{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:GB6DXCJBOCSVDCYKKPZFSKRAL7","short_pith_number":"pith:GB6DXCJB","schema_version":"1.0","canonical_sha256":"307c3b892170a5518b0a53f2592a205fc0a840c08fd04023cde3e2646dee7993","source":{"kind":"arxiv","id":"2606.12548","version":1},"attestation_state":"computed","paper":{"title":"Constraining the Geometry of Galactic Dark Matter with Gaia Data Release 3","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Francesco Sylos Labini, Roberto Capuzzo-Dolcetta","submitted_at":"2026-06-10T18:01:01Z","abstract_excerpt":"We derive both the mid-plane and off-plane rotation curves, $v_c(R,z)$, and the vertical acceleration, $a_z(R,z)$, of the Milky Way (MW) using \\textit{Gaia}~DR3 data over the ranges of vertical heights $z \\in (-2,2)\\,$ kpc and galactocentric distances $R \\in (8.5,14)$ kpc where the velocity components are determined with high precision, i.e., with an error $< 5\\%$. In contrast, the vertical acceleration $a_z(R,z)$ is dominated by model-dependent systematics, with uncertainties of up to $\\sim 20\\%$. This level of accuracy allows us to place stringent constraints on the geometry of the MW's dark"},"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":"2606.12548","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-06-10T18:01:01Z","cross_cats_sorted":[],"title_canon_sha256":"af04a1b70b28adac53472a516d311f6094a93c185cd11f204c79e39d4942ea50","abstract_canon_sha256":"36bfd26bbc523fe367c6c3bf6125a2e7ab308654544be6987ebc4fe428e72ef7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-12T00:07:54.257557Z","signature_b64":"tSpSklBG44NIDtg6yxQOPfuWHIF2MgL8RumOlKEDPKbqmUEDVmA7Sjw5brt5FX3rlPEfQ/GbMrsXf4P3nF5PDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"307c3b892170a5518b0a53f2592a205fc0a840c08fd04023cde3e2646dee7993","last_reissued_at":"2026-06-12T00:07:54.257126Z","signature_status":"signed_v1","first_computed_at":"2026-06-12T00:07:54.257126Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the Geometry of Galactic Dark Matter with Gaia Data Release 3","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Francesco Sylos Labini, Roberto Capuzzo-Dolcetta","submitted_at":"2026-06-10T18:01:01Z","abstract_excerpt":"We derive both the mid-plane and off-plane rotation curves, $v_c(R,z)$, and the vertical acceleration, $a_z(R,z)$, of the Milky Way (MW) using \\textit{Gaia}~DR3 data over the ranges of vertical heights $z \\in (-2,2)\\,$ kpc and galactocentric distances $R \\in (8.5,14)$ kpc where the velocity components are determined with high precision, i.e., with an error $< 5\\%$. In contrast, the vertical acceleration $a_z(R,z)$ is dominated by model-dependent systematics, with uncertainties of up to $\\sim 20\\%$. This level of accuracy allows us to place stringent constraints on the geometry of the MW's dark"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.12548","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/2606.12548/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":"2606.12548","created_at":"2026-06-12T00:07:54.257191+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.12548v1","created_at":"2026-06-12T00:07:54.257191+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.12548","created_at":"2026-06-12T00:07:54.257191+00:00"},{"alias_kind":"pith_short_12","alias_value":"GB6DXCJBOCSV","created_at":"2026-06-12T00:07:54.257191+00:00"},{"alias_kind":"pith_short_16","alias_value":"GB6DXCJBOCSVDCYK","created_at":"2026-06-12T00:07:54.257191+00:00"},{"alias_kind":"pith_short_8","alias_value":"GB6DXCJB","created_at":"2026-06-12T00:07:54.257191+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/GB6DXCJBOCSVDCYKKPZFSKRAL7","json":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7.json","graph_json":"https://pith.science/api/pith-number/GB6DXCJBOCSVDCYKKPZFSKRAL7/graph.json","events_json":"https://pith.science/api/pith-number/GB6DXCJBOCSVDCYKKPZFSKRAL7/events.json","paper":"https://pith.science/paper/GB6DXCJB"},"agent_actions":{"view_html":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7","download_json":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7.json","view_paper":"https://pith.science/paper/GB6DXCJB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.12548&json=true","fetch_graph":"https://pith.science/api/pith-number/GB6DXCJBOCSVDCYKKPZFSKRAL7/graph.json","fetch_events":"https://pith.science/api/pith-number/GB6DXCJBOCSVDCYKKPZFSKRAL7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7/action/storage_attestation","attest_author":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7/action/author_attestation","sign_citation":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7/action/citation_signature","submit_replication":"https://pith.science/pith/GB6DXCJBOCSVDCYKKPZFSKRAL7/action/replication_record"}},"created_at":"2026-06-12T00:07:54.257191+00:00","updated_at":"2026-06-12T00:07:54.257191+00:00"}