Extended Data Fig. 3: Spectra from the four individual reductions.
From: A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
Comparison of the brightness temperature spectra obtained by fitting with ExoTEP the four separate reductions and binned at a resolving power of R = 50. All data are plotted with their 1σ error bars. We overplot the best-fit SCARLET model (blue line) to the reductions for further comparison. All reductions are consistent within less than one standard deviation on average when compared at full resolution (408 bins).
