{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BNCC3RLU5I5PW53IEJ6SMY7GJ2","short_pith_number":"pith:BNCC3RLU","schema_version":"1.0","canonical_sha256":"0b442dc574ea3afb7768227d2663e64ea9d8d1c71b8365928b74d730f7ae613f","source":{"kind":"arxiv","id":"1410.8135","version":2},"attestation_state":"computed","paper":{"title":"The power spectrum of the Milky Way: Velocity fluctuations in the Galactic disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana E. Garc\\'ia P\\'erez, David L. Nidever, Gail Zasowski, Jo Bovy (IAS), Jonathan C. Bird, Steven R. Majewski","submitted_at":"2014-10-29T20:00:08Z","abstract_excerpt":"We investigate the kinematics of stars in the mid-plane of the Milky Way on scales between 25 pc and 10 kpc with data from the Apache Point Observatory Galactic Evolution Experiment (APOGEE), the Radial Velocity Experiment (RAVE), and the Geneva-Copenhagen Survey (GCS). Using red-clump stars in APOGEE, we determine the large-scale line-of-sight velocity field out to 5 kpc from the Sun in (0.75 kpc)^2 bins. The solar motion V_{sun-c} with respect to the circular velocity V_c is the largest contribution to the power on large scales after subtracting an axisymmetric rotation field; we determine t"},"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":"1410.8135","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-10-29T20:00:08Z","cross_cats_sorted":[],"title_canon_sha256":"1c8c2f3bde8ec6415da6c3f2d9d7f981ea39b908fbc41ba28af4e5b824c93a95","abstract_canon_sha256":"65c5ca7bae3992636ea911056325a971c3e2aaa0722fc49cc6cabc7572351407"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:38.801866Z","signature_b64":"vo1NQjIC/eS29W09w5NEoN5/0b6lpZLklY1aR2nn+SToyF4D8/yAN/qpVq13jXBiJ8hn8TRZIKpZ1EUkeP3vDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b442dc574ea3afb7768227d2663e64ea9d8d1c71b8365928b74d730f7ae613f","last_reissued_at":"2026-05-18T01:41:38.801247Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:38.801247Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The power spectrum of the Milky Way: Velocity fluctuations in the Galactic disk","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana E. Garc\\'ia P\\'erez, David L. Nidever, Gail Zasowski, Jo Bovy (IAS), Jonathan C. Bird, Steven R. Majewski","submitted_at":"2014-10-29T20:00:08Z","abstract_excerpt":"We investigate the kinematics of stars in the mid-plane of the Milky Way on scales between 25 pc and 10 kpc with data from the Apache Point Observatory Galactic Evolution Experiment (APOGEE), the Radial Velocity Experiment (RAVE), and the Geneva-Copenhagen Survey (GCS). Using red-clump stars in APOGEE, we determine the large-scale line-of-sight velocity field out to 5 kpc from the Sun in (0.75 kpc)^2 bins. The solar motion V_{sun-c} with respect to the circular velocity V_c is the largest contribution to the power on large scales after subtracting an axisymmetric rotation field; we determine t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.8135","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":""},"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":"1410.8135","created_at":"2026-05-18T01:41:38.801326+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.8135v2","created_at":"2026-05-18T01:41:38.801326+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.8135","created_at":"2026-05-18T01:41:38.801326+00:00"},{"alias_kind":"pith_short_12","alias_value":"BNCC3RLU5I5P","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BNCC3RLU5I5PW53I","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BNCC3RLU","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.02712","citing_title":"Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2606.10623","citing_title":"Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies","ref_index":108,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2","json":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2.json","graph_json":"https://pith.science/api/pith-number/BNCC3RLU5I5PW53IEJ6SMY7GJ2/graph.json","events_json":"https://pith.science/api/pith-number/BNCC3RLU5I5PW53IEJ6SMY7GJ2/events.json","paper":"https://pith.science/paper/BNCC3RLU"},"agent_actions":{"view_html":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2","download_json":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2.json","view_paper":"https://pith.science/paper/BNCC3RLU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.8135&json=true","fetch_graph":"https://pith.science/api/pith-number/BNCC3RLU5I5PW53IEJ6SMY7GJ2/graph.json","fetch_events":"https://pith.science/api/pith-number/BNCC3RLU5I5PW53IEJ6SMY7GJ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2/action/storage_attestation","attest_author":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2/action/author_attestation","sign_citation":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2/action/citation_signature","submit_replication":"https://pith.science/pith/BNCC3RLU5I5PW53IEJ6SMY7GJ2/action/replication_record"}},"created_at":"2026-05-18T01:41:38.801326+00:00","updated_at":"2026-05-18T01:41:38.801326+00:00"}