Direct Measurement of Intrinsic Alignments with DESI
Intrinsic alignments are a limiting systematic for cosmic shear studies;
coherent distortions from lensing by foreground structure must be separated from correlations between galaxy shapes and the local density field.
We make direct measurements of intrinsic alignments using spectroscopy from the first year of the DESI Survey and imaging from four lensing surveys: DES, HSC, KiDS, and SDSS.
These measurements will inform novel modeling of intrinsic alignments for cosmic shear and the optimal selection of blue weakly aligned galaxies.
With Alex Amon, Jamie McCullough, and the DESI collaboration.