Shape, colour, and distance in weak gravitational flexion

Canonically, elliptical galaxies might be expected to have a perfect rotational symmetry, making them ideal targets for flexion studies - however, this assumption has not been tested. We have undertaken an analysis of low- and high-redshift galaxy catalogues of known morphological type with a new gravitational lensing code, Lenser. Using colour measurements in the u - r bands and fit Sersic index values, objects with characteristics consistent with early-type galaxies are found to have a lower intrinsic scatter in flexion signal than late-type galaxies. We find this measured flexion noise can be reduced by more than a factor of two at both low and high redshift.

Automated summary

The study found that objects with characteristics consistent with early-type galaxies have lower intrinsic scatter in flexion signal, while late-type galaxies have higher scatter. The measured flexion noise can be reduced by more than a factor of two at both low and high redshifts.