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Lyman Alpha Emitters for High-redshift Cosmology

Cosmology, Physical Cosmology and seminar by Haruki Ebina, University of California, Berkeley

Hosted by Perimeter Institute Recorded Seminar Archive

Tuesday 13:00 UTC

Recording available

Waterloo, Canada
Related content

Recording

56 min

Abstract

Lyman-alpha galaxies offer a way to map structure beyond redshift two and connect galaxy surveys with microwave-background lensing. This talk demonstrates selection from IBIS medium-band images and spectroscopic follow-up with DESI. Joint clustering measurements of these galaxies and quasars constrain bias, small-scale velocity effects and radiative-transfer contributions, testing the modelling needed for future high-redshift surveys.

Topics

Lyman-alpha galaxiesredshift twoIBIS medium-band imagesDESIspectroscopic follow-upmicrowave-background lensingJoint clustering measurementsquasarssmall-scale velocity effectsradiative-transfer contributions