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Van Grootel","submitted_at":"2013-12-06T10:47:53Z","abstract_excerpt":"We report the discovery by the WASP transit survey of three new hot Jupiters, WASP-68 b, WASP-73 b and WASP-88 b. WASP-68 b has a mass of 0.95+-0.03 M_Jup, a radius of 1.24-0.06+0.10 R_Jup, and orbits a V=10.7 G0-type star (1.24+-0.03 M_sun, 1.69-0.06+0.11 R_sun, T_eff=5911+-60 K) with a period of 5.084298+-0.000015 days. Its size is typical of hot Jupiters with similar masses. WASP-73 b is significantly more massive (1.88-0.06+0.07 M_Jup) and slightly larger (1.16-0.08+0.12 R_Jup) than Jupiter. It orbits a V=10.5 F9-type star (1.34-0.04+0.05 M_sun, 2.07-0.08+0.19 R_sun, T_eff=6036+-120 K) eve"},"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":"1312.1827","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-12-06T10:47:53Z","cross_cats_sorted":[],"title_canon_sha256":"d599e3aedb4bb437759d5cf8ed8772402a90b9997579f01bdf8bd3e3ac75d700","abstract_canon_sha256":"099da00a254c063832d2877242927f7cb1fc98884c98425f6b0d5b2df2ad53f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:57.892652Z","signature_b64":"6WQOfkzryPHvi7cS71Lyqkb7LIyU/EAtHFN0/ZqhFKZ5nMnWcYMOpcdXjS93d276cuPhHCNbFFkQPNv09v6/Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ba24dff4b1131c860a5b389f855fafc5d52bd90bcdcc175ab8aca560b38215f","last_reissued_at":"2026-05-18T01:45:57.892038Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:57.892038Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Transiting planets from WASP-South, Euler and TRAPPIST: WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Collier-Cameron, A. Fumel, A. H. M. J. Triaud, A. M. S. Smith, A. P. Doyle, B. Smalley, C. Hellier, D. Pollacco, D. Queloz, D. R. Anderson, D. S\\'egransan, E. Jehin, F. Pepe, J. Southworth, L. Delrez, M. Gillon, M. Lendl, M. Neveu-VanMalle, P. F. L. Maxted, R. G. West, S. Udry, V. Van Grootel","submitted_at":"2013-12-06T10:47:53Z","abstract_excerpt":"We report the discovery by the WASP transit survey of three new hot Jupiters, WASP-68 b, WASP-73 b and WASP-88 b. WASP-68 b has a mass of 0.95+-0.03 M_Jup, a radius of 1.24-0.06+0.10 R_Jup, and orbits a V=10.7 G0-type star (1.24+-0.03 M_sun, 1.69-0.06+0.11 R_sun, T_eff=5911+-60 K) with a period of 5.084298+-0.000015 days. Its size is typical of hot Jupiters with similar masses. WASP-73 b is significantly more massive (1.88-0.06+0.07 M_Jup) and slightly larger (1.16-0.08+0.12 R_Jup) than Jupiter. 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