{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:ZT7NVJ4AF745CNV646Y2HGLIV6","short_pith_number":"pith:ZT7NVJ4A","schema_version":"1.0","canonical_sha256":"ccfedaa7802ff9d136bee7b1a39968afad667b2c9457fc6cccef7662fc2d82ba","source":{"kind":"arxiv","id":"1306.0624","version":1},"attestation_state":"computed","paper":{"title":"HATS-3b: An inflated hot Jupiter transiting an F-type star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jord\\'an, B. Addison, B. B\\'eky, B. Cs\\'ak, B. Schmidt, C. Tinney, D. Bayliss, D. Sasselov, D. Wright, G. Bakos, G. Zhou, I. Papp, J. Hartman, J. L\\'az\\'ar, K. Penev, L. Buchhave, L. Mancini, M. Mohler, M. Rabus, N. Espinoza, N. Nikolov, P. Conroy, P. Sackett, P. S\\'ari, R. Brahm, R. Noyes, T. Henning, V. Suc, Z. Csubry","submitted_at":"2013-06-04T00:00:43Z","abstract_excerpt":"We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V=12.4 F-dwarf star. HATS-3b has a period of P = 3.5479d, mass of Mp = 1.07MJ, and radius of Rp = 1.38RJ. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsini = 9.0km/s), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transit"},"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":"1306.0624","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-06-04T00:00:43Z","cross_cats_sorted":[],"title_canon_sha256":"a8bb576c834201983a8c3e70906415b7c362352e1e6abedda66864bef31ec694","abstract_canon_sha256":"3a63928a88e2294c2bf531e027215923ad06727fa964dd0678ea384ab94f8cfe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:33.334430Z","signature_b64":"WjeQj9XpzrWtCQLZeiW4WzHD1czNGQ4Uqy1svzSE0+zt6x7b0ZQQ5a7Pehc/ymUbS6BCQg6Phqscw1lmrID8Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ccfedaa7802ff9d136bee7b1a39968afad667b2c9457fc6cccef7662fc2d82ba","last_reissued_at":"2026-05-18T01:49:33.333952Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:33.333952Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HATS-3b: An inflated hot Jupiter transiting an F-type star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Jord\\'an, B. Addison, B. B\\'eky, B. Cs\\'ak, B. Schmidt, C. Tinney, D. Bayliss, D. Sasselov, D. Wright, G. Bakos, G. Zhou, I. Papp, J. Hartman, J. L\\'az\\'ar, K. Penev, L. Buchhave, L. Mancini, M. Mohler, M. Rabus, N. Espinoza, N. Nikolov, P. Conroy, P. Sackett, P. S\\'ari, R. Brahm, R. Noyes, T. Henning, V. Suc, Z. Csubry","submitted_at":"2013-06-04T00:00:43Z","abstract_excerpt":"We report the discovery by the HATSouth survey of HATS-3b, a transiting extrasolar planet orbiting a V=12.4 F-dwarf star. HATS-3b has a period of P = 3.5479d, mass of Mp = 1.07MJ, and radius of Rp = 1.38RJ. Given the radius of the planet, the brightness of the host star, and the stellar rotational velocity (vsini = 9.0km/s), this system will make an interesting target for future observations to measure the Rossiter-McLaughlin effect and determine its spin-orbit alignment. We detail the low/medium-resolution reconnaissance spectroscopy that we are now using to deal with large numbers of transit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.0624","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":"1306.0624","created_at":"2026-05-18T01:49:33.334015+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.0624v1","created_at":"2026-05-18T01:49:33.334015+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.0624","created_at":"2026-05-18T01:49:33.334015+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZT7NVJ4AF745","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZT7NVJ4AF745CNV6","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZT7NVJ4A","created_at":"2026-05-18T12:28:09.283467+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/ZT7NVJ4AF745CNV646Y2HGLIV6","json":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6.json","graph_json":"https://pith.science/api/pith-number/ZT7NVJ4AF745CNV646Y2HGLIV6/graph.json","events_json":"https://pith.science/api/pith-number/ZT7NVJ4AF745CNV646Y2HGLIV6/events.json","paper":"https://pith.science/paper/ZT7NVJ4A"},"agent_actions":{"view_html":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6","download_json":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6.json","view_paper":"https://pith.science/paper/ZT7NVJ4A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.0624&json=true","fetch_graph":"https://pith.science/api/pith-number/ZT7NVJ4AF745CNV646Y2HGLIV6/graph.json","fetch_events":"https://pith.science/api/pith-number/ZT7NVJ4AF745CNV646Y2HGLIV6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6/action/storage_attestation","attest_author":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6/action/author_attestation","sign_citation":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6/action/citation_signature","submit_replication":"https://pith.science/pith/ZT7NVJ4AF745CNV646Y2HGLIV6/action/replication_record"}},"created_at":"2026-05-18T01:49:33.334015+00:00","updated_at":"2026-05-18T01:49:33.334015+00:00"}