An independent wavelet-based reanalysis of WASP43 b's Spitzer phase curves finds higher nightside flux, smaller hotspot offsets, and consistency with atmospheric circulation models and a prior reanalysis.
E., Thomas Megeath, S., et al
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An independent analysis of the Spitzer/IRAC phase curves of WASP43 b
An independent wavelet-based reanalysis of WASP43 b's Spitzer phase curves finds higher nightside flux, smaller hotspot offsets, and consistency with atmospheric circulation models and a prior reanalysis.