{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:O5W6KIPTRT6OJDSLYDP7U6VTIM","short_pith_number":"pith:O5W6KIPT","schema_version":"1.0","canonical_sha256":"776de521f38cfce48e4bc0dffa7ab3431912301ae3ac903fa7c50c5125d132a8","source":{"kind":"arxiv","id":"1609.08534","version":1},"attestation_state":"computed","paper":{"title":"Variation Of The Tully-Fisher Relation As A Function Of The Magnitude Interval Of A Sample Of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. M. Garc\\'ia, A. Nigoche-Netro, A. Ruelas-Mayorga, J. Echevarr\\'ia, J. Ram\\'irez-V\\'elez, L. J. S\\'anchez, M. Trujillo-Lara","submitted_at":"2016-09-27T17:02:54Z","abstract_excerpt":"In this paper we carry out a preliminary study of the dependence of the Tully-Fisher Relation (TFR) with the width and intensity level of the absolute magnitude interval of a limited sample of 2411 galaxies taken from Mathewson \\& Ford (1996). The galaxies in this sample do not differ significantly in morphological type, and are distributed over an $\\sim11$-magnitude interval ($-24.4 < I < -13.0$). We take as directives the papers by Nigoche-Netro et al. (2008, 2009, 2010) in which they study the dependence of the Kormendy (KR), the Fundamental Plane (FPR) and the Faber-Jackson Relations (FJR)"},"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":"1609.08534","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-09-27T17:02:54Z","cross_cats_sorted":[],"title_canon_sha256":"4f6ae7d21db0de533c4dbcd4c1463c5671ddcdf3ef557e76bcb340180cdf52f8","abstract_canon_sha256":"4979250163f93acb97faed58e6adc8838029c5db3c748571b1cf064825733c55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:45.695945Z","signature_b64":"ywnXkRmJVQIg6/NccY4/UzngV78+xnP6GyZmtCo+Rj9hsNgPYeVxiytp8DC/lBq4OqJ75qoBzkA+x0g2n/fYAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"776de521f38cfce48e4bc0dffa7ab3431912301ae3ac903fa7c50c5125d132a8","last_reissued_at":"2026-05-18T01:03:45.695485Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:45.695485Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Variation Of The Tully-Fisher Relation As A Function Of The Magnitude Interval Of A Sample Of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. M. Garc\\'ia, A. Nigoche-Netro, A. Ruelas-Mayorga, J. Echevarr\\'ia, J. Ram\\'irez-V\\'elez, L. J. S\\'anchez, M. Trujillo-Lara","submitted_at":"2016-09-27T17:02:54Z","abstract_excerpt":"In this paper we carry out a preliminary study of the dependence of the Tully-Fisher Relation (TFR) with the width and intensity level of the absolute magnitude interval of a limited sample of 2411 galaxies taken from Mathewson \\& Ford (1996). The galaxies in this sample do not differ significantly in morphological type, and are distributed over an $\\sim11$-magnitude interval ($-24.4 < I < -13.0$). We take as directives the papers by Nigoche-Netro et al. (2008, 2009, 2010) in which they study the dependence of the Kormendy (KR), the Fundamental Plane (FPR) and the Faber-Jackson Relations (FJR)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.08534","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":"1609.08534","created_at":"2026-05-18T01:03:45.695560+00:00"},{"alias_kind":"arxiv_version","alias_value":"1609.08534v1","created_at":"2026-05-18T01:03:45.695560+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.08534","created_at":"2026-05-18T01:03:45.695560+00:00"},{"alias_kind":"pith_short_12","alias_value":"O5W6KIPTRT6O","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"O5W6KIPTRT6OJDSL","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"O5W6KIPT","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/O5W6KIPTRT6OJDSLYDP7U6VTIM","json":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM.json","graph_json":"https://pith.science/api/pith-number/O5W6KIPTRT6OJDSLYDP7U6VTIM/graph.json","events_json":"https://pith.science/api/pith-number/O5W6KIPTRT6OJDSLYDP7U6VTIM/events.json","paper":"https://pith.science/paper/O5W6KIPT"},"agent_actions":{"view_html":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM","download_json":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM.json","view_paper":"https://pith.science/paper/O5W6KIPT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1609.08534&json=true","fetch_graph":"https://pith.science/api/pith-number/O5W6KIPTRT6OJDSLYDP7U6VTIM/graph.json","fetch_events":"https://pith.science/api/pith-number/O5W6KIPTRT6OJDSLYDP7U6VTIM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM/action/storage_attestation","attest_author":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM/action/author_attestation","sign_citation":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM/action/citation_signature","submit_replication":"https://pith.science/pith/O5W6KIPTRT6OJDSLYDP7U6VTIM/action/replication_record"}},"created_at":"2026-05-18T01:03:45.695560+00:00","updated_at":"2026-05-18T01:03:45.695560+00:00"}