The Circumgalactic Hα Spectrograph (CHαS) is a new narrowband integral field spectrograph optimized for observing faint emission from the ionized circumgalactic medium (CGM) of nearby galaxies. CHαS is deployed on the 2.4m Hiltner telescope at MDM Observatory in Arizona, where we are conducting an initial science survey collecting deep spectral imaging of 10 galaxies in Ha emission. Here we debut the commissioning of a blue channel, extending the spectral coverage to include Hβ and OIII emission. We present modeling for new narrowband filters that can tilt in order to center on different wavelengths, expanding our range of observable redshifts while limiting spectral overlap. Finally, we discuss the development of an actuated lenslet array mount to precisely shift the lenslet array across the focal plane, offsetting instrument flexure. CHαS will be an ideal test-bed for new focal plane and detector technologies as we develop it into a facility instrument at MDM Observatory.
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