{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:ZMSQUFCNGUZTPNHIY3RVYBPM4E","short_pith_number":"pith:ZMSQUFCN","schema_version":"1.0","canonical_sha256":"cb250a144d353337b4e8c6e35c05ece101bae8f29c1d73457333cc930bd26325","source":{"kind":"arxiv","id":"astro-ph/0609736","version":1},"attestation_state":"computed","paper":{"title":"Improved $u'g'r'i'z'$ to $UBVR_CI_C$ Transformation Equations for Main Sequence Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Christopher T. Rodgers, Douglas L. Tucker, J. Allyn Smith, Michael J. Pierce, Ron Canterna","submitted_at":"2006-09-27T05:45:02Z","abstract_excerpt":"We report improved transformation equations between the $u'g'r'i'z'$ and $UBVR_CI_C$ photometric systems. Although the details of the transformations depend on luminosity class, we find a typical rms scatter on the order of 0.001 magnitude if the sample is limited to main sequence stars. Furthermore, we find an accurate transformation requires complex, multi-color dependencies for the bluer bandpasses. Results for giant stars will be reported in a subsequent paper."},"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/0609736","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-27T05:45:02Z","cross_cats_sorted":[],"title_canon_sha256":"372461705741d6864213f1a339ed4ad2020326733cc259f34243ffeebb39e060","abstract_canon_sha256":"9e04f966baf9b792ac994f359e45d455093383106b9dbf737cc04e98841c77a4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:25:55.859028Z","signature_b64":"wC+zJAkok3YdhIhr/lrIvBs8LFGx8vLuU3czGAzDhaET1gcFXNFThypztismUxHGzjqKDifHQUWXZCbTSgGvBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cb250a144d353337b4e8c6e35c05ece101bae8f29c1d73457333cc930bd26325","last_reissued_at":"2026-07-04T15:25:55.858505Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:25:55.858505Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Improved $u'g'r'i'z'$ to $UBVR_CI_C$ Transformation Equations for Main Sequence Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Christopher T. Rodgers, Douglas L. Tucker, J. Allyn Smith, Michael J. Pierce, Ron Canterna","submitted_at":"2006-09-27T05:45:02Z","abstract_excerpt":"We report improved transformation equations between the $u'g'r'i'z'$ and $UBVR_CI_C$ photometric systems. Although the details of the transformations depend on luminosity class, we find a typical rms scatter on the order of 0.001 magnitude if the sample is limited to main sequence stars. Furthermore, we find an accurate transformation requires complex, multi-color dependencies for the bluer bandpasses. Results for giant stars will be reported in a subsequent paper."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609736","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0609736/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0609736","created_at":"2026-07-04T15:25:55.858559+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609736v1","created_at":"2026-07-04T15:25:55.858559+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609736","created_at":"2026-07-04T15:25:55.858559+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZMSQUFCNGUZT","created_at":"2026-07-04T15:25:55.858559+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZMSQUFCNGUZTPNHI","created_at":"2026-07-04T15:25:55.858559+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZMSQUFCN","created_at":"2026-07-04T15:25:55.858559+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/ZMSQUFCNGUZTPNHIY3RVYBPM4E","json":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E.json","graph_json":"https://pith.science/api/pith-number/ZMSQUFCNGUZTPNHIY3RVYBPM4E/graph.json","events_json":"https://pith.science/api/pith-number/ZMSQUFCNGUZTPNHIY3RVYBPM4E/events.json","paper":"https://pith.science/paper/ZMSQUFCN"},"agent_actions":{"view_html":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E","download_json":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E.json","view_paper":"https://pith.science/paper/ZMSQUFCN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0609736&json=true","fetch_graph":"https://pith.science/api/pith-number/ZMSQUFCNGUZTPNHIY3RVYBPM4E/graph.json","fetch_events":"https://pith.science/api/pith-number/ZMSQUFCNGUZTPNHIY3RVYBPM4E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E/action/storage_attestation","attest_author":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E/action/author_attestation","sign_citation":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E/action/citation_signature","submit_replication":"https://pith.science/pith/ZMSQUFCNGUZTPNHIY3RVYBPM4E/action/replication_record"}},"created_at":"2026-07-04T15:25:55.858559+00:00","updated_at":"2026-07-04T15:25:55.858559+00:00"}