{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:N6NGW6LU36OXGKZJIJLJVC4TU2","short_pith_number":"pith:N6NGW6LU","schema_version":"1.0","canonical_sha256":"6f9a6b7974df9d732b2942569a8b93a6b5f68db4df8ea88bed36545c3abc4050","source":{"kind":"arxiv","id":"2203.11090","version":1},"attestation_state":"computed","paper":{"title":"Substellar Hyades Candidates from the UKIRT Hemisphere Survey","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Adam C. Schneider, Arttu Sainio, Austin Rothermich, Byran N. Dorland, Christopher Tanner, Dan Caselden, Emily Calamari, Frederick J. Vrba, Jacqueline K. Faherty, Jeffrey A. Munn, Justice Bruursema, Martin Kabatnik, Michael C. Cushing, Nikolaj Stevnbak Andersen, Scott E. Dahm, Stephen J. Williams, William Pendrill","submitted_at":"2022-03-21T16:15:11Z","abstract_excerpt":"We have used data from the UKIRT Hemisphere Survey (UHS) to search for substellar members of the Hyades cluster. Our search recovered several known substellar Hyades members, and two known brown dwarfs that we suggest may be members based on a new kinematic analysis. We uncovered thirteen new substellar Hyades candidates, and obtained near-infrared follow-up spectroscopy of each with IRTF/SpeX. Six candidates with spectral types between M7 and L0 are ruled out as potential members based on their photometric distances ($\\gtrsim$100 pc). The remaining seven candidates, with spectral types betwee"},"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":"2203.11090","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-03-21T16:15:11Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"5d844905dd66704557077449a0975a077baeae673d5e4673872dba90c221e27c","abstract_canon_sha256":"23c01b0489b65fc81b5a59cf232f407a5036a2e7446ff0537512e1e827e2e80f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:22:06.022492Z","signature_b64":"EwjzXM8y6KPnCG8Lk2JXpF4BgXHgJe2sv688ZC4sVPH3uYCOhGTpyew2aue0nlxY9XJ7ew+QAzoqOBP4zH3mBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6f9a6b7974df9d732b2942569a8b93a6b5f68db4df8ea88bed36545c3abc4050","last_reissued_at":"2026-07-05T04:22:06.022060Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:22:06.022060Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Substellar Hyades Candidates from the UKIRT Hemisphere Survey","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Adam C. Schneider, Arttu Sainio, Austin Rothermich, Byran N. Dorland, Christopher Tanner, Dan Caselden, Emily Calamari, Frederick J. Vrba, Jacqueline K. Faherty, Jeffrey A. Munn, Justice Bruursema, Martin Kabatnik, Michael C. Cushing, Nikolaj Stevnbak Andersen, Scott E. Dahm, Stephen J. Williams, William Pendrill","submitted_at":"2022-03-21T16:15:11Z","abstract_excerpt":"We have used data from the UKIRT Hemisphere Survey (UHS) to search for substellar members of the Hyades cluster. Our search recovered several known substellar Hyades members, and two known brown dwarfs that we suggest may be members based on a new kinematic analysis. We uncovered thirteen new substellar Hyades candidates, and obtained near-infrared follow-up spectroscopy of each with IRTF/SpeX. Six candidates with spectral types between M7 and L0 are ruled out as potential members based on their photometric distances ($\\gtrsim$100 pc). The remaining seven candidates, with spectral types betwee"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.11090","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/2203.11090/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":"2203.11090","created_at":"2026-07-05T04:22:06.022125+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.11090v1","created_at":"2026-07-05T04:22:06.022125+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.11090","created_at":"2026-07-05T04:22:06.022125+00:00"},{"alias_kind":"pith_short_12","alias_value":"N6NGW6LU36OX","created_at":"2026-07-05T04:22:06.022125+00:00"},{"alias_kind":"pith_short_16","alias_value":"N6NGW6LU36OXGKZJ","created_at":"2026-07-05T04:22:06.022125+00:00"},{"alias_kind":"pith_short_8","alias_value":"N6NGW6LU","created_at":"2026-07-05T04:22:06.022125+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/N6NGW6LU36OXGKZJIJLJVC4TU2","json":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2.json","graph_json":"https://pith.science/api/pith-number/N6NGW6LU36OXGKZJIJLJVC4TU2/graph.json","events_json":"https://pith.science/api/pith-number/N6NGW6LU36OXGKZJIJLJVC4TU2/events.json","paper":"https://pith.science/paper/N6NGW6LU"},"agent_actions":{"view_html":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2","download_json":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2.json","view_paper":"https://pith.science/paper/N6NGW6LU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.11090&json=true","fetch_graph":"https://pith.science/api/pith-number/N6NGW6LU36OXGKZJIJLJVC4TU2/graph.json","fetch_events":"https://pith.science/api/pith-number/N6NGW6LU36OXGKZJIJLJVC4TU2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2/action/storage_attestation","attest_author":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2/action/author_attestation","sign_citation":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2/action/citation_signature","submit_replication":"https://pith.science/pith/N6NGW6LU36OXGKZJIJLJVC4TU2/action/replication_record"}},"created_at":"2026-07-05T04:22:06.022125+00:00","updated_at":"2026-07-05T04:22:06.022125+00:00"}