  Current time-domain wide-field sky surveys generally operate with
few-degree-sized fields and take many individual images to cover large sky
areas each night. We present the design and project status of the Evryscope
("wide-seer"), which takes a different approach: using an array of 7cm
telescopes to form a single wide-field-of-view pointed at every part of the
accessible sky simultaneously and continuously. The Evryscope is a
gigapixel-scale imager with a 9060 sq. deg. field of view and has an etendue
three times larger than the Pan-STARRS sky survey. The system will search for
transiting exoplanets around bright stars, M-dwarfs and white dwarfs, as well
as detecting microlensing events, nearby supernovae, and gamma-ray burst
afterglows. We present the current project status, including an update on the
Evryscope prototype telescopes we have been operating for the last three years
in the Canadian High Arctic.
