{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NPFXUPGJLNHNKWR3JTIVRC2UDD","short_pith_number":"pith:NPFXUPGJ","schema_version":"1.0","canonical_sha256":"6bcb7a3cc95b4ed55a3b4cd1588b5418f57848ed829c3cc8cd009c341e59fdc2","source":{"kind":"arxiv","id":"1602.07870","version":1},"attestation_state":"computed","paper":{"title":"Search for Hyper Infrared-Luminous Dust Obscured Galaxies selected with WISE and SDSS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Tohru Nagao, Yoshiki Toba","submitted_at":"2016-02-25T10:23:10Z","abstract_excerpt":"We aim to search for hyperliminous infrared (IR) galaxies (HyLIRGs) with IR luminosity $L_{{\\rm IR}}$ $>$ 10$^{13}$ $L_{\\odot}$ by applying the selection method of Dust Obscured Galaxies (DOGs). They are spatially rare but could correspond to a maximum phase of cosmic star formation and/or active galactic nucleus (AGN) activity, hence they are a crucial population for understanding the star formation and mass assembly history of galaxies. Combining the optical and IR catalogs obtained from Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE), we performed the extensiv"},"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":"1602.07870","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-25T10:23:10Z","cross_cats_sorted":[],"title_canon_sha256":"53c3850b748ca147ebedd393b23a088e4e57751443949becd01733519a7ef8f8","abstract_canon_sha256":"dbf177e5f90577cbe413ddc06fc201aadea7271bbd305282241f43143618cff5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:28.831774Z","signature_b64":"iTQjjrLNCA3o1dE/R0AjD6F12V/u66r33+N3G1Y6ScpyDXkkq8RCA+wTnof/hshIjT7PDdMs4joI/8aC0Z+hCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6bcb7a3cc95b4ed55a3b4cd1588b5418f57848ed829c3cc8cd009c341e59fdc2","last_reissued_at":"2026-05-18T01:18:28.831166Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:28.831166Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for Hyper Infrared-Luminous Dust Obscured Galaxies selected with WISE and SDSS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Tohru Nagao, Yoshiki Toba","submitted_at":"2016-02-25T10:23:10Z","abstract_excerpt":"We aim to search for hyperliminous infrared (IR) galaxies (HyLIRGs) with IR luminosity $L_{{\\rm IR}}$ $>$ 10$^{13}$ $L_{\\odot}$ by applying the selection method of Dust Obscured Galaxies (DOGs). They are spatially rare but could correspond to a maximum phase of cosmic star formation and/or active galactic nucleus (AGN) activity, hence they are a crucial population for understanding the star formation and mass assembly history of galaxies. Combining the optical and IR catalogs obtained from Sloan Digital Sky Survey (SDSS) and Wide-field Infrared Survey Explorer (WISE), we performed the extensiv"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.07870","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":"1602.07870","created_at":"2026-05-18T01:18:28.831256+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.07870v1","created_at":"2026-05-18T01:18:28.831256+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.07870","created_at":"2026-05-18T01:18:28.831256+00:00"},{"alias_kind":"pith_short_12","alias_value":"NPFXUPGJLNHN","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"NPFXUPGJLNHNKWR3","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"NPFXUPGJ","created_at":"2026-05-18T12:30:36.002864+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/NPFXUPGJLNHNKWR3JTIVRC2UDD","json":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD.json","graph_json":"https://pith.science/api/pith-number/NPFXUPGJLNHNKWR3JTIVRC2UDD/graph.json","events_json":"https://pith.science/api/pith-number/NPFXUPGJLNHNKWR3JTIVRC2UDD/events.json","paper":"https://pith.science/paper/NPFXUPGJ"},"agent_actions":{"view_html":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD","download_json":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD.json","view_paper":"https://pith.science/paper/NPFXUPGJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.07870&json=true","fetch_graph":"https://pith.science/api/pith-number/NPFXUPGJLNHNKWR3JTIVRC2UDD/graph.json","fetch_events":"https://pith.science/api/pith-number/NPFXUPGJLNHNKWR3JTIVRC2UDD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD/action/storage_attestation","attest_author":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD/action/author_attestation","sign_citation":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD/action/citation_signature","submit_replication":"https://pith.science/pith/NPFXUPGJLNHNKWR3JTIVRC2UDD/action/replication_record"}},"created_at":"2026-05-18T01:18:28.831256+00:00","updated_at":"2026-05-18T01:18:28.831256+00:00"}