Speaker
András Kovács
(Konkoly Observatory)
Description
The ISW and gravitational lensing signals of cosmic large-scale structures probe the growth of structure in the low-redshift cosmic web. In this talk, I will summarise the recent results on detecting cosmic voids in the galaxy distribution, and their cross-correlations with CMB lensing and temperature maps, using different surveys such as DES, DESI, Euclid, Pan-STARRS, and also Gaia quasars. I will also explain how we are using the Gower St simulations with hundreds of different cosmologies to build a new modelling framework for cosmological constraints using cosmic voids.
Author
András Kovács
(Konkoly Observatory)
