http://arxiv.org/pdf/1407.0026.pdf
Most current general time-domain sky surveys (e.g. the Palomar Transient Factory, Pan-STARRS, SkyMapper, CRTS, ATLAS) image thousands of square degrees each night in few-degree-wide segments and use large apertures to achieve deep imaging in those areas. The resulting survey is necessarily optimized for events such as supernovae that occur on day-or-longer timescales. However, these surveys are not sensitive to the very diverse class of shorter-timescale objects, including transiting exoplanets, young stellar variability, eclipsing binaries, microlensing planet events, gamma ray bursts, young supernovae, and other exotic transients.
To reach these rare short-timescale events we are building an instrument that takes a different approach. 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 Wideseer, which usies 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.