Description
Window Convolution & Interloper Modeling in the Euclid Data Analysis
The power spectrum of the spectroscopic galaxy catalog is one of the main observables of the Euclid mission.
I will discuss possible systematic errors directly related to the adopted estimator and its implementation.
I will quantify their contribution to the overall error budget and compare it to the expected statistical error for the full mission.
In addition, I will discuss the impact of line and noise interlopers that might be important for Euclid results.
