{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:Q5YHN2PEB2SXQLHYFKZVESEXSJ","short_pith_number":"pith:Q5YHN2PE","schema_version":"1.0","canonical_sha256":"877076e9e40ea5782cf82ab352489792479aaab50246f6ff4487b94174407396","source":{"kind":"arxiv","id":"1602.06739","version":1},"attestation_state":"computed","paper":{"title":"A quality check of the $AKARI$ mid-infrared all-sky diffuse map toward the massive star-forming regions NGC 6334 and NGC 6357","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Daisuke Ishihara, Hidehiro Kaneda, Hidetoshi Sano, Keichiro Nakamichi, Kengo Tachihara, Mitsuyoshi Yamagishi, Shinki Oyabu, Tomoya Amatsutsu, Toru Kondo, Yasuo Fukui","submitted_at":"2016-02-22T11:41:36Z","abstract_excerpt":"We present a comparative study of CO and polycyclic aromatic hydrocarbon (PAH) emission toward a region including the massive star-forming regions of NGC 6334 and NGC 6357. We use the NANTEN $^{12}$CO($J$ = 1--0) data and the $AKARI$ 9 $\\mu$m All-Sky diffuse map in order to evaluate the calibration accuracy of the $AKARI$ data. We confirm that the overall CO distribution shows a good spatial correspondence with the PAH emission, and their intensities exhibit a good power-law correlation with a spatial resolution down to 4$'$ over the region of 10$^\\circ$$\\times$10$^\\circ$. We also reveal poore"},"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":"1602.06739","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-22T11:41:36Z","cross_cats_sorted":[],"title_canon_sha256":"102e9f29785f3d8d4d15350faaad67aaed4d458661cc81f9e176ac23ba925d61","abstract_canon_sha256":"95cf085ef535e5ba0ab5ceee933eca92b5b8a4c3c32f2339f42a706c3d18d2e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:13.243654Z","signature_b64":"q4GXIErIT2488kG1MaYDMdXttvFBwDOxad3vhSBQJiYRbPOft5FP/AMTIAB1YXs1s2Cgy/1SftKdJQJLu3iwAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"877076e9e40ea5782cf82ab352489792479aaab50246f6ff4487b94174407396","last_reissued_at":"2026-05-18T01:20:13.242992Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:13.242992Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A quality check of the $AKARI$ mid-infrared all-sky diffuse map toward the massive star-forming regions NGC 6334 and NGC 6357","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Daisuke Ishihara, Hidehiro Kaneda, Hidetoshi Sano, Keichiro Nakamichi, Kengo Tachihara, Mitsuyoshi Yamagishi, Shinki Oyabu, Tomoya Amatsutsu, Toru Kondo, Yasuo Fukui","submitted_at":"2016-02-22T11:41:36Z","abstract_excerpt":"We present a comparative study of CO and polycyclic aromatic hydrocarbon (PAH) emission toward a region including the massive star-forming regions of NGC 6334 and NGC 6357. We use the NANTEN $^{12}$CO($J$ = 1--0) data and the $AKARI$ 9 $\\mu$m All-Sky diffuse map in order to evaluate the calibration accuracy of the $AKARI$ data. We confirm that the overall CO distribution shows a good spatial correspondence with the PAH emission, and their intensities exhibit a good power-law correlation with a spatial resolution down to 4$'$ over the region of 10$^\\circ$$\\times$10$^\\circ$. We also reveal poore"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.06739","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":"1602.06739","created_at":"2026-05-18T01:20:13.243106+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.06739v1","created_at":"2026-05-18T01:20:13.243106+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.06739","created_at":"2026-05-18T01:20:13.243106+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q5YHN2PEB2SX","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q5YHN2PEB2SXQLHY","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q5YHN2PE","created_at":"2026-05-18T12:30:39.010887+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/Q5YHN2PEB2SXQLHYFKZVESEXSJ","json":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ.json","graph_json":"https://pith.science/api/pith-number/Q5YHN2PEB2SXQLHYFKZVESEXSJ/graph.json","events_json":"https://pith.science/api/pith-number/Q5YHN2PEB2SXQLHYFKZVESEXSJ/events.json","paper":"https://pith.science/paper/Q5YHN2PE"},"agent_actions":{"view_html":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ","download_json":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ.json","view_paper":"https://pith.science/paper/Q5YHN2PE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.06739&json=true","fetch_graph":"https://pith.science/api/pith-number/Q5YHN2PEB2SXQLHYFKZVESEXSJ/graph.json","fetch_events":"https://pith.science/api/pith-number/Q5YHN2PEB2SXQLHYFKZVESEXSJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ/action/storage_attestation","attest_author":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ/action/author_attestation","sign_citation":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ/action/citation_signature","submit_replication":"https://pith.science/pith/Q5YHN2PEB2SXQLHYFKZVESEXSJ/action/replication_record"}},"created_at":"2026-05-18T01:20:13.243106+00:00","updated_at":"2026-05-18T01:20:13.243106+00:00"}