Image Details
Caption: Figure 8.
Panels (a)–(e): theoretical response to changing PWV levels for different spectral types in various NIR filters. Panel (f): the magnitude of the PWV response of an L6 dwarf calibrated to the response of a G0 in each filter. The second-order extinction effect is minimized in MKO J band.
© 2022. The Author(s). Published by the American Astronomical Society.