{"paper":{"title":"3.6 and 4.5 $\\mu$m Phase Curves of the Highly-Irradiated Eccentric Hot Jupiter WASP-14b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adam Burrows, Adam P. Showman, Andrew W. Howard, Benjamin J. Fulton, Drake Deming, Eric Agol, Gregory Laughlin, Heather A. Knutson, Ian Wong, Jean-Michel D\\'esert, Joel Schwartz, Jonathan J. Fortney, Jonathan Langton, Kamen Todorov, Nicolas B. Cowan, Nikole K. Lewis, Tiffany Kataria","submitted_at":"2015-05-12T20:02:21Z","abstract_excerpt":"We present full-orbit phase curve observations of the eccentric ($e\\sim 0.08$) transiting hot Jupiter WASP-14b obtained in the 3.6 and 4.5 $\\mu$m bands using the \\textit{Spitzer Space Telescope}. We use two different methods for removing the intrapixel sensitivity effect and compare their efficacy in decoupling the instrumental noise. Our measured secondary eclipse depths of $0.1882\\%\\pm 0.0048\\%$ and $0.2247\\%\\pm 0.0086\\%$ at 3.6 and 4.5 $\\mu$m, respectively, are both consistent with a blackbody temperature of $2402\\pm 35$ K. We place a $2\\sigma$ upper limit on the nightside flux at 3.6 $\\mu$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.03158","kind":"arxiv","version":2},"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"}