{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:YALXL6R4XGSUFANZR27ECTLWYR","short_pith_number":"pith:YALXL6R4","schema_version":"1.0","canonical_sha256":"c01775fa3cb9a54281b98ebe414d76c45137095b99d47bd3a00ccaecb4d34517","source":{"kind":"arxiv","id":"astro-ph/9607024","version":3},"attestation_state":"computed","paper":{"title":"Distance Measurement of Galaxies to Redshift of 0.1 using the CO-Line Tully-Fisher Relation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Schoeniger, I. Kazes, J. Dickey, K. Wakamatsu, M. Honma, T. Ichikawa, Y. Sofue, Y. Tutui","submitted_at":"1996-07-04T03:02:00Z","abstract_excerpt":"We report on the first results of a long-term project to derive distances of galaxies at cosmological distances by applying the CO-line width-luminosity relation. We have obtained deep CO-line observations of galaxies at redshifts up to 29,000 km/s using the Nobeyama 45-m mm-wave Telescope, and some supplementary data were obtained by using the IRAM 30-m telescope. We have detected the CO line emission for several galaxies, and used their CO line widths to estimate the absolute luminosities using the line-width-luminosity relation. In order to obtain photometric data and inclination correction"},"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/9607024","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-04T03:02:00Z","cross_cats_sorted":[],"title_canon_sha256":"a2671d57cc2246e23f15f9425ea89c00c90e79a3177f1a937a3d5aa205dccf1d","abstract_canon_sha256":"e17ccd6a09b8e1dded21877ec25eb5a9f596bedda44083c96d02639a24d80810"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:19.774252Z","signature_b64":"bbR7YFiHJhQEzv5s2ucFBWlZBTFNwTRiekwRGetbLQwcUG06fprcVR6McgsXYcCHW3XdRzij+nr7YZ6hOpo0CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c01775fa3cb9a54281b98ebe414d76c45137095b99d47bd3a00ccaecb4d34517","last_reissued_at":"2026-05-18T01:40:19.773837Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:19.773837Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Distance Measurement of Galaxies to Redshift of 0.1 using the CO-Line Tully-Fisher Relation","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Schoeniger, I. Kazes, J. Dickey, K. Wakamatsu, M. Honma, T. Ichikawa, Y. Sofue, Y. Tutui","submitted_at":"1996-07-04T03:02:00Z","abstract_excerpt":"We report on the first results of a long-term project to derive distances of galaxies at cosmological distances by applying the CO-line width-luminosity relation. We have obtained deep CO-line observations of galaxies at redshifts up to 29,000 km/s using the Nobeyama 45-m mm-wave Telescope, and some supplementary data were obtained by using the IRAM 30-m telescope. We have detected the CO line emission for several galaxies, and used their CO line widths to estimate the absolute luminosities using the line-width-luminosity relation. In order to obtain photometric data and inclination correction"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9607024","kind":"arxiv","version":3},"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/9607024","created_at":"2026-05-18T01:40:19.773889+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9607024v3","created_at":"2026-05-18T01:40:19.773889+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9607024","created_at":"2026-05-18T01:40:19.773889+00:00"},{"alias_kind":"pith_short_12","alias_value":"YALXL6R4XGSU","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_16","alias_value":"YALXL6R4XGSUFANZ","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_8","alias_value":"YALXL6R4","created_at":"2026-05-18T12:25:48.327863+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/YALXL6R4XGSUFANZR27ECTLWYR","json":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR.json","graph_json":"https://pith.science/api/pith-number/YALXL6R4XGSUFANZR27ECTLWYR/graph.json","events_json":"https://pith.science/api/pith-number/YALXL6R4XGSUFANZR27ECTLWYR/events.json","paper":"https://pith.science/paper/YALXL6R4"},"agent_actions":{"view_html":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR","download_json":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR.json","view_paper":"https://pith.science/paper/YALXL6R4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9607024&json=true","fetch_graph":"https://pith.science/api/pith-number/YALXL6R4XGSUFANZR27ECTLWYR/graph.json","fetch_events":"https://pith.science/api/pith-number/YALXL6R4XGSUFANZR27ECTLWYR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR/action/storage_attestation","attest_author":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR/action/author_attestation","sign_citation":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR/action/citation_signature","submit_replication":"https://pith.science/pith/YALXL6R4XGSUFANZR27ECTLWYR/action/replication_record"}},"created_at":"2026-05-18T01:40:19.773889+00:00","updated_at":"2026-05-18T01:40:19.773889+00:00"}