Measuring Structural Parameters Through Stacking Galaxy Images

TL;DR

This paper evaluates the effectiveness of galaxy image stacking in recovering average structural parameters of faint high-redshift galaxies, highlighting biases and correction methods for accurate measurements.

Contribution

It introduces a simulation-based analysis of stacking techniques to quantify biases in recovering galaxy structural parameters, providing correction strategies.

Findings

Stacking can accurately recover mean galaxy profiles with biases.

Inclined galaxies cause overestimation of Sersic index and underestimation of Re.

Biases depend on the distributions of Re, AR, and n in galaxy samples.

Abstract

It remains challenging to detect the low surface brightness structures of faint high-z galaxies, which is key to understanding the structural evolution of galaxies. The technique of image stacking allows us to measure the averaged light profile beneath the detection limit and probe the extended structure of a group of galaxies. We carry out simulations to examine the recovery of the averaged surface brightness profile through stacking model HST/ACS images of a set of galaxies as functions of Sersic index (n), effective radius (Re) and axis ratio (AR). The Sersic profile best fitting the radial profile of the stacked image is taken as the recovered profile, in comparison with the intrinsic mean profile of the model galaxies. Our results show that, in general, the structural parameters of the mean profile can be properly determined through stacking, although systematic biases need to be corrected when spreads of Re and AR are counted. We find that Sersic index is slightly overestimated and Re is underestimated at AR < 0.5 as the stacked image appears to be more compact due to the presence of inclined galaxies; the spread of Re biases the stacked profile to have a higher Sersic index. We stress that the measurements of structural parameters through stacking should take these biases into account. We estimate the biases in the recovered structural parameters from stacks of galaxies when the samples have distributions of Re, AR and n seen in local galaxies.