© public
CHIME is a transit interferometer with no moving parts, which uses a massive computing backend to image the radio sky from 400-800MHz, corresponding to 21cm radiation emanating from a redshift range of 0.8 < z < 2.5. Earth rotation sweeps its field of view across the sky, resulting in complete daily coverage of the northern celestial hemisphere and an unprecedented survey sensitivity. I will discuss the motivation, construction, and status of CHIME, as well as a pair of extensions which probe the high-cadence time-domain radio sky, monitoring radio pulsars and exploring a more recent mystery in radio astronomy, Fast Radio Bursts. Looking forward, I will present the technology path towards adding FRB localization capabilities to CHIME, and the new wide-band CHORD telescope, presently under development in Canada.