This program is motivated by the recent observational insights concerning white dwarfs as individuals and as a population, based on the astrometry from Gaia and large photometric (e.g. Kepler,TESS, ZTF) and spectroscopic...

Astrometric, photometric and spectroscopic all-sky surveys provide the first complete, unbiased view of the Galactic population of the most abundant type of stellar remnants: white dwarfs.

A workshop to further explore science cases for KWFI

The Keck Wide-Field Imager (KWFI) is a proposed prime focus camera mounted on the Keck telescopes and will be the world’s most sensitive wide-field optical imager...

Join co-organizers Blakesley Burkhart, Mike Shelley and David Spergel in an interactive workshop held at the Flatiron Institute in New York City 2-6 December entitled, Universality: Turbulence Across Vast Scales.