{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:I5IT2HLXTT3YHBMJH4I2XQLAMR","short_pith_number":"pith:I5IT2HLX","schema_version":"1.0","canonical_sha256":"47513d1d779cf78385893f11abc160646c5d393fd27c765365e25b9a7614d7ba","source":{"kind":"arxiv","id":"1307.6356","version":1},"attestation_state":"computed","paper":{"title":"A relation of the PAH 3.3 um feature with star-forming activity for galaxies with a wide range of infrared luminosity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Daisuke Ishihara, Hidehiro Kaneda, Ji Hoon Kim, Mitsuyoshi Yamagishi, Myungshin Im, Rika Yamada, Shinki Oyabu","submitted_at":"2013-07-24T09:42:30Z","abstract_excerpt":"For star-forming galaxies, we investigate a global relation between polycyclic aromatic hydrocarbon (PAH) emission luminosity at 3.3 um, L_PAH3.3, and infrared (8-1000 um) luminosity, L_IR, to understand how the PAH 3.3 um feature relates to the star formation activity. With AKARI, we performed near-infrared (2.5-5 um) spectroscopy of 184 galaxies which have L_IR \\sim 10^8 - 10^13 L_sun. We classify the samples into infrared galaxies (IRGs; L_IR < 10^11 L_sun), luminous infrared galaxies (LIRGs; L_IR \\sim 10^11 -10^12 L_sun) and ultra luminous infrared galaxies (ULIRGs; L_IR > 10^12 L_sun). We"},"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":"1307.6356","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-07-24T09:42:30Z","cross_cats_sorted":[],"title_canon_sha256":"9e083c093b137ef28cc42d5ff2654b3ffce552caab382d27b030308b0fd46535","abstract_canon_sha256":"4fd7f82e6a2f9c8f91b688f593314bf7a9c8a049c6e41bd29f5060165af62aac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:40.706605Z","signature_b64":"cqZl3iKGbHLOXfcEpTgJjKr4MCE0zQsEoi03C+19bDtEXCt7/jynAfJYz3Q4fuRihPwHbXQLwnp/hLkbW2fyDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"47513d1d779cf78385893f11abc160646c5d393fd27c765365e25b9a7614d7ba","last_reissued_at":"2026-05-18T01:48:40.705840Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:40.705840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A relation of the PAH 3.3 um feature with star-forming activity for galaxies with a wide range of infrared luminosity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Daisuke Ishihara, Hidehiro Kaneda, Ji Hoon Kim, Mitsuyoshi Yamagishi, Myungshin Im, Rika Yamada, Shinki Oyabu","submitted_at":"2013-07-24T09:42:30Z","abstract_excerpt":"For star-forming galaxies, we investigate a global relation between polycyclic aromatic hydrocarbon (PAH) emission luminosity at 3.3 um, L_PAH3.3, and infrared (8-1000 um) luminosity, L_IR, to understand how the PAH 3.3 um feature relates to the star formation activity. With AKARI, we performed near-infrared (2.5-5 um) spectroscopy of 184 galaxies which have L_IR \\sim 10^8 - 10^13 L_sun. We classify the samples into infrared galaxies (IRGs; L_IR < 10^11 L_sun), luminous infrared galaxies (LIRGs; L_IR \\sim 10^11 -10^12 L_sun) and ultra luminous infrared galaxies (ULIRGs; L_IR > 10^12 L_sun). We"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.6356","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":"1307.6356","created_at":"2026-05-18T01:48:40.705963+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.6356v1","created_at":"2026-05-18T01:48:40.705963+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.6356","created_at":"2026-05-18T01:48:40.705963+00:00"},{"alias_kind":"pith_short_12","alias_value":"I5IT2HLXTT3Y","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"I5IT2HLXTT3YHBMJ","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"I5IT2HLX","created_at":"2026-05-18T12:27:46.883200+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.19658","citing_title":"The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs","ref_index":243,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR","json":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR.json","graph_json":"https://pith.science/api/pith-number/I5IT2HLXTT3YHBMJH4I2XQLAMR/graph.json","events_json":"https://pith.science/api/pith-number/I5IT2HLXTT3YHBMJH4I2XQLAMR/events.json","paper":"https://pith.science/paper/I5IT2HLX"},"agent_actions":{"view_html":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR","download_json":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR.json","view_paper":"https://pith.science/paper/I5IT2HLX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.6356&json=true","fetch_graph":"https://pith.science/api/pith-number/I5IT2HLXTT3YHBMJH4I2XQLAMR/graph.json","fetch_events":"https://pith.science/api/pith-number/I5IT2HLXTT3YHBMJH4I2XQLAMR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR/action/storage_attestation","attest_author":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR/action/author_attestation","sign_citation":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR/action/citation_signature","submit_replication":"https://pith.science/pith/I5IT2HLXTT3YHBMJH4I2XQLAMR/action/replication_record"}},"created_at":"2026-05-18T01:48:40.705963+00:00","updated_at":"2026-05-18T01:48:40.705963+00:00"}