{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:FQKSFXPZFHGR44JBFSZU7RKJG3","short_pith_number":"pith:FQKSFXPZ","schema_version":"1.0","canonical_sha256":"2c1522ddf929cd1e71212cb34fc54936e8edec3f6765df292f0eec00f388ab86","source":{"kind":"arxiv","id":"1510.04903","version":1},"attestation_state":"computed","paper":{"title":"Kinematics of M dwarfs in the CARMENES input catalogue: membership in young moving groups","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. Montes, F. J. Alonso-Floriano, I. Gallardo, J. A. Caballero, M. Cortes-Contreras","submitted_at":"2015-10-11T15:54:01Z","abstract_excerpt":"We present a detailed study of the kinematics of M dwarfs in the CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) input catalog. We have selected all M dwarfs with known parallactic distance or a good photometric distance estimation, precise proper motion in the literature or as determined by us, and radial velocity measurements. Using these parameters, we computed the M dwarfs galactic space motions (U, V, W). For the stars with U and V velocity components inside or near the boundaries that determine the young disk p"},"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":"1510.04903","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-10-11T15:54:01Z","cross_cats_sorted":[],"title_canon_sha256":"2219c9f6f0270497025e8a93e79d43f9050a0fa437911dfa66c46343dd81e9e7","abstract_canon_sha256":"ed02e9aa62205b8398c6a5a98ed1396138821cb4ea062e30249ddc27a43b228a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:21:30.510489Z","signature_b64":"uhOTMGbSk4Yv4nSs942WzoDE+f7pPbcPCOGwd7NWPq5DL8CbNFp2tqWw1c4JCVCsxLRl7D7emApWe87U4ajxBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2c1522ddf929cd1e71212cb34fc54936e8edec3f6765df292f0eec00f388ab86","last_reissued_at":"2026-05-18T01:21:30.509760Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:21:30.509760Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinematics of M dwarfs in the CARMENES input catalogue: membership in young moving groups","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. Montes, F. J. Alonso-Floriano, I. Gallardo, J. A. Caballero, M. Cortes-Contreras","submitted_at":"2015-10-11T15:54:01Z","abstract_excerpt":"We present a detailed study of the kinematics of M dwarfs in the CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) input catalog. We have selected all M dwarfs with known parallactic distance or a good photometric distance estimation, precise proper motion in the literature or as determined by us, and radial velocity measurements. Using these parameters, we computed the M dwarfs galactic space motions (U, V, W). For the stars with U and V velocity components inside or near the boundaries that determine the young disk p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.04903","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":""},"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":"1510.04903","created_at":"2026-05-18T01:21:30.509871+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.04903v1","created_at":"2026-05-18T01:21:30.509871+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.04903","created_at":"2026-05-18T01:21:30.509871+00:00"},{"alias_kind":"pith_short_12","alias_value":"FQKSFXPZFHGR","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_16","alias_value":"FQKSFXPZFHGR44JB","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_8","alias_value":"FQKSFXPZ","created_at":"2026-05-18T12:29:19.899920+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/FQKSFXPZFHGR44JBFSZU7RKJG3","json":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3.json","graph_json":"https://pith.science/api/pith-number/FQKSFXPZFHGR44JBFSZU7RKJG3/graph.json","events_json":"https://pith.science/api/pith-number/FQKSFXPZFHGR44JBFSZU7RKJG3/events.json","paper":"https://pith.science/paper/FQKSFXPZ"},"agent_actions":{"view_html":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3","download_json":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3.json","view_paper":"https://pith.science/paper/FQKSFXPZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.04903&json=true","fetch_graph":"https://pith.science/api/pith-number/FQKSFXPZFHGR44JBFSZU7RKJG3/graph.json","fetch_events":"https://pith.science/api/pith-number/FQKSFXPZFHGR44JBFSZU7RKJG3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3/action/storage_attestation","attest_author":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3/action/author_attestation","sign_citation":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3/action/citation_signature","submit_replication":"https://pith.science/pith/FQKSFXPZFHGR44JBFSZU7RKJG3/action/replication_record"}},"created_at":"2026-05-18T01:21:30.509871+00:00","updated_at":"2026-05-18T01:21:30.509871+00:00"}