{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QLQE5YVFWYKYLIPKYU27IDMO4U","short_pith_number":"pith:QLQE5YVF","schema_version":"1.0","canonical_sha256":"82e04ee2a5b61585a1eac535f40d8ee53e62a13737a0126df9023f3470885aa2","source":{"kind":"arxiv","id":"1607.01393","version":2},"attestation_state":"computed","paper":{"title":"The Tully-Fisher Relation of COLD GASS Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alfred L. Tiley (Oxford), Am\\'elie Saintonge (UCL), Cardiff), Kazufumi Torii (Nagoya), Martin Bureau (Oxford), Selcuk Topal (Oxford), Timothy A. Davis (Hertfordshire","submitted_at":"2016-07-05T20:00:02Z","abstract_excerpt":"We present the stellar mass (M_*) and Wide-Field Infrared Survey Explorer (WISE) absolute Band 1 magnitude (M_W1) Tully-Fisher relations (TFRs) of subsets of galaxies from the CO Legacy Database for the Galex Arecibo SDSS Survey (COLD GASS). We examine the benefits and drawbacks of several commonly used fitting functions in the context of measuring CO(1-0) line widths (and thus rotation velocities), favouring the Gaussian Double Peak function. We find the M_W1 and M_* TFR, for a carefully selected sub-sample, to be M_W1 = (-7.1 +/- 0.6) [log(W_50/sin i) - 2.58] - 23.83 +/- 0.09 and log(M_*/M_S"},"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":"1607.01393","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-07-05T20:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"e31b40e99ccd09e13955fda28f9ebe05be744d933689295287f63c7fbf364879","abstract_canon_sha256":"bcc0253dd994a8b51854a170401989869d82eb41f2027b2b49371d63b8909f1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:16.964879Z","signature_b64":"dxaH4/sKQY0j2ZK2QdlHjERLQtvU6dhudMC88VZjJ6YbXK7CQCFQgorKsOYeZyGgJ1u8h5nYrqCltSX5cWz4DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"82e04ee2a5b61585a1eac535f40d8ee53e62a13737a0126df9023f3470885aa2","last_reissued_at":"2026-05-18T01:11:16.964222Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:16.964222Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Tully-Fisher Relation of COLD GASS Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alfred L. Tiley (Oxford), Am\\'elie Saintonge (UCL), Cardiff), Kazufumi Torii (Nagoya), Martin Bureau (Oxford), Selcuk Topal (Oxford), Timothy A. Davis (Hertfordshire","submitted_at":"2016-07-05T20:00:02Z","abstract_excerpt":"We present the stellar mass (M_*) and Wide-Field Infrared Survey Explorer (WISE) absolute Band 1 magnitude (M_W1) Tully-Fisher relations (TFRs) of subsets of galaxies from the CO Legacy Database for the Galex Arecibo SDSS Survey (COLD GASS). We examine the benefits and drawbacks of several commonly used fitting functions in the context of measuring CO(1-0) line widths (and thus rotation velocities), favouring the Gaussian Double Peak function. We find the M_W1 and M_* TFR, for a carefully selected sub-sample, to be M_W1 = (-7.1 +/- 0.6) [log(W_50/sin i) - 2.58] - 23.83 +/- 0.09 and log(M_*/M_S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1607.01393","kind":"arxiv","version":2},"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":"1607.01393","created_at":"2026-05-18T01:11:16.964347+00:00"},{"alias_kind":"arxiv_version","alias_value":"1607.01393v2","created_at":"2026-05-18T01:11:16.964347+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1607.01393","created_at":"2026-05-18T01:11:16.964347+00:00"},{"alias_kind":"pith_short_12","alias_value":"QLQE5YVFWYKY","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"QLQE5YVFWYKYLIPK","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"QLQE5YVF","created_at":"2026-05-18T12:30:39.010887+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/QLQE5YVFWYKYLIPKYU27IDMO4U","json":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U.json","graph_json":"https://pith.science/api/pith-number/QLQE5YVFWYKYLIPKYU27IDMO4U/graph.json","events_json":"https://pith.science/api/pith-number/QLQE5YVFWYKYLIPKYU27IDMO4U/events.json","paper":"https://pith.science/paper/QLQE5YVF"},"agent_actions":{"view_html":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U","download_json":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U.json","view_paper":"https://pith.science/paper/QLQE5YVF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1607.01393&json=true","fetch_graph":"https://pith.science/api/pith-number/QLQE5YVFWYKYLIPKYU27IDMO4U/graph.json","fetch_events":"https://pith.science/api/pith-number/QLQE5YVFWYKYLIPKYU27IDMO4U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U/action/storage_attestation","attest_author":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U/action/author_attestation","sign_citation":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U/action/citation_signature","submit_replication":"https://pith.science/pith/QLQE5YVFWYKYLIPKYU27IDMO4U/action/replication_record"}},"created_at":"2026-05-18T01:11:16.964347+00:00","updated_at":"2026-05-18T01:11:16.964347+00:00"}