Speaker
Theo Steele
(University of Sussex)
Description
Large scale structure correlators will be one of the most important probes of fundamental physics in the years to come. The results of redshift surveys which are used to measure these correlators sort their results into redshift bins for convenient analysis. In this short talk, we will discuss the implementation of corrections to account for differences in redshift between observables in the context of what we call field and spectrum level projections, which are built upon Fourier transforming expansions around assumed redshifts and deriving correlators from the ensuing fields.
Primary authors
Theo Steele
(University of Sussex)
Zvonimir Vlah
(Ruder Boskovic Institute and the University of Cambridge)
Alvise Raccanelli
(University of Padova and the Theoretical Physics Department at CERN)
