09-15T03:15:39Z","abstract_excerpt":"We present mid-infrared (MIR) luminosity functions (LFs) of local star-forming (SF) galaxies in the AKARI NEP-Wide Survey field. In order to derive more accurate luminosity function, we used spectroscopic sample only. Based on the NEP-Wide point source catalogue containing a large number of infrared (IR) sources distributed over the wide (5.4 sq. deg.) field, we incorporated the spectroscopic redshift data for about 1790 selected targets obtained by optical follow-up surveys with MMT/Hectospec and WIYN/Hydra. The AKARI continuous 2 to 24 micron wavelength coverage as well as photometric data f"},"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":"1509.04384","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-09-15T03:15:39Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"29422da2918bf7e32826d5eaaa2d9843b43b94bcb8a4bccfe4dfa4e688c2f6d0","abstract_canon_sha256":"16726fb0ba7835956373a3cae9559c9fb1d895b6cfbbd0dd07ce090e66dadb1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:30:17.736731Z","signature_b64":"w+DQ4CuTNvQ77dFEbC4jz1zY/aTwI7eUXWLeF1fDZG+pemUa8n2P4xkwwOfOR+XeluEfpLejLUo6rprgVF1BDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6da63bcfdc82a43b0c21ea64dc64525ed845261f983fdb0f2bef0d9f70e88257","last_reissued_at":"2026-05-18T01:30:17.736023Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:30:17.736023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mid-Infrared Luminosity Function of Local Star-Forming Galaxies in the NEP-Wide Survey Field of AKARI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Hideo Matsuhara, Hyung Mok Lee, Hyunjin Shim, Min Gyu Kim, Myung Gyoon Lee, Myungshin Im, Seong Jin Kim, Tomotsugu Goto, Woong-Seob Jeong","submitted_at":"2015-09-15T03:15:39Z","abstract_excerpt":"We present mid-infrared (MIR) luminosity functions (LFs) of local star-forming (SF) galaxies in the AKARI NEP-Wide Survey field. In order to derive more accurate luminosity function, we used spectroscopic sample only. Based on the NEP-Wide point source catalogue containing a large number of infrared (IR) sources distributed over the wide (5.4 sq. deg.) field, we incorporated the spectroscopic redshift data for about 1790 selected targets obtained by optical follow-up surveys with MMT/Hectospec and WIYN/Hydra. The AKARI continuous 2 to 24 micron wavelength coverage as well as photometric data f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.04384","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":"1509.04384","created_at":"2026-05-18T01:30:17.736166+00:00"},{"alias_kind":"arxiv_version","alias_value":"1509.04384v1","created_at":"2026-05-18T01:30:17.736166+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1509.04384","created_at":"2026-05-18T01:30:17.736166+00:00"},{"alias_kind":"pith_short_12","alias_value":"NWTDXT64QKSD","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"NWTDXT64QKSDWDBB","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"NWTDXT64","created_at":"2026-05-18T12:29:34.919912+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/NWTDXT64QKSDWDBB5JSNYZCSL3","json":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3.json","graph_json":"https://pith.science/api/pith-number/NWTDXT64QKSDWDBB5JSNYZCSL3/graph.json","events_json":"https://pith.science/api/pith-number/NWTDXT64QKSDWDBB5JSNYZCSL3/events.json","paper":"https://pith.science/paper/NWTDXT64"},"agent_actions":{"view_html":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3","download_json":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3.json","view_paper":"https://pith.science/paper/NWTDXT64","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1509.04384&json=true","fetch_graph":"https://pith.science/api/pith-number/NWTDXT64QKSDWDBB5JSNYZCSL3/graph.json","fetch_events":"https://pith.science/api/pith-number/NWTDXT64QKSDWDBB5JSNYZCSL3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3/action/storage_attestation","attest_author":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3/action/author_attestation","sign_citation":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3/action/citation_signature","submit_replication":"https://pith.science/pith/NWTDXT64QKSDWDBB5JSNYZCSL3/action/replication_record"}},"created_at":"2026-05-18T01:30:17.736166+00:00","updated_at":"2026-05-18T01:30:17.736166+00:00"}