12-13 May 2017; Columbia University, Pupin Hall
A workshop will be held at Columbia University to begin the scientific preparation for the detection of optical counterparts of gravitational wave events with LSST. LSST is uniquely suited to find optical counterparts of gravitational waves. Gravitational waves have been detected at high significance by LIGO. Observation of optical counterparts of gravitational wave events, including mergers of black holes and neutron stars as well as other phenomena will provide a more precise measurement on the direction, redshift and other properties of the event, necessary for its full characterization. This is essential for testing cosmology, general relativity and probing the properties of matter at supranuclear densities in neutron stars.
LSSTC Support: $4,800