{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:AX7XJBA4EWMUEIWNUOGAVVOQ6Q","short_pith_number":"pith:AX7XJBA4","schema_version":"1.0","canonical_sha256":"05ff74841c25994222cda38c0ad5d0f413444624a99b7487b8e5b4c7f027f28b","source":{"kind":"arxiv","id":"1308.2367","version":1},"attestation_state":"computed","paper":{"title":"The 9 and 18 Micron Luminosity Function of Various Types of Galaxies with AKARI: Implication for the Dust Torus Structure of AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chisato Yamauchi, Daisuke Ishihara, Hideo Matsuhara, Matthew A. Malkan, Satoshi Takita, Shinki Oyabu, Takehiko Wada, Yoshiki Toba, Youichi Ohyama","submitted_at":"2013-08-11T06:41:07Z","abstract_excerpt":"We present the 9 and 18 micron luminosity functions (LFs) of galaxies at 0.006 < z < 0.8 (with an average redshift of ~ 0.04) using the AKARI mid-infrared all-sky survey catalog. We selected 243 galaxies at 9 micron and 255 galaxies at 18 micron from the Sloan Digital Sky Survey (SDSS) spectroscopy region. These galaxies were then classified by their optical emission lines, such as the line width of H_alpha or by their emission line ratios of [OIII]/H_beta and [NII]/H_alpha into five types: Type 1 active galactic nuclei (AGN) (Type 1); Type 2 AGN (Type 2); low-ionization narrow emission line g"},"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":"1308.2367","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-08-11T06:41:07Z","cross_cats_sorted":[],"title_canon_sha256":"003af61581f2c3cbdb0d57bcf3cbab5608db2762da7986eeaa9f9fafd4330c5b","abstract_canon_sha256":"9ebf7a06e404919d1d2aba76c16ac21de5ee9d2e40d8d3ca75d86ba785aff25a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:16.529223Z","signature_b64":"4YiZ7otuILdTKGIorXjjeDoyZ8PXhJHwPdnul6H6fpPOhjSkRDgbmWnUyq9l5sq32pUzFCYgMR3taUGlPtipAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"05ff74841c25994222cda38c0ad5d0f413444624a99b7487b8e5b4c7f027f28b","last_reissued_at":"2026-05-18T01:48:16.528761Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:16.528761Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The 9 and 18 Micron Luminosity Function of Various Types of Galaxies with AKARI: Implication for the Dust Torus Structure of AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Chisato Yamauchi, Daisuke Ishihara, Hideo Matsuhara, Matthew A. Malkan, Satoshi Takita, Shinki Oyabu, Takehiko Wada, Yoshiki Toba, Youichi Ohyama","submitted_at":"2013-08-11T06:41:07Z","abstract_excerpt":"We present the 9 and 18 micron luminosity functions (LFs) of galaxies at 0.006 < z < 0.8 (with an average redshift of ~ 0.04) using the AKARI mid-infrared all-sky survey catalog. We selected 243 galaxies at 9 micron and 255 galaxies at 18 micron from the Sloan Digital Sky Survey (SDSS) spectroscopy region. These galaxies were then classified by their optical emission lines, such as the line width of H_alpha or by their emission line ratios of [OIII]/H_beta and [NII]/H_alpha into five types: Type 1 active galactic nuclei (AGN) (Type 1); Type 2 AGN (Type 2); low-ionization narrow emission line g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.2367","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":"1308.2367","created_at":"2026-05-18T01:48:16.528837+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.2367v1","created_at":"2026-05-18T01:48:16.528837+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.2367","created_at":"2026-05-18T01:48:16.528837+00:00"},{"alias_kind":"pith_short_12","alias_value":"AX7XJBA4EWMU","created_at":"2026-05-18T12:27:38.830355+00:00"},{"alias_kind":"pith_short_16","alias_value":"AX7XJBA4EWMUEIWN","created_at":"2026-05-18T12:27:38.830355+00:00"},{"alias_kind":"pith_short_8","alias_value":"AX7XJBA4","created_at":"2026-05-18T12:27:38.830355+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/AX7XJBA4EWMUEIWNUOGAVVOQ6Q","json":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q.json","graph_json":"https://pith.science/api/pith-number/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/graph.json","events_json":"https://pith.science/api/pith-number/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/events.json","paper":"https://pith.science/paper/AX7XJBA4"},"agent_actions":{"view_html":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q","download_json":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q.json","view_paper":"https://pith.science/paper/AX7XJBA4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.2367&json=true","fetch_graph":"https://pith.science/api/pith-number/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/graph.json","fetch_events":"https://pith.science/api/pith-number/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/action/storage_attestation","attest_author":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/action/author_attestation","sign_citation":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/action/citation_signature","submit_replication":"https://pith.science/pith/AX7XJBA4EWMUEIWNUOGAVVOQ6Q/action/replication_record"}},"created_at":"2026-05-18T01:48:16.528837+00:00","updated_at":"2026-05-18T01:48:16.528837+00:00"}