{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:CTN7GA36E4J6WB45DQZCMAKSOQ","short_pith_number":"pith:CTN7GA36","schema_version":"1.0","canonical_sha256":"14dbf3037e2713eb079d1c322601527433448c7bc0ee585c8f7bb5378a9926d2","source":{"kind":"arxiv","id":"1601.05508","version":2},"attestation_state":"computed","paper":{"title":"Searching for Binary Y dwarfs with the Gemini Multi-Conjugate Adaptive Optics System (GeMS)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. G. Tinney, Christopher R. Gelino, Daniela Opitz, Jacqueline Faherty, J. Davy Kirkpatrick, Sarah Sweet","submitted_at":"2016-01-21T04:27:16Z","abstract_excerpt":"The NASA Wide-field Infrared Survey Explorer (WISE) has discovered almost all the known members of the new class of Y-type brown dwarfs. Most of these Y dwarfs have been identified as isolated objects in the field. It is known that binaries with L- and T-type brown dwarf primaries are less prevalent than either M-dwarf or solar-type primaries, they tend to have smaller separations and are more frequently detected in near-equal mass configurations. The binary statistics for Y-type brown dwarfs, however, are sparse, and so it is unclear if the same trends that hold for L- and T-type brown dwarfs"},"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":"1601.05508","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-01-21T04:27:16Z","cross_cats_sorted":[],"title_canon_sha256":"aba5dc3e1be36e065cdc2d68738d1c6dc8ab7bf4654449020d7132a85f4ee066","abstract_canon_sha256":"ac57d564cd5b33b025613f6404568078143822e4e147379aca8ffc3271d12118"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:19:01.250389Z","signature_b64":"V8R0yS2RLEUdOspmV+rn10vI53Yd1Qq+IduBEEH5wZ4oQFULVGUTkgLKjsUUFMjeoOProMPefBrnYg7ALkzhAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14dbf3037e2713eb079d1c322601527433448c7bc0ee585c8f7bb5378a9926d2","last_reissued_at":"2026-05-18T01:19:01.249866Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:19:01.249866Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for Binary Y dwarfs with the Gemini Multi-Conjugate Adaptive Optics System (GeMS)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. G. Tinney, Christopher R. Gelino, Daniela Opitz, Jacqueline Faherty, J. Davy Kirkpatrick, Sarah Sweet","submitted_at":"2016-01-21T04:27:16Z","abstract_excerpt":"The NASA Wide-field Infrared Survey Explorer (WISE) has discovered almost all the known members of the new class of Y-type brown dwarfs. Most of these Y dwarfs have been identified as isolated objects in the field. It is known that binaries with L- and T-type brown dwarf primaries are less prevalent than either M-dwarf or solar-type primaries, they tend to have smaller separations and are more frequently detected in near-equal mass configurations. The binary statistics for Y-type brown dwarfs, however, are sparse, and so it is unclear if the same trends that hold for L- and T-type brown dwarfs"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.05508","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":"1601.05508","created_at":"2026-05-18T01:19:01.249949+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.05508v2","created_at":"2026-05-18T01:19:01.249949+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.05508","created_at":"2026-05-18T01:19:01.249949+00:00"},{"alias_kind":"pith_short_12","alias_value":"CTN7GA36E4J6","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_16","alias_value":"CTN7GA36E4J6WB45","created_at":"2026-05-18T12:30:09.641336+00:00"},{"alias_kind":"pith_short_8","alias_value":"CTN7GA36","created_at":"2026-05-18T12:30:09.641336+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/CTN7GA36E4J6WB45DQZCMAKSOQ","json":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ.json","graph_json":"https://pith.science/api/pith-number/CTN7GA36E4J6WB45DQZCMAKSOQ/graph.json","events_json":"https://pith.science/api/pith-number/CTN7GA36E4J6WB45DQZCMAKSOQ/events.json","paper":"https://pith.science/paper/CTN7GA36"},"agent_actions":{"view_html":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ","download_json":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ.json","view_paper":"https://pith.science/paper/CTN7GA36","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.05508&json=true","fetch_graph":"https://pith.science/api/pith-number/CTN7GA36E4J6WB45DQZCMAKSOQ/graph.json","fetch_events":"https://pith.science/api/pith-number/CTN7GA36E4J6WB45DQZCMAKSOQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ/action/storage_attestation","attest_author":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ/action/author_attestation","sign_citation":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ/action/citation_signature","submit_replication":"https://pith.science/pith/CTN7GA36E4J6WB45DQZCMAKSOQ/action/replication_record"}},"created_at":"2026-05-18T01:19:01.249949+00:00","updated_at":"2026-05-18T01:19:01.249949+00:00"}