{"paper":{"title":"High-precision multi-wavelength eclipse photometry of the ultra-hot gas giant exoplanet WASP-103 b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Burdanov, A. Collier-Cameron, A. H. M. J. Triaud, B.-O. Demory, B. Smalley, C. Hellier, D. Queloz, D. R. Anderson, E. Jehin, F. Bouchy, L. Delrez, M. Gillon, M. Lendl, M. Neveu-VanMalle, N. Madhusudhan, P. F. L. Maxted, P. Magain","submitted_at":"2017-11-07T15:45:09Z","abstract_excerpt":"We present sixteen occultation and three transit light curves for the ultra-short period hot Jupiter WASP-103 b, in addition to five new radial velocity measurements. We combine these observations with archival data and perform a global analysis of the resulting extensive dataset, accounting for the contamination from a nearby star. We detect the thermal emission of the planet in both the $z'$ and $K_{\\mathrm{S}}$-bands, the measured occultation depths being 699$\\pm$110 ppm (6.4-$\\sigma$) and $3567_{-350}^{+400}$ ppm (10.2-$\\sigma$), respectively. We use these two measurements together with re"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.02566","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"}