{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:WEAWHXR5S7TFKQRNJUZFOAYQZU","short_pith_number":"pith:WEAWHXR5","schema_version":"1.0","canonical_sha256":"b10163de3d97e655422d4d32570310cd22a780376963ce5a95f9164be4dee0c2","source":{"kind":"arxiv","id":"1910.00719","version":2},"attestation_state":"computed","paper":{"title":"Testing the radius scaling relation with ${\\it Gaia}$ DR2 in the ${\\it Kepler}$ field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aldo Serenelli, Daniel Huber, Dennis Stello, Joel C. Zinn, Keivan Stassun, Marc H. Pinsonneault","submitted_at":"2019-10-01T23:56:49Z","abstract_excerpt":"We compare radii based on ${\\it Gaia}$ parallaxes to asteroseismic scaling relation-based radii of $\\sim 300$ dwarfs $\\&$ subgiants and $\\sim 3600$ first-ascent giants from the ${\\it Kepler}$ mission. Systematics due to temperature, bolometric correction, extinction, asteroseismic radius, and the spatially-correlated ${\\it Gaia}$ parallax zero-point, contribute to a $2\\%$ systematic uncertainty on the ${\\it Gaia}$-asteroseismic radius agreement. We find that dwarf and giant scaling radii are on a parallactic scale at the $-2.1 \\% \\pm 0.5 \\% {\\rm \\ (rand.)} \\pm 2.0\\% {\\rm \\ (syst.)}$ level (dwa"},"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":"1910.00719","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-10-01T23:56:49Z","cross_cats_sorted":[],"title_canon_sha256":"ad4e5880c16b6836a7e240de5e85dbd8e31f9feebd4b4788a348ba5e2562a5fb","abstract_canon_sha256":"593501657098171ce722cebe70abffb729cfe9b6c35d499f88bbd6ec516ee33f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:20:20.638067Z","signature_b64":"kAzB8F91wgSNTs7PsbJT7XuARlJ/BtdG+Vvh3H7FBSDEq5lRqVVLpqvploJjQPedSoU4dLFOssydV4XamnW2BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b10163de3d97e655422d4d32570310cd22a780376963ce5a95f9164be4dee0c2","last_reissued_at":"2026-07-05T00:20:20.637635Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:20:20.637635Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing the radius scaling relation with ${\\it Gaia}$ DR2 in the ${\\it Kepler}$ field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aldo Serenelli, Daniel Huber, Dennis Stello, Joel C. Zinn, Keivan Stassun, Marc H. Pinsonneault","submitted_at":"2019-10-01T23:56:49Z","abstract_excerpt":"We compare radii based on ${\\it Gaia}$ parallaxes to asteroseismic scaling relation-based radii of $\\sim 300$ dwarfs $\\&$ subgiants and $\\sim 3600$ first-ascent giants from the ${\\it Kepler}$ mission. Systematics due to temperature, bolometric correction, extinction, asteroseismic radius, and the spatially-correlated ${\\it Gaia}$ parallax zero-point, contribute to a $2\\%$ systematic uncertainty on the ${\\it Gaia}$-asteroseismic radius agreement. We find that dwarf and giant scaling radii are on a parallactic scale at the $-2.1 \\% \\pm 0.5 \\% {\\rm \\ (rand.)} \\pm 2.0\\% {\\rm \\ (syst.)}$ level (dwa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.00719","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1910.00719/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":"1910.00719","created_at":"2026-07-05T00:20:20.637693+00:00"},{"alias_kind":"arxiv_version","alias_value":"1910.00719v2","created_at":"2026-07-05T00:20:20.637693+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1910.00719","created_at":"2026-07-05T00:20:20.637693+00:00"},{"alias_kind":"pith_short_12","alias_value":"WEAWHXR5S7TF","created_at":"2026-07-05T00:20:20.637693+00:00"},{"alias_kind":"pith_short_16","alias_value":"WEAWHXR5S7TFKQRN","created_at":"2026-07-05T00:20:20.637693+00:00"},{"alias_kind":"pith_short_8","alias_value":"WEAWHXR5","created_at":"2026-07-05T00:20:20.637693+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/WEAWHXR5S7TFKQRNJUZFOAYQZU","json":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU.json","graph_json":"https://pith.science/api/pith-number/WEAWHXR5S7TFKQRNJUZFOAYQZU/graph.json","events_json":"https://pith.science/api/pith-number/WEAWHXR5S7TFKQRNJUZFOAYQZU/events.json","paper":"https://pith.science/paper/WEAWHXR5"},"agent_actions":{"view_html":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU","download_json":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU.json","view_paper":"https://pith.science/paper/WEAWHXR5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1910.00719&json=true","fetch_graph":"https://pith.science/api/pith-number/WEAWHXR5S7TFKQRNJUZFOAYQZU/graph.json","fetch_events":"https://pith.science/api/pith-number/WEAWHXR5S7TFKQRNJUZFOAYQZU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU/action/storage_attestation","attest_author":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU/action/author_attestation","sign_citation":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU/action/citation_signature","submit_replication":"https://pith.science/pith/WEAWHXR5S7TFKQRNJUZFOAYQZU/action/replication_record"}},"created_at":"2026-07-05T00:20:20.637693+00:00","updated_at":"2026-07-05T00:20:20.637693+00:00"}