{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:4TOUAHVKRHM75AKIPQQP5FMHWL","short_pith_number":"pith:4TOUAHVK","schema_version":"1.0","canonical_sha256":"e4dd401eaa89d9fe81487c20fe9587b2d35de75a5a7ddf4bb51c12a1af3f842b","source":{"kind":"arxiv","id":"1402.6315","version":2},"attestation_state":"computed","paper":{"title":"The Baryonic Tully-Fisher Relationship for S$^4$G Galaxies and the \"Condensed\" Baryon Fraction of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bosma, A. Gil de Paz, B. Holwerda, D. A. Gadotti, Dennis Zaritsky, E. Athanassoula, E. Laurikainen, Helene Courtois, H. Salo, Jenny Sorce, J. Laine, J. L. Hinz, Juan-Carlos Mu\\~noz-Mateos, K. Men\\'endez-Delmestre, K. Sheth, Luis C. Ho, M. Cisternas, M. Seibert, M. W. Regan, S. Comer\\'on, S. Erroz-Ferrer, T. Kim, T. Mizusawa","submitted_at":"2014-02-25T20:59:37Z","abstract_excerpt":"We combine data from the Spitzer Survey for Stellar Structure in Galaxies (S$^4$G), a recently calibrated empirical stellar mass estimator from Eskew et al., and an extensive database of HI spectral line profiles to examine the baryonic Tully-Fisher (BTF) relation. We find 1) that the BTF has lower scatter than the classic Tully-Fisher (TF) relation and is better described as a linear relationship, confirming similar previous results, 2) that the inclusion of a radial scale in the BTF decreases the scatter but only modestly, as seen previously for the TF relation, and 3) that the slope of the "},"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":"1402.6315","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-25T20:59:37Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"9eccb79e588d066524fbe9d43ed5d4a2b51feb1f64ca3fd5d94c90e6daffdfdf","abstract_canon_sha256":"d0dea18e65eda3cce9b61859d5986744c0ccac0fd3184bd9143f9ad67380d4c4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:27.298842Z","signature_b64":"SzIg/XRYS0vHIPhmiiPoXOp8qoN4/tKFJS0kflLrBRt+6um9O6NPeXgdjeac2ykHQQ5sj5Bret1eUParhwHECA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e4dd401eaa89d9fe81487c20fe9587b2d35de75a5a7ddf4bb51c12a1af3f842b","last_reissued_at":"2026-05-18T01:44:27.298295Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:27.298295Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Baryonic Tully-Fisher Relationship for S$^4$G Galaxies and the \"Condensed\" Baryon Fraction of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bosma, A. Gil de Paz, B. Holwerda, D. A. Gadotti, Dennis Zaritsky, E. Athanassoula, E. Laurikainen, Helene Courtois, H. Salo, Jenny Sorce, J. Laine, J. L. Hinz, Juan-Carlos Mu\\~noz-Mateos, K. Men\\'endez-Delmestre, K. Sheth, Luis C. Ho, M. Cisternas, M. Seibert, M. W. Regan, S. Comer\\'on, S. Erroz-Ferrer, T. Kim, T. Mizusawa","submitted_at":"2014-02-25T20:59:37Z","abstract_excerpt":"We combine data from the Spitzer Survey for Stellar Structure in Galaxies (S$^4$G), a recently calibrated empirical stellar mass estimator from Eskew et al., and an extensive database of HI spectral line profiles to examine the baryonic Tully-Fisher (BTF) relation. We find 1) that the BTF has lower scatter than the classic Tully-Fisher (TF) relation and is better described as a linear relationship, confirming similar previous results, 2) that the inclusion of a radial scale in the BTF decreases the scatter but only modestly, as seen previously for the TF relation, and 3) that the slope of the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.6315","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":"1402.6315","created_at":"2026-05-18T01:44:27.298386+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.6315v2","created_at":"2026-05-18T01:44:27.298386+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.6315","created_at":"2026-05-18T01:44:27.298386+00:00"},{"alias_kind":"pith_short_12","alias_value":"4TOUAHVKRHM7","created_at":"2026-05-18T12:28:14.216126+00:00"},{"alias_kind":"pith_short_16","alias_value":"4TOUAHVKRHM75AKI","created_at":"2026-05-18T12:28:14.216126+00:00"},{"alias_kind":"pith_short_8","alias_value":"4TOUAHVK","created_at":"2026-05-18T12:28:14.216126+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/4TOUAHVKRHM75AKIPQQP5FMHWL","json":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL.json","graph_json":"https://pith.science/api/pith-number/4TOUAHVKRHM75AKIPQQP5FMHWL/graph.json","events_json":"https://pith.science/api/pith-number/4TOUAHVKRHM75AKIPQQP5FMHWL/events.json","paper":"https://pith.science/paper/4TOUAHVK"},"agent_actions":{"view_html":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL","download_json":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL.json","view_paper":"https://pith.science/paper/4TOUAHVK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.6315&json=true","fetch_graph":"https://pith.science/api/pith-number/4TOUAHVKRHM75AKIPQQP5FMHWL/graph.json","fetch_events":"https://pith.science/api/pith-number/4TOUAHVKRHM75AKIPQQP5FMHWL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL/action/storage_attestation","attest_author":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL/action/author_attestation","sign_citation":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL/action/citation_signature","submit_replication":"https://pith.science/pith/4TOUAHVKRHM75AKIPQQP5FMHWL/action/replication_record"}},"created_at":"2026-05-18T01:44:27.298386+00:00","updated_at":"2026-05-18T01:44:27.298386+00:00"}