PIRSA:18050012

Video URL

https://pirsa.org/18050012

Lensing reconstruction using line intensity maps

Foreman, S. (2018). Lensing reconstruction using line intensity maps. Perimeter Institute for Theoretical Physics. https://pirsa.org/18050012

Foreman, Simon. Lensing reconstruction using line intensity maps. Perimeter Institute for Theoretical Physics, May. 01, 2018, https://pirsa.org/18050012 

          @misc{ scivideos_PIRSA:18050012,
            doi = {10.48660/18050012},
            url = {https://pirsa.org/18050012},
            author = {Foreman, Simon},
            keywords = {Cosmology},
            language = {en},
            title = {Lensing reconstruction using line intensity maps},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2018},
            month = {may},
            note = {PIRSA:18050012 see, \url{https://scivideos.org/pirsa/18050012}}
          }

Simon Foreman Arizona State University

Talk numberPIRSA:18050012
DOI10.48660/18050012
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Gravitational lensing of the cosmic microwave background has emerged as a powerful cosmological probe, made possible by the development and characterization of nearly-optimal estimators for extracting the lensing signal from temperature and polarization maps. One can ask whether similar tools can be applied to upcoming "intensity maps" of emission lines at other wavelengths (e.g. 21cm). In this talk, I will present recent work in this direction, focusing in particular on the impact of gravitational nonlinearities on standard quadratic lensing estimators. I will show how these nonlinearities can provide a significant contaminant to lensing reconstruction, even for observations at reionization-era redshifts, but will also describe how this contamination can largely be mitigated by modifying the lensing estimator. Finally, I will present estimates for the detectability of lensing in ongoing and future intensity mapping surveys.