{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:UC77YDFNBPAJ464OSN6NT3KHAA","short_pith_number":"pith:UC77YDFN","schema_version":"1.0","canonical_sha256":"a0bffc0cad0bc09e7b8e937cd9ed470026de74525260d52b47edd14ffb540e40","source":{"kind":"arxiv","id":"1605.05091","version":1},"attestation_state":"computed","paper":{"title":"YETI observations of the young transiting planet candidate CVSO 30 b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Sota, C. Brice\\~no, Ch. Adam, Ch. Ginski, C. Marka, D. Kjurkchieva, D.P. Dimitrov, G. Maciejewski, H. Takahashi, J. Gelszinnis, J.G. Schmidt, J. Hern\\'andez, J. J. Downes, L. Holmes, L. Trepl, M. Fern\\'andez, M. Kitze, M.M. Hohle, M. Moualla, M. Mugrauer, M. Seeliger, N. Pawellek, R. Errmann, R. Neuh\\\"auser, S. Buder, S. Czesla, S. Masda, St. Raetz, T. Henych, T.Klocov\\'a, T.O.B. Schmidt, T. Pribulla, V. Radeva, X. Zhou, Z.-Y. Wu","submitted_at":"2016-05-17T10:16:08Z","abstract_excerpt":"CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possible young transiting planet orbiting a previously known weak-lined T-Tauri star. With five telescopes of the 'Young Exoplanet Transit Initiative' (YETI) located in Asia, Europe and South America we monitored CVSO 30 over three years in a total of 144 nights and detected 33 fading events. In two more seasons we carried out follow-up observations with three telescopes. We c"},"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":"1605.05091","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-05-17T10:16:08Z","cross_cats_sorted":[],"title_canon_sha256":"17b831a1fdea06a6158cebf4426bc9587491bb5d9bce0527325a425a4111602a","abstract_canon_sha256":"9acf4e8ffbc2bb8904700dccde751309ff34ab5345d146552433a29e380056e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:14:37.422345Z","signature_b64":"zJ/jhdRW0UKBTrvHkbqDouTAch+c4jBAC7a41MJe8jQJvLb5xvsIBjpCSzsCFJ6/Rn81zLbZS5NQ5Fmh7hnqBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a0bffc0cad0bc09e7b8e937cd9ed470026de74525260d52b47edd14ffb540e40","last_reissued_at":"2026-05-18T01:14:37.421568Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:14:37.421568Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"YETI observations of the young transiting planet candidate CVSO 30 b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Sota, C. Brice\\~no, Ch. Adam, Ch. Ginski, C. Marka, D. Kjurkchieva, D.P. Dimitrov, G. Maciejewski, H. Takahashi, J. Gelszinnis, J.G. Schmidt, J. Hern\\'andez, J. J. Downes, L. Holmes, L. Trepl, M. Fern\\'andez, M. Kitze, M.M. Hohle, M. Moualla, M. Mugrauer, M. Seeliger, N. Pawellek, R. Errmann, R. Neuh\\\"auser, S. Buder, S. Czesla, S. Masda, St. Raetz, T. Henych, T.Klocov\\'a, T.O.B. Schmidt, T. Pribulla, V. Radeva, X. Zhou, Z.-Y. Wu","submitted_at":"2016-05-17T10:16:08Z","abstract_excerpt":"CVSO 30 is a unique young low-mass system, because, for the first time, a close-in transiting and a wide directly imaged planet candidates are found around a common host star. The inner companion, CVSO 30 b, is the first possible young transiting planet orbiting a previously known weak-lined T-Tauri star. With five telescopes of the 'Young Exoplanet Transit Initiative' (YETI) located in Asia, Europe and South America we monitored CVSO 30 over three years in a total of 144 nights and detected 33 fading events. In two more seasons we carried out follow-up observations with three telescopes. We c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.05091","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":"1605.05091","created_at":"2026-05-18T01:14:37.421695+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.05091v1","created_at":"2026-05-18T01:14:37.421695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.05091","created_at":"2026-05-18T01:14:37.421695+00:00"},{"alias_kind":"pith_short_12","alias_value":"UC77YDFNBPAJ","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"UC77YDFNBPAJ464O","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"UC77YDFN","created_at":"2026-05-18T12:30:46.583412+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/UC77YDFNBPAJ464OSN6NT3KHAA","json":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA.json","graph_json":"https://pith.science/api/pith-number/UC77YDFNBPAJ464OSN6NT3KHAA/graph.json","events_json":"https://pith.science/api/pith-number/UC77YDFNBPAJ464OSN6NT3KHAA/events.json","paper":"https://pith.science/paper/UC77YDFN"},"agent_actions":{"view_html":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA","download_json":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA.json","view_paper":"https://pith.science/paper/UC77YDFN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.05091&json=true","fetch_graph":"https://pith.science/api/pith-number/UC77YDFNBPAJ464OSN6NT3KHAA/graph.json","fetch_events":"https://pith.science/api/pith-number/UC77YDFNBPAJ464OSN6NT3KHAA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA/action/storage_attestation","attest_author":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA/action/author_attestation","sign_citation":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA/action/citation_signature","submit_replication":"https://pith.science/pith/UC77YDFNBPAJ464OSN6NT3KHAA/action/replication_record"}},"created_at":"2026-05-18T01:14:37.421695+00:00","updated_at":"2026-05-18T01:14:37.421695+00:00"}