{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:6TLA4UATFFZNBUVSUBNM4HB67W","short_pith_number":"pith:6TLA4UAT","schema_version":"1.0","canonical_sha256":"f4d60e50132972d0d2b2a05ace1c3efdaf960fe6d4c61ccf2a90be2c3f7f8d2f","source":{"kind":"arxiv","id":"astro-ph/0007005","version":1},"attestation_state":"computed","paper":{"title":"CO Observations of Luminous IR Galaxies at Intermediate Redshift","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"K. Wakamatsu, M. Honma, T. Ichikawa, Y. Sofue, Y. Tutui","submitted_at":"2000-07-01T15:23:25Z","abstract_excerpt":"We present new measurement of $^{12}$CO($J=1-0$) emission from 16 luminous infrared galaxies (LIGs) at intermediate redshift ($cz \\sim 10,000 - 50,000 {\\rm km s^{-1}}$). These new data were selected by isolated and normal morphology. The CO observations were performed using the NRO 45-m telescope. Comparison of the CO and dust properties of the new result with those from other CO measurements revealed characteristics of this sample: (1) It is the deepest CO observations of IRAS galaxies at intermediate redshift without strong interaction features. (2) It has typical properties of normal IRAS g"},"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":"astro-ph/0007005","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-07-01T15:23:25Z","cross_cats_sorted":[],"title_canon_sha256":"05b8aac89da433a1b05e17da8c2ad56ea212b06411dd3fab0274333d57711bd2","abstract_canon_sha256":"425163bcb773810b18dd1791692ea2d7c29c0d2d1bec6121ce02d8a749c68baf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:47.596609Z","signature_b64":"ODe7MGe676fehJ+KlzhAHO26900UI4YAw30s7tvqzsoniNE3xJvnkFFaK0yJ0dAh8fAC1U+kq7sVE/htIxXdDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f4d60e50132972d0d2b2a05ace1c3efdaf960fe6d4c61ccf2a90be2c3f7f8d2f","last_reissued_at":"2026-05-18T01:40:47.596106Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:47.596106Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CO Observations of Luminous IR Galaxies at Intermediate Redshift","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"K. Wakamatsu, M. Honma, T. Ichikawa, Y. Sofue, Y. Tutui","submitted_at":"2000-07-01T15:23:25Z","abstract_excerpt":"We present new measurement of $^{12}$CO($J=1-0$) emission from 16 luminous infrared galaxies (LIGs) at intermediate redshift ($cz \\sim 10,000 - 50,000 {\\rm km s^{-1}}$). These new data were selected by isolated and normal morphology. The CO observations were performed using the NRO 45-m telescope. Comparison of the CO and dust properties of the new result with those from other CO measurements revealed characteristics of this sample: (1) It is the deepest CO observations of IRAS galaxies at intermediate redshift without strong interaction features. (2) It has typical properties of normal IRAS g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0007005","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":"astro-ph/0007005","created_at":"2026-05-18T01:40:47.596185+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0007005v1","created_at":"2026-05-18T01:40:47.596185+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0007005","created_at":"2026-05-18T01:40:47.596185+00:00"},{"alias_kind":"pith_short_12","alias_value":"6TLA4UATFFZN","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_16","alias_value":"6TLA4UATFFZNBUVS","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_8","alias_value":"6TLA4UAT","created_at":"2026-05-18T12:25:49.631198+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/6TLA4UATFFZNBUVSUBNM4HB67W","json":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W.json","graph_json":"https://pith.science/api/pith-number/6TLA4UATFFZNBUVSUBNM4HB67W/graph.json","events_json":"https://pith.science/api/pith-number/6TLA4UATFFZNBUVSUBNM4HB67W/events.json","paper":"https://pith.science/paper/6TLA4UAT"},"agent_actions":{"view_html":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W","download_json":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W.json","view_paper":"https://pith.science/paper/6TLA4UAT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0007005&json=true","fetch_graph":"https://pith.science/api/pith-number/6TLA4UATFFZNBUVSUBNM4HB67W/graph.json","fetch_events":"https://pith.science/api/pith-number/6TLA4UATFFZNBUVSUBNM4HB67W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W/action/storage_attestation","attest_author":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W/action/author_attestation","sign_citation":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W/action/citation_signature","submit_replication":"https://pith.science/pith/6TLA4UATFFZNBUVSUBNM4HB67W/action/replication_record"}},"created_at":"2026-05-18T01:40:47.596185+00:00","updated_at":"2026-05-18T01:40:47.596185+00:00"}