adsabs/AstroCLIMB huggingface dataset:
Paper: ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
Authors: Chima D. McGruder, Mercedes López-Morales, James Kirk, Néstor Espinoza, Benjamin V. Rackham, Munazza K. Alam, Natalie Allen, Nikolay Nikolov, Ian C. Weaver, Kevin Ortiz Ceballos, David J. Osip, Dániel Apai, Andrés Jordán, Jonathan J. Fortney
Figure caption: The process used to correct for second-order light. The left panel shows the normalized IMACS observations taken on UT170804, which had no filter (red); UT170804 convolved with the GG495 transmission profile (green); and UT171108, which had the GG495 filter (blue). The middle panel shows the normalized second-order light correction, determined by dividing the filter convolved first night (green) by the second night (blue). The right panel shows normalized UT170804 (red), UT170804 convolved with the GG495 profile and corrected for second-order light (green), and UT171108 (blue). Dotted lines representing the modeled continua of each spectrum are overlaid in the same respective colors as their spectra. These steps are also applied to each comparison, so every spectrum is corrected from second-order light.