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Near-Infrared Studies of Substellar Companions

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Figure 2.1: Illustration of the differences between the CRIRES (left) and the multi-epoch (right) approaches
Figure 2.2: Representation of one night of CRIRES-style and multi-epoch style data.
Figure 2.3: Known planets from Exoplanets Data Explorer (www.exoplanets.org;
Figure 2.4: Multi-epoch simulations with the wavelength scale and saturated telluric positions taken directly from observed data vs
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Appendix Introduction Comparison to Data Appendix Discussion Instrumental Considerations Wavelength RegionWavelength Region Analytic Considerations Wavelength CalibrationWavelength Calibration Introduction Discussion

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