{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3CZFFCEQUDLNH4ABGT2XRDAFXO","short_pith_number":"pith:3CZFFCEQ","schema_version":"1.0","canonical_sha256":"d8b2528890a0d6d3f00134f5788c05bb90d844bd63eb6cf8bc9136cb9ccb8645","source":{"kind":"arxiv","id":"1704.03655","version":1},"attestation_state":"computed","paper":{"title":"Far-infrared properties of infrared bright dust-obscured galaxies selected with IRAS and AKARI far-infrared all-sky survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hideo Matsuhara, Issei Yamamura, Masayuki Akiyama, Tohru Nagao, Tomotsugu Goto, Wei-hao Wang, Yoshiki Toba, Youich Ohyama, Yusei Koyama","submitted_at":"2017-04-12T08:15:21Z","abstract_excerpt":"We investigate the star forming activity of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that show an extreme red color in the optical and IR regime, $(i - [22])_{\\rm AB} > 7.0$. Combining an IR-bright DOG sample with the flux at 22 $\\mu$m $>$ 3.8 mJy discovered by Toba & Nagao (2016) with IRAS faint source catalog version 2 and AKARI far-IR (FIR) all-sky survey bright source catalog version 2, we selected 109 DOGs with FIR data. For a subsample of 7 IR-bright DOGs with spectroscopic redshift ($0.07 < z < 1.0$) that was obtained from literature, we estimated their IR luminosi"},"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":"1704.03655","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-12T08:15:21Z","cross_cats_sorted":[],"title_canon_sha256":"eec4656c61f003dfde5452e2fc16b66f371b0858692a96bf708616bf56248045","abstract_canon_sha256":"1382cdac8b105bbcebe60a36447f54b84d93f6cd435ccb8d9253005de21a04f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:44:51.139465Z","signature_b64":"wqmkJh0fBSBWN0K/4KrEVPYzsgJeopGG5zXXna5ifRO7sSXMp82XnZU0yNm434fKrv8fCq/vkf+m8+3Y+jFKDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d8b2528890a0d6d3f00134f5788c05bb90d844bd63eb6cf8bc9136cb9ccb8645","last_reissued_at":"2026-05-18T00:44:51.138828Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:44:51.138828Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Far-infrared properties of infrared bright dust-obscured galaxies selected with IRAS and AKARI far-infrared all-sky survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hideo Matsuhara, Issei Yamamura, Masayuki Akiyama, Tohru Nagao, Tomotsugu Goto, Wei-hao Wang, Yoshiki Toba, Youich Ohyama, Yusei Koyama","submitted_at":"2017-04-12T08:15:21Z","abstract_excerpt":"We investigate the star forming activity of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that show an extreme red color in the optical and IR regime, $(i - [22])_{\\rm AB} > 7.0$. Combining an IR-bright DOG sample with the flux at 22 $\\mu$m $>$ 3.8 mJy discovered by Toba & Nagao (2016) with IRAS faint source catalog version 2 and AKARI far-IR (FIR) all-sky survey bright source catalog version 2, we selected 109 DOGs with FIR data. For a subsample of 7 IR-bright DOGs with spectroscopic redshift ($0.07 < z < 1.0$) that was obtained from literature, we estimated their IR luminosi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.03655","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":"1704.03655","created_at":"2026-05-18T00:44:51.138920+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.03655v1","created_at":"2026-05-18T00:44:51.138920+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.03655","created_at":"2026-05-18T00:44:51.138920+00:00"},{"alias_kind":"pith_short_12","alias_value":"3CZFFCEQUDLN","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3CZFFCEQUDLNH4AB","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3CZFFCEQ","created_at":"2026-05-18T12:30:58.224056+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/3CZFFCEQUDLNH4ABGT2XRDAFXO","json":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO.json","graph_json":"https://pith.science/api/pith-number/3CZFFCEQUDLNH4ABGT2XRDAFXO/graph.json","events_json":"https://pith.science/api/pith-number/3CZFFCEQUDLNH4ABGT2XRDAFXO/events.json","paper":"https://pith.science/paper/3CZFFCEQ"},"agent_actions":{"view_html":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO","download_json":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO.json","view_paper":"https://pith.science/paper/3CZFFCEQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.03655&json=true","fetch_graph":"https://pith.science/api/pith-number/3CZFFCEQUDLNH4ABGT2XRDAFXO/graph.json","fetch_events":"https://pith.science/api/pith-number/3CZFFCEQUDLNH4ABGT2XRDAFXO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO/action/storage_attestation","attest_author":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO/action/author_attestation","sign_citation":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO/action/citation_signature","submit_replication":"https://pith.science/pith/3CZFFCEQUDLNH4ABGT2XRDAFXO/action/replication_record"}},"created_at":"2026-05-18T00:44:51.138920+00:00","updated_at":"2026-05-18T00:44:51.138920+00:00"}