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From the sample of 92395 stars with the age estimates we have obtained the following kinematic parameters: (U,V,W)=(9.42,20.34,7.21)+/-0.12,0.10,0.09) km/s, \\Omega=26.29+/-0.39 km/s/kpc and \\Omega'=-3.89+/-0.08 km/s/kpc^2, where V0=210+/-6 km/s (for adopted R0=8.0+/-0.2 kpc), and the Oort constants A=15.57+/-0.31 km/s/kpc and B=-10.72+/-0.50 km/s/kpc. It is shown that the parameters \\Omega and \\Omega' are"},"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":"1711.01476","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-04T18:47:24Z","cross_cats_sorted":[],"title_canon_sha256":"e969e66883dd05ebdb0fea7c4667a58877f14c9d8c24c5192bfb6bf7bdd8aad5","abstract_canon_sha256":"b51d9392fc237ec3be8ea6a3da441d36ba219ef6e1943025682adfa5e1d3e36a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:27:41.910424Z","signature_b64":"CyYIdSNmV96JVJVASzw6BHuwXYq4l5CcudWHKLDmjyCT1yEGVQvtYD+SZKX9YJ+8jx8RyqV70SfABFMDsWLzBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5785f42786342898dbec8728d1b6d278a0a1bbe48c31268d2c0883ec27fa2b6a","last_reissued_at":"2026-05-18T00:27:41.909773Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:27:41.909773Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic Kinematics Derived from Data in the RAVE5, UCAC4, PPMXL, and Gaia TGAS Catalogs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.S. Tsvetkov, A.T. Bajkova, V.V. Bobylev, V.V. Vityazev","submitted_at":"2017-11-04T18:47:24Z","abstract_excerpt":"The spatial velocities of the stars with high-precision positions, proper motions and parallaxes from the Gaia TGAS catalog and line-of-sight velocities from the RAVE5 catalog are considered. From the sample of 92395 stars with the age estimates we have obtained the following kinematic parameters: (U,V,W)=(9.42,20.34,7.21)+/-0.12,0.10,0.09) km/s, \\Omega=26.29+/-0.39 km/s/kpc and \\Omega'=-3.89+/-0.08 km/s/kpc^2, where V0=210+/-6 km/s (for adopted R0=8.0+/-0.2 kpc), and the Oort constants A=15.57+/-0.31 km/s/kpc and B=-10.72+/-0.50 km/s/kpc. It is shown that the parameters \\Omega and \\Omega' are"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01476","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":"1711.01476","created_at":"2026-05-18T00:27:41.909865+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.01476v1","created_at":"2026-05-18T00:27:41.909865+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.01476","created_at":"2026-05-18T00:27:41.909865+00:00"},{"alias_kind":"pith_short_12","alias_value":"K6C7IJ4GGQUJ","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"K6C7IJ4GGQUJRW7M","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"K6C7IJ4G","created_at":"2026-05-18T12:31:24.725408+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/K6C7IJ4GGQUJRW7MQ4UNDNWSPC","json":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC.json","graph_json":"https://pith.science/api/pith-number/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/graph.json","events_json":"https://pith.science/api/pith-number/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/events.json","paper":"https://pith.science/paper/K6C7IJ4G"},"agent_actions":{"view_html":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC","download_json":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC.json","view_paper":"https://pith.science/paper/K6C7IJ4G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.01476&json=true","fetch_graph":"https://pith.science/api/pith-number/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/graph.json","fetch_events":"https://pith.science/api/pith-number/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/action/storage_attestation","attest_author":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/action/author_attestation","sign_citation":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/action/citation_signature","submit_replication":"https://pith.science/pith/K6C7IJ4GGQUJRW7MQ4UNDNWSPC/action/replication_record"}},"created_at":"2026-05-18T00:27:41.909865+00:00","updated_at":"2026-05-18T00:27:41.909865+00:00"}