{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:TDCGA4BUVW4YLDF4D75WGW7PHO","short_pith_number":"pith:TDCGA4BU","schema_version":"1.0","canonical_sha256":"98c4607034adb9858cbc1ffb635bef3bbe3c40b8659582db93d19273233ca9bc","source":{"kind":"arxiv","id":"1408.1786","version":1},"attestation_state":"computed","paper":{"title":"The 2 to 24 micron source counts from the AKARI North Ecliptic Pole survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C.P. Pearson, H. Matsuhara, K. Murata, S.J. Kim, T. Goto, T. Wada","submitted_at":"2014-08-08T08:40:53Z","abstract_excerpt":"We present herein galaxy number counts of the nine bands in the 2-24 micron range on the basis of the AKARI North Ecliptic Pole (NEP) surveys. The number counts are derived from NEP-deep and NEP-wide surveys, which cover areas of 0.5 and 5.8 deg2, respectively. To produce reliable number counts, the sources were extracted from recently updated images. Completeness and difference between observed and intrinsic magnitudes were corrected by Monte Carlo simulation. Stellar counts were subtracted by using the stellar fraction estimated from optical data. The resultant source counts are given down t"},"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":"1408.1786","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-08-08T08:40:53Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"f02a4a1e3843a0a16c0a584315edcef04571af29312bb1adf06357636068bcec","abstract_canon_sha256":"cf6680ceadb4695fd5fef3678a7297699c10423f3343a74f42f703fa97bd1140"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:22.639126Z","signature_b64":"kQ6+I/nSvxLCMYw7PhWEpEgKIkZS6QDqNRa6xqyMJzvUhdVEkuWh+/Y9mpYG6eBpTAjDguLzW3Lqod1MSXx8BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98c4607034adb9858cbc1ffb635bef3bbe3c40b8659582db93d19273233ca9bc","last_reissued_at":"2026-05-18T01:42:22.638668Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:22.638668Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The 2 to 24 micron source counts from the AKARI North Ecliptic Pole survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C.P. Pearson, H. Matsuhara, K. Murata, S.J. Kim, T. Goto, T. Wada","submitted_at":"2014-08-08T08:40:53Z","abstract_excerpt":"We present herein galaxy number counts of the nine bands in the 2-24 micron range on the basis of the AKARI North Ecliptic Pole (NEP) surveys. The number counts are derived from NEP-deep and NEP-wide surveys, which cover areas of 0.5 and 5.8 deg2, respectively. To produce reliable number counts, the sources were extracted from recently updated images. Completeness and difference between observed and intrinsic magnitudes were corrected by Monte Carlo simulation. Stellar counts were subtracted by using the stellar fraction estimated from optical data. The resultant source counts are given down t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.1786","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":"1408.1786","created_at":"2026-05-18T01:42:22.638734+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.1786v1","created_at":"2026-05-18T01:42:22.638734+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.1786","created_at":"2026-05-18T01:42:22.638734+00:00"},{"alias_kind":"pith_short_12","alias_value":"TDCGA4BUVW4Y","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"TDCGA4BUVW4YLDF4","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"TDCGA4BU","created_at":"2026-05-18T12:28:49.207871+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/TDCGA4BUVW4YLDF4D75WGW7PHO","json":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO.json","graph_json":"https://pith.science/api/pith-number/TDCGA4BUVW4YLDF4D75WGW7PHO/graph.json","events_json":"https://pith.science/api/pith-number/TDCGA4BUVW4YLDF4D75WGW7PHO/events.json","paper":"https://pith.science/paper/TDCGA4BU"},"agent_actions":{"view_html":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO","download_json":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO.json","view_paper":"https://pith.science/paper/TDCGA4BU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.1786&json=true","fetch_graph":"https://pith.science/api/pith-number/TDCGA4BUVW4YLDF4D75WGW7PHO/graph.json","fetch_events":"https://pith.science/api/pith-number/TDCGA4BUVW4YLDF4D75WGW7PHO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO/action/storage_attestation","attest_author":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO/action/author_attestation","sign_citation":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO/action/citation_signature","submit_replication":"https://pith.science/pith/TDCGA4BUVW4YLDF4D75WGW7PHO/action/replication_record"}},"created_at":"2026-05-18T01:42:22.638734+00:00","updated_at":"2026-05-18T01:42:22.638734+00:00"}