Speaker
Alvise Raccanelli
(University of Padova)
Description
Future surveys will measure galaxy clustering on unexplored regimes and with better than ever precision.
In my talk I will discuss some investigations on how this precision will be wasted if not matched by a comparable level of accuracy.
I will present the recent developement of a formalism for including radial modes information and new observables based on it.
Furthermore, I will show studies quantifying the mis-estimation of cosmological parameters when taking approximations that were acceptable until now but will not be for future surveys.
Finally, I will present a new proposal for a galaxy survey measuring the clustering at very high redshift.
Primary author
Alvise Raccanelli
(University of Padova)
