Daniel Scolnic, University of Chicago, "What's Next for Cosmology with Type Ia Supernovae"
KICP seminar: February 27, 2015 @ 12PM
We are currently in the midst of a huge explosion in the number of Type Ia Supernovae we've found to better determine cosmological parameters. With the release of Pan-STARRs data, the start of the Dark Energy Survey, and multiple surveys at both low and high-redshift, our statistics will soon improve by an order of magnitude.