29 Oct 2013: The time of secondary eclipse is given in the table for the 3.6 micron eclipse. For The 4.6 micron secondary eclipse it is 2456182.62027 ± 0.001 (Beatty et al. 2013).
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Spitzer Phase Curves of KELT-1b and the Signatures of Nightside Clouds in Thermal Phase Observations
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The DOHA algorithm: a new recipe for cotrending large-scale transiting exoplanet survey light curves
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Exploration of the brown dwarf regime around solar-like stars by CoRoT
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The Broadband and Spectrally-Resolved H-band Eclipse of KELT-1b and the Role of Surface Gravity in Stratospheric Inversions in Hot Jupiters
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Spitzer and z' Secondary Eclipse Observations of the Highly Irradiated Transiting Brown Dwarf KELT-1b
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Near-infrared Thermal Emission Detections of a number of hot Jupiters and the Systematics of Ground-based Near-infrared Photometry
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KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star
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