{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:R5WAQ2OZH4DU6H7P6Y5UDMAP67","short_pith_number":"pith:R5WAQ2OZ","schema_version":"1.0","canonical_sha256":"8f6c0869d93f074f1feff63b41b00ff7cc11118a0ec04e10c018976218942faf","source":{"kind":"arxiv","id":"1712.04324","version":1},"attestation_state":"computed","paper":{"title":"HATS-50b through HATS-53b: four transiting hot Jupiters orbiting G-type stars discovered by the HATSouth survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jordan, A. W. Howard, B. J. Fulton, C. G. Tinney, D. Bayliss, D. J. Wright, G. A. Bakos, G. W. Marcy, G. Zhou, H. T. Isaacson, I. Papp, J. Bento, J. D. Hartman, J. Lazar, K. Penev, L. Mancini, M. de Val-Borro, M. Rabus, N. Espinoza, P. Sari, P. Sarkis, R. Brahm, S. Ciceri, S. Durkan, T. G. Tan, Th. Henning, V. Suc, W. Bhatti, Z. Csubry","submitted_at":"2017-12-12T14:52:55Z","abstract_excerpt":"We report the discovery of four close-in transiting exoplanets, HATS-50 through HATS-53, discovered using the HATSouth three-continent network of homogeneous and automated telescopes. These new exoplanets belong to the class of hot Jupiters and orbit G-type dwarf stars, with brightness in the range V=12.5-14.0 mag. While HATS-53 has many physical characteristics similar to the Sun, the other three stars appear to be metal rich, larger and more massive. Three of the new exoplanets, namely HATS-50, HATS-51 and HATS-53, have low density and similar orbital period. Instead, HATS-52 is more dense a"},"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":"1712.04324","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-12-12T14:52:55Z","cross_cats_sorted":[],"title_canon_sha256":"6713b38a7a0b9582b54afbfa701df05b26d223f54b058efc8ea4c97e101f28d7","abstract_canon_sha256":"a20a0ca588a2482e07dfe025f9e7bb802c3ab177bfab2d5a0aa5b80e26875dfd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:59.322304Z","signature_b64":"a7/tjwvPRB32oqSdaYr/Ic+/hNV2b+j/zXlbHOBkwNFSIa1lGh7dkLFZAD91TppwXqNeGCRGSwxvB9sCrPhPDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f6c0869d93f074f1feff63b41b00ff7cc11118a0ec04e10c018976218942faf","last_reissued_at":"2026-05-18T00:24:59.321786Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:59.321786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HATS-50b through HATS-53b: four transiting hot Jupiters orbiting G-type stars discovered by the HATSouth survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jordan, A. W. Howard, B. J. Fulton, C. G. Tinney, D. Bayliss, D. J. Wright, G. A. Bakos, G. W. Marcy, G. Zhou, H. T. Isaacson, I. Papp, J. Bento, J. D. Hartman, J. Lazar, K. Penev, L. Mancini, M. de Val-Borro, M. Rabus, N. Espinoza, P. Sari, P. Sarkis, R. Brahm, S. Ciceri, S. Durkan, T. G. Tan, Th. Henning, V. Suc, W. Bhatti, Z. Csubry","submitted_at":"2017-12-12T14:52:55Z","abstract_excerpt":"We report the discovery of four close-in transiting exoplanets, HATS-50 through HATS-53, discovered using the HATSouth three-continent network of homogeneous and automated telescopes. These new exoplanets belong to the class of hot Jupiters and orbit G-type dwarf stars, with brightness in the range V=12.5-14.0 mag. While HATS-53 has many physical characteristics similar to the Sun, the other three stars appear to be metal rich, larger and more massive. Three of the new exoplanets, namely HATS-50, HATS-51 and HATS-53, have low density and similar orbital period. Instead, HATS-52 is more dense a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.04324","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":"1712.04324","created_at":"2026-05-18T00:24:59.321852+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.04324v1","created_at":"2026-05-18T00:24:59.321852+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.04324","created_at":"2026-05-18T00:24:59.321852+00:00"},{"alias_kind":"pith_short_12","alias_value":"R5WAQ2OZH4DU","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_16","alias_value":"R5WAQ2OZH4DU6H7P","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_8","alias_value":"R5WAQ2OZ","created_at":"2026-05-18T12:31:39.905425+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/R5WAQ2OZH4DU6H7P6Y5UDMAP67","json":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67.json","graph_json":"https://pith.science/api/pith-number/R5WAQ2OZH4DU6H7P6Y5UDMAP67/graph.json","events_json":"https://pith.science/api/pith-number/R5WAQ2OZH4DU6H7P6Y5UDMAP67/events.json","paper":"https://pith.science/paper/R5WAQ2OZ"},"agent_actions":{"view_html":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67","download_json":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67.json","view_paper":"https://pith.science/paper/R5WAQ2OZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.04324&json=true","fetch_graph":"https://pith.science/api/pith-number/R5WAQ2OZH4DU6H7P6Y5UDMAP67/graph.json","fetch_events":"https://pith.science/api/pith-number/R5WAQ2OZH4DU6H7P6Y5UDMAP67/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67/action/storage_attestation","attest_author":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67/action/author_attestation","sign_citation":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67/action/citation_signature","submit_replication":"https://pith.science/pith/R5WAQ2OZH4DU6H7P6Y5UDMAP67/action/replication_record"}},"created_at":"2026-05-18T00:24:59.321852+00:00","updated_at":"2026-05-18T00:24:59.321852+00:00"}