{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:FVE7ZMQL44NXBPQUYB26ZMQPVU","short_pith_number":"pith:FVE7ZMQL","schema_version":"1.0","canonical_sha256":"2d49fcb20be71b70be14c075ecb20fad25f7f334250c0dd09eded6e8a706bc20","source":{"kind":"arxiv","id":"2301.00203","version":2},"attestation_state":"computed","paper":{"title":"The vertex coordinates of the Galaxy's stellar systems according to the Gaia DR3 catalogue","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"A. B. Velichko, A. M. Dmytrenko, P. N. Fedorov, S. I. Denyshchenko, V. S. Akhmetov","submitted_at":"2022-12-31T13:54:57Z","abstract_excerpt":"We present the results of determining the coordinates of the vertices of various stellar systems, the centroids of which are located in the Galactic plane. To do this, the positions, parallaxes, proper motions, and radial velocities of red giants and subgiants contained in the $Gaia$~DR3 catalogue have been used. When determining the components of the deformation velocity tensors in local coordinate systems, we found the coordinates of the vertices of the stellar systems under study. It turned out that there is a complex dependence of vertex deviations $l_{xy}$ in Galactocentric cylindrical ($"},"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":"2301.00203","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-12-31T13:54:57Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"6bf64c9daf68a615936887a83f089065019279fba84ed265704d263dfe478ad2","abstract_canon_sha256":"f2a44b3002e2efddfd1f7ee3f05d25e68501a22dbb07e0bc1b4d38e675fec8aa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:55:16.619421Z","signature_b64":"rLE1fpgh9C/mv+7eJ6D0U1JGLiVd97yQj5r3znTsmnyZo/4+bOeyppAa8npOOBp/UJ6Dj+qxNLr6Gmf2yS67CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2d49fcb20be71b70be14c075ecb20fad25f7f334250c0dd09eded6e8a706bc20","last_reissued_at":"2026-07-05T05:55:16.618834Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:55:16.618834Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The vertex coordinates of the Galaxy's stellar systems according to the Gaia DR3 catalogue","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"A. B. Velichko, A. M. Dmytrenko, P. N. Fedorov, S. I. Denyshchenko, V. S. Akhmetov","submitted_at":"2022-12-31T13:54:57Z","abstract_excerpt":"We present the results of determining the coordinates of the vertices of various stellar systems, the centroids of which are located in the Galactic plane. To do this, the positions, parallaxes, proper motions, and radial velocities of red giants and subgiants contained in the $Gaia$~DR3 catalogue have been used. When determining the components of the deformation velocity tensors in local coordinate systems, we found the coordinates of the vertices of the stellar systems under study. It turned out that there is a complex dependence of vertex deviations $l_{xy}$ in Galactocentric cylindrical ($"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.00203","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/2301.00203/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":"2301.00203","created_at":"2026-07-05T05:55:16.618916+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.00203v2","created_at":"2026-07-05T05:55:16.618916+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.00203","created_at":"2026-07-05T05:55:16.618916+00:00"},{"alias_kind":"pith_short_12","alias_value":"FVE7ZMQL44NX","created_at":"2026-07-05T05:55:16.618916+00:00"},{"alias_kind":"pith_short_16","alias_value":"FVE7ZMQL44NXBPQU","created_at":"2026-07-05T05:55:16.618916+00:00"},{"alias_kind":"pith_short_8","alias_value":"FVE7ZMQL","created_at":"2026-07-05T05:55:16.618916+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.04075","citing_title":"Milky Way dynamics in light of Gaia","ref_index":68,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU","json":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU.json","graph_json":"https://pith.science/api/pith-number/FVE7ZMQL44NXBPQUYB26ZMQPVU/graph.json","events_json":"https://pith.science/api/pith-number/FVE7ZMQL44NXBPQUYB26ZMQPVU/events.json","paper":"https://pith.science/paper/FVE7ZMQL"},"agent_actions":{"view_html":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU","download_json":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU.json","view_paper":"https://pith.science/paper/FVE7ZMQL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.00203&json=true","fetch_graph":"https://pith.science/api/pith-number/FVE7ZMQL44NXBPQUYB26ZMQPVU/graph.json","fetch_events":"https://pith.science/api/pith-number/FVE7ZMQL44NXBPQUYB26ZMQPVU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU/action/storage_attestation","attest_author":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU/action/author_attestation","sign_citation":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU/action/citation_signature","submit_replication":"https://pith.science/pith/FVE7ZMQL44NXBPQUYB26ZMQPVU/action/replication_record"}},"created_at":"2026-07-05T05:55:16.618916+00:00","updated_at":"2026-07-05T05:55:16.618916+00:00"}