{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:KCFDUWU6JETBTHKF2P6MC6HWMD","short_pith_number":"pith:KCFDUWU6","schema_version":"1.0","canonical_sha256":"508a3a5a9e4926199d45d3fcc178f660faf5bb77d03469846400b05631d4aa8a","source":{"kind":"arxiv","id":"2507.02455","version":1},"attestation_state":"computed","paper":{"title":"Constraining nearby substellar companion architectures using High Contrast Imaging, Radial Velocity and Astrometry data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Boehle, F. A. Dannert, L. F. Sartori, M. J. Bonse, S. P. Quanz, Y. Li","submitted_at":"2025-07-03T09:12:05Z","abstract_excerpt":"Nearby stars offer prime opportunities for exoplanet discovery and characterization through various detection methods. By combining HCI, RV, and astrometry, it is possible to better constrain the presence of substellar companions, as each method probes different regions of their parameter space. A detailed census of planets around nearby stars is essential to guide the selection of targets for future space missions seeking to identify Earth-like planets and potentially habitable worlds. In addition, the detection and characterisation of giant planets and brown dwarfs is crucial for understandi"},"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":"2507.02455","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-07-03T09:12:05Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"b4a241825c37470fca4d1cd63c24f390253bbaa5c657ef54a1e4994063862508","abstract_canon_sha256":"38b3d3925004929ed610d87550ec68a8ea089119e8d5d6a4b7d7483570a63fb7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:31:18.606610Z","signature_b64":"1tUUUDfsv60j3tOC5TvKdNNh2eCuHz5UrWZ9OM0RVFxQWNluBrkB9/mf/Jz3mNmbqQh2lLB+MJGNAi2elKquDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"508a3a5a9e4926199d45d3fcc178f660faf5bb77d03469846400b05631d4aa8a","last_reissued_at":"2026-07-05T11:31:18.606162Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:31:18.606162Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining nearby substellar companion architectures using High Contrast Imaging, Radial Velocity and Astrometry data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Boehle, F. A. Dannert, L. F. Sartori, M. J. Bonse, S. P. Quanz, Y. Li","submitted_at":"2025-07-03T09:12:05Z","abstract_excerpt":"Nearby stars offer prime opportunities for exoplanet discovery and characterization through various detection methods. By combining HCI, RV, and astrometry, it is possible to better constrain the presence of substellar companions, as each method probes different regions of their parameter space. A detailed census of planets around nearby stars is essential to guide the selection of targets for future space missions seeking to identify Earth-like planets and potentially habitable worlds. In addition, the detection and characterisation of giant planets and brown dwarfs is crucial for understandi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.02455","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/2507.02455/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":"2507.02455","created_at":"2026-07-05T11:31:18.606217+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.02455v1","created_at":"2026-07-05T11:31:18.606217+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.02455","created_at":"2026-07-05T11:31:18.606217+00:00"},{"alias_kind":"pith_short_12","alias_value":"KCFDUWU6JETB","created_at":"2026-07-05T11:31:18.606217+00:00"},{"alias_kind":"pith_short_16","alias_value":"KCFDUWU6JETBTHKF","created_at":"2026-07-05T11:31:18.606217+00:00"},{"alias_kind":"pith_short_8","alias_value":"KCFDUWU6","created_at":"2026-07-05T11:31:18.606217+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/KCFDUWU6JETBTHKF2P6MC6HWMD","json":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD.json","graph_json":"https://pith.science/api/pith-number/KCFDUWU6JETBTHKF2P6MC6HWMD/graph.json","events_json":"https://pith.science/api/pith-number/KCFDUWU6JETBTHKF2P6MC6HWMD/events.json","paper":"https://pith.science/paper/KCFDUWU6"},"agent_actions":{"view_html":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD","download_json":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD.json","view_paper":"https://pith.science/paper/KCFDUWU6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.02455&json=true","fetch_graph":"https://pith.science/api/pith-number/KCFDUWU6JETBTHKF2P6MC6HWMD/graph.json","fetch_events":"https://pith.science/api/pith-number/KCFDUWU6JETBTHKF2P6MC6HWMD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD/action/storage_attestation","attest_author":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD/action/author_attestation","sign_citation":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD/action/citation_signature","submit_replication":"https://pith.science/pith/KCFDUWU6JETBTHKF2P6MC6HWMD/action/replication_record"}},"created_at":"2026-07-05T11:31:18.606217+00:00","updated_at":"2026-07-05T11:31:18.606217+00:00"}