{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:PIS4LTNX3H2I7FEBURAX5WFHFW","short_pith_number":"pith:PIS4LTNX","schema_version":"1.0","canonical_sha256":"7a25c5cdb7d9f48f9481a4417ed8a72db6a23078dc0e57c87cc5a66e219072ce","source":{"kind":"arxiv","id":"1608.04225","version":1},"attestation_state":"computed","paper":{"title":"WASP-86b and WASP-102b: super-dense versus bloated planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Collier Cameron, A. H. M. Triaud, A. J. Norton, A. P. Doyle, A. Scholz, B. Smalley, C. A. Haswell, C. Hellier, D. Anderson, D. J. A. Brown, D. J. Armstrong, D. Pollacco, D. Queloz, D. S\\'egransan, D. Veras, E. Palle, F. Bouchy, F. Faedi, F. Pepe, G. H\\'ebrard, H. P. Osborn, I. Boisse, I. Plauchu-Frayn, J. McCormac, J. Prieto-Arranz, K. L. Hay, K. W. F. Lam, L. Mancini, M. Gillon, M. Lendl, M. R. Goad, P. A. Wilson, P. Boumis, P. F. L. Maxted, P. J. Wheatley, R. Street, R. West, S. C. C. Barros, S. Udry, U. Kolb, Y. G\\'omez Maqueo Chew","submitted_at":"2016-08-15T10:19:26Z","abstract_excerpt":"We report the discovery of two transiting planetary systems: a super dense, sub-Jupiter mass planet WASP-86b (\\mpl\\ = 0.82 $\\pm$ 0.06 \\mj, \\rpl\\ = 0.63 $\\pm$ 0.01 \\rj), and a bloated, Saturn-like planet WASP-102b (\\mpl\\ = 0.62 $\\pm$ 0.04 \\mj, \\rpl\\=1.27 $\\pm$ 0.03 \\rj). They orbit their host star every $\\sim$5.03, and $\\sim$2.71 days, respectively. The planet hosting WASP-86 is a F7 star (\\teff\\ = 6330$\\pm$110 K, \\feh\\ = $+$0.23 $\\pm$ 0.14 dex, and age $\\sim$0.8--1~Gyr), WASP-102 is a G0 star (\\teff\\ = 5940$\\pm$140 K, \\feh\\ = $-$0.09$\\pm$ 0.19 dex, and age $\\sim$1~Gyr). These two systems highl"},"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":"1608.04225","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-08-15T10:19:26Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"9d9d7b875229532ebb4677b3224766b613dbd58b417f11478250de3e48a025b8","abstract_canon_sha256":"cdcdf3e30259e0416863d730b9ac16b7522571791e8e2c48d14c304409fc283c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:04.034628Z","signature_b64":"+kQ1MYRWBZI2tVAJyXDk5l6bhxDlL5b9Zdwv0xkIIgYR7ht0DpVAqYWOcgZZ4pckEphz5w3nNtmK4hsH9CyMBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a25c5cdb7d9f48f9481a4417ed8a72db6a23078dc0e57c87cc5a66e219072ce","last_reissued_at":"2026-05-18T01:09:04.034251Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:04.034251Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"WASP-86b and WASP-102b: super-dense versus bloated planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. Collier Cameron, A. H. M. Triaud, A. J. Norton, A. P. Doyle, A. Scholz, B. Smalley, C. A. Haswell, C. Hellier, D. Anderson, D. J. A. Brown, D. J. Armstrong, D. Pollacco, D. Queloz, D. S\\'egransan, D. Veras, E. Palle, F. Bouchy, F. Faedi, F. Pepe, G. H\\'ebrard, H. P. Osborn, I. Boisse, I. Plauchu-Frayn, J. McCormac, J. Prieto-Arranz, K. L. Hay, K. W. F. Lam, L. Mancini, M. Gillon, M. Lendl, M. R. Goad, P. A. Wilson, P. Boumis, P. F. L. Maxted, P. J. Wheatley, R. Street, R. West, S. C. C. Barros, S. Udry, U. Kolb, Y. G\\'omez Maqueo Chew","submitted_at":"2016-08-15T10:19:26Z","abstract_excerpt":"We report the discovery of two transiting planetary systems: a super dense, sub-Jupiter mass planet WASP-86b (\\mpl\\ = 0.82 $\\pm$ 0.06 \\mj, \\rpl\\ = 0.63 $\\pm$ 0.01 \\rj), and a bloated, Saturn-like planet WASP-102b (\\mpl\\ = 0.62 $\\pm$ 0.04 \\mj, \\rpl\\=1.27 $\\pm$ 0.03 \\rj). They orbit their host star every $\\sim$5.03, and $\\sim$2.71 days, respectively. 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