We describe a laboratory facility and experimental testbed that supports the emulation of a wide range of mission concepts such as gravitational
weak lensing measurements by WFIRST and high precision spectrophotometry of transiting exoplanets by JWST.
Not exact matches
Taking models of galaxies from the Hubble Space Telescope Ultra Deep Field (HUDF) and applying a correction for the HUDF point spread function we generate
lensed simulations of deep, opti... ▽ More We present a simulation analysis of
weak gravitational
lensing flexion and shear
measurement using shapelet decomposition, and identify differences between flexion and shear
measurement noise in deep survey data.
Abstract: We present a simulation analysis of
weak gravitational
lensing flexion and shear
measurement using shapelet decomposition, and identify differences between flexion and shear
measurement noise in deep survey data.
Weak lensing cosmology will be challenging: in addition to highly accurate galaxy shape measurements, statistically robust and accurate photometric redshift (photo - z) estimates for billions of faint galaxies will... ▽ More A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the growth of structure with cosmic time from weak lensing analysis over large regions of the
Weak lensing cosmology will be challenging: in addition to highly accurate galaxy shape
measurements, statistically robust and accurate photometric redshift (photo - z) estimates for billions of faint galaxies will... ▽ More A key goal of the Stage IV dark energy experiments Euclid, LSST and WFIRST is to measure the growth of structure with cosmic time from
weak lensing analysis over large regions of the
weak lensing analysis over large regions of the sky.