A number of major new and near future survey facilities are set to have a large impact on cool star science. With increased sky coverage and sensitivity over a wide wavelength range and in the time domain, a variety of new populations will be discovered. We discuss the capabilities of these new surveys and some of the science they will facilitate in the coming years.
|Title of host publication||In: Procs of the 14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun - ASP Conference Series 384|
|Publisher||Astronomical Society of the Pacific|
|ISBN (Print)||978-1-58381-332-4, 978-1-58381-331-7|
|Publication status||Published - 2008|