{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:WKFW35VAYZGB27KTHS6OGBXYFF","short_pith_number":"pith:WKFW35VA","schema_version":"1.0","canonical_sha256":"b28b6df6a0c64c1d7d533cbce306f82976b3c62540e500a3a2cdc59ccce0cf09","source":{"kind":"arxiv","id":"1310.1405","version":1},"attestation_state":"computed","paper":{"title":"Astrometric Detection of Giant Planets Around Nearby M Dwarfs: The Gaia Potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Sozzetti, G. Micela, G. Tinetti, M.G. Lattanzi, P. Giacobbe, R. Morbidelli","submitted_at":"2013-10-04T20:22:26Z","abstract_excerpt":"[abridged] We carry out numerical simulations to gauge the Gaia potential for precision astrometry of exoplanets orbiting a sample of known dM stars within 30 pc from the Sun. (1) It will be possible to accurately determine orbits and masses for Jupiter-mass planets with orbital periods in the range 0.2<P<6.0 yr and with an astrometric signal-to-noise ratio > 10. Given present-day estimates of the planet fraction f_p around M dwarfs, 100 giant planets could be found by Gaia around the sample. Comprehensive screening by Gaia of the reservoir of 4x10^5 M dwarfs within 100 pc could result in 2600"},"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":"1310.1405","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-10-04T20:22:26Z","cross_cats_sorted":[],"title_canon_sha256":"e340cdee47b3e68bc7e24d959a50936acfcc2b5a532e57327e92e90d06bfd7a3","abstract_canon_sha256":"9a59a039be5d64f671d28663e7e6dc99c1ae2669f277be60819229e85f4b4a01"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:14.967444Z","signature_b64":"Mp//JUA2koHsswGhQ4R3CON1CN8y6wWbYeYqfmD9F3iI0IVxlN8roU5rSxM4PdCoHp0TTr+C8sf1sBsSHJ4/Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b28b6df6a0c64c1d7d533cbce306f82976b3c62540e500a3a2cdc59ccce0cf09","last_reissued_at":"2026-05-18T01:47:14.966770Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:14.966770Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Astrometric Detection of Giant Planets Around Nearby M Dwarfs: The Gaia Potential","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Sozzetti, G. Micela, G. Tinetti, M.G. Lattanzi, P. Giacobbe, R. Morbidelli","submitted_at":"2013-10-04T20:22:26Z","abstract_excerpt":"[abridged] We carry out numerical simulations to gauge the Gaia potential for precision astrometry of exoplanets orbiting a sample of known dM stars within 30 pc from the Sun. (1) It will be possible to accurately determine orbits and masses for Jupiter-mass planets with orbital periods in the range 0.2<P<6.0 yr and with an astrometric signal-to-noise ratio > 10. Given present-day estimates of the planet fraction f_p around M dwarfs, 100 giant planets could be found by Gaia around the sample. Comprehensive screening by Gaia of the reservoir of 4x10^5 M dwarfs within 100 pc could result in 2600"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.1405","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":"1310.1405","created_at":"2026-05-18T01:47:14.966869+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.1405v1","created_at":"2026-05-18T01:47:14.966869+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.1405","created_at":"2026-05-18T01:47:14.966869+00:00"},{"alias_kind":"pith_short_12","alias_value":"WKFW35VAYZGB","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_16","alias_value":"WKFW35VAYZGB27KT","created_at":"2026-05-18T12:28:04.890932+00:00"},{"alias_kind":"pith_short_8","alias_value":"WKFW35VA","created_at":"2026-05-18T12:28:04.890932+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.24862","citing_title":"Ultra-Precise Astrometric Search for Exoplanets with SKA-VLBI","ref_index":61,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF","json":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF.json","graph_json":"https://pith.science/api/pith-number/WKFW35VAYZGB27KTHS6OGBXYFF/graph.json","events_json":"https://pith.science/api/pith-number/WKFW35VAYZGB27KTHS6OGBXYFF/events.json","paper":"https://pith.science/paper/WKFW35VA"},"agent_actions":{"view_html":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF","download_json":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF.json","view_paper":"https://pith.science/paper/WKFW35VA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.1405&json=true","fetch_graph":"https://pith.science/api/pith-number/WKFW35VAYZGB27KTHS6OGBXYFF/graph.json","fetch_events":"https://pith.science/api/pith-number/WKFW35VAYZGB27KTHS6OGBXYFF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF/action/storage_attestation","attest_author":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF/action/author_attestation","sign_citation":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF/action/citation_signature","submit_replication":"https://pith.science/pith/WKFW35VAYZGB27KTHS6OGBXYFF/action/replication_record"}},"created_at":"2026-05-18T01:47:14.966869+00:00","updated_at":"2026-05-18T01:47:14.966869+00:00"}