We present DARKNESS (the DARK-speckle Near-infrared Energy-resolving Superconducting Spectrophotometer), the first of several planned integral field spectrographs to use optical/near-infrared Microwave Kinetic Inductance Detectors (MKIDs) for high-contrast imaging. The photon counting and simultaneous low-resolution spectroscopy provided by MKIDs will enable real-time speckle control techniques and post-processing speckle suppression at frame rates capable of resolving the atmospheric speckles that currently limit high-contrast imaging from the ground. DARKNESS is now operational behind the PALM-3000 extreme adaptive optics system and the Stellar Double Coronagraph at Palomar Observatory. Here, we describe the motivation, design, and characterization of the instrument, early on-sky results, and future prospects.
CITATION STYLE
Meeker, S. R., Mazin, B. A., Walter, A. B., Strader, P., Fruitwala, N., Bockstiegel, C., … Serabyn, E. (2018). DARKNESS: A microwave kinetic inductance detector integral field spectrograph for high-contrast astronomy. Publications of the Astronomical Society of the Pacific, 130(988). https://doi.org/10.1088/1538-3873/aab5e7
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