Kavli Affiliate: Patricia Burchat | Summary:Wavelength-dependent point spread functions (PSFs) violate an implicit assumption in current galaxy shape measurement algorithms that deconvolve the PSF measured from stars (which have stellar spectral energy distributions (SEDs)) from images of galaxies (which have galactic SEDs). Since the absorption length of silicon depends on wavelength, CCDs are a potential […]
Continue.. Chromatic CCD effects on weak lensing measurements for LSST