{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:YBVRKCYY3YXDB33DFDWFW43WTX","short_pith_number":"pith:YBVRKCYY","schema_version":"1.0","canonical_sha256":"c06b150b18de2e30ef6328ec5b73769de30db3469e3dbf9bed890a64e6a64b6e","source":{"kind":"arxiv","id":"2112.09185","version":1},"attestation_state":"computed","paper":{"title":"Predicted Trends in Milky Way Bulge Proper Motion Rotation Curves: future Prospects for HST and LSST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Annalisa Calamida, Kailash C. Sahu, Mario Gennaro, Oscar A. Gonzalez, Steven Gough-Kelly, Stuart R. Anderson, Victor P. Debattista, William I. Clarkson","submitted_at":"2021-12-16T20:15:38Z","abstract_excerpt":"We use an $N$-body+smoothed particle hydrodynamics simulation of an isolated barred galaxy to study the age dependence of bulge longitudinal proper motion ($\\mu_l$) rotation curves. We show that close to the minor axis ($|l| \\sim 0^\\circ$) the relatively young stars rotate more rapidly than the old stars, as found by Hubble Space Telescope in the Milky Way's (MW's) bulge. This behaviour would be expected also if the MW were unbarred. At larger $|l|$ a different behaviour emerges. Because younger stars trace a strong bar, their galactocentric radial motions dominate their $\\mu_l$ at $|l| \\sim 6"},"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":"2112.09185","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-12-16T20:15:38Z","cross_cats_sorted":[],"title_canon_sha256":"5f3d537633e73ae0f02a000c5e609d2d7712f8935bd5bc3c9cd8249186e25b36","abstract_canon_sha256":"2e86a3bffe466252cfe0c65f4801802a6508b726173f3bab16b5d4c98c036cc6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:41:43.591506Z","signature_b64":"sDlxkqE306yvGent3HhtphFk5FGrqzssDK02dZSHWWTaRs5jrFGKB0MGKiWfrzWrtX7ahTKAZY/gdUljs0NQCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c06b150b18de2e30ef6328ec5b73769de30db3469e3dbf9bed890a64e6a64b6e","last_reissued_at":"2026-07-05T03:41:43.591124Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:41:43.591124Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Predicted Trends in Milky Way Bulge Proper Motion Rotation Curves: future Prospects for HST and LSST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Annalisa Calamida, Kailash C. Sahu, Mario Gennaro, Oscar A. Gonzalez, Steven Gough-Kelly, Stuart R. Anderson, Victor P. Debattista, William I. Clarkson","submitted_at":"2021-12-16T20:15:38Z","abstract_excerpt":"We use an $N$-body+smoothed particle hydrodynamics simulation of an isolated barred galaxy to study the age dependence of bulge longitudinal proper motion ($\\mu_l$) rotation curves. We show that close to the minor axis ($|l| \\sim 0^\\circ$) the relatively young stars rotate more rapidly than the old stars, as found by Hubble Space Telescope in the Milky Way's (MW's) bulge. This behaviour would be expected also if the MW were unbarred. At larger $|l|$ a different behaviour emerges. Because younger stars trace a strong bar, their galactocentric radial motions dominate their $\\mu_l$ at $|l| \\sim 6"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2112.09185","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/2112.09185/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":"2112.09185","created_at":"2026-07-05T03:41:43.591179+00:00"},{"alias_kind":"arxiv_version","alias_value":"2112.09185v1","created_at":"2026-07-05T03:41:43.591179+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2112.09185","created_at":"2026-07-05T03:41:43.591179+00:00"},{"alias_kind":"pith_short_12","alias_value":"YBVRKCYY3YXD","created_at":"2026-07-05T03:41:43.591179+00:00"},{"alias_kind":"pith_short_16","alias_value":"YBVRKCYY3YXDB33D","created_at":"2026-07-05T03:41:43.591179+00:00"},{"alias_kind":"pith_short_8","alias_value":"YBVRKCYY","created_at":"2026-07-05T03:41:43.591179+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/YBVRKCYY3YXDB33DFDWFW43WTX","json":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX.json","graph_json":"https://pith.science/api/pith-number/YBVRKCYY3YXDB33DFDWFW43WTX/graph.json","events_json":"https://pith.science/api/pith-number/YBVRKCYY3YXDB33DFDWFW43WTX/events.json","paper":"https://pith.science/paper/YBVRKCYY"},"agent_actions":{"view_html":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX","download_json":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX.json","view_paper":"https://pith.science/paper/YBVRKCYY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2112.09185&json=true","fetch_graph":"https://pith.science/api/pith-number/YBVRKCYY3YXDB33DFDWFW43WTX/graph.json","fetch_events":"https://pith.science/api/pith-number/YBVRKCYY3YXDB33DFDWFW43WTX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX/action/storage_attestation","attest_author":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX/action/author_attestation","sign_citation":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX/action/citation_signature","submit_replication":"https://pith.science/pith/YBVRKCYY3YXDB33DFDWFW43WTX/action/replication_record"}},"created_at":"2026-07-05T03:41:43.591179+00:00","updated_at":"2026-07-05T03:41:43.591179+00:00"}