{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:OEK4RLJ72WNNDCNLQ7V3KFUDPL","short_pith_number":"pith:OEK4RLJ7","schema_version":"1.0","canonical_sha256":"7115c8ad3fd59ad189ab87ebb516837adadaddcb444c5f7d01e8cd9716bf3253","source":{"kind":"arxiv","id":"1704.05063","version":2},"attestation_state":"computed","paper":{"title":"Stellar Inventory of the Solar Neighborhood using Gaia DR1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jo Bovy","submitted_at":"2017-04-17T18:00:00Z","abstract_excerpt":"The absolute number and the density profiles of different types of stars in the solar neighborhood are a fundamental anchor for studies of the initial mass function, stellar evolution, and galactic structure. Using data from the Gaia DR1 Tycho-Gaia Astrometric Solution, we reconstruct Gaia's selection function and we determine Gaia's volume completeness, the local number density, and the vertical profiles of different spectral types along the main sequence from early A stars to late K stars as well as along the giant branch. We clearly detect the expected flattening of the stellar density prof"},"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":"1704.05063","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-04-17T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"22843af534072b54fa05cd2b44c1d237cddf7c8324e2eb9f2c987a71c563248e","abstract_canon_sha256":"24b1e14ec45760e48cfe44e4b95335129cc8b8072277b203c6af13aa4281e8da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:19.103338Z","signature_b64":"THKskg6uxMuucX2vKWNOJfrNoK+MoGN0JIdZr8CLog2/NkOIMRA95Lg2VCjBrRJDqMG+x3Nh5xQpdpWfN6S+Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7115c8ad3fd59ad189ab87ebb516837adadaddcb444c5f7d01e8cd9716bf3253","last_reissued_at":"2026-05-18T00:40:19.102434Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:19.102434Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar Inventory of the Solar Neighborhood using Gaia DR1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Jo Bovy","submitted_at":"2017-04-17T18:00:00Z","abstract_excerpt":"The absolute number and the density profiles of different types of stars in the solar neighborhood are a fundamental anchor for studies of the initial mass function, stellar evolution, and galactic structure. Using data from the Gaia DR1 Tycho-Gaia Astrometric Solution, we reconstruct Gaia's selection function and we determine Gaia's volume completeness, the local number density, and the vertical profiles of different spectral types along the main sequence from early A stars to late K stars as well as along the giant branch. We clearly detect the expected flattening of the stellar density prof"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.05063","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":"1704.05063","created_at":"2026-05-18T00:40:19.102580+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.05063v2","created_at":"2026-05-18T00:40:19.102580+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.05063","created_at":"2026-05-18T00:40:19.102580+00:00"},{"alias_kind":"pith_short_12","alias_value":"OEK4RLJ72WNN","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"OEK4RLJ72WNNDCNL","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"OEK4RLJ7","created_at":"2026-05-18T12:31:34.259226+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.31042","citing_title":"An Acceleration is Worth a Hundred Thousand Phase Space Measurements","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL","json":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL.json","graph_json":"https://pith.science/api/pith-number/OEK4RLJ72WNNDCNLQ7V3KFUDPL/graph.json","events_json":"https://pith.science/api/pith-number/OEK4RLJ72WNNDCNLQ7V3KFUDPL/events.json","paper":"https://pith.science/paper/OEK4RLJ7"},"agent_actions":{"view_html":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL","download_json":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL.json","view_paper":"https://pith.science/paper/OEK4RLJ7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.05063&json=true","fetch_graph":"https://pith.science/api/pith-number/OEK4RLJ72WNNDCNLQ7V3KFUDPL/graph.json","fetch_events":"https://pith.science/api/pith-number/OEK4RLJ72WNNDCNLQ7V3KFUDPL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL/action/storage_attestation","attest_author":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL/action/author_attestation","sign_citation":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL/action/citation_signature","submit_replication":"https://pith.science/pith/OEK4RLJ72WNNDCNLQ7V3KFUDPL/action/replication_record"}},"created_at":"2026-05-18T00:40:19.102580+00:00","updated_at":"2026-05-18T00:40:19.102580+00:00"}