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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. 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