Phan, Anh; Jensen, Joseph (Utah Valley University)
Faculty Advisor: Jensen, Joseph (Utah Valley University, Physics)
We have measured the Surface Brightness Fluctuation (SBF) distances to 12 galaxies. SBF is usually used to measure distances to giant elliptical galaxies that have uniform ages and composition. On the other hand, galaxies that are more disk-shaped potentially have a range of ages, they may have an SBF and color gradient. Elliptical masks that match the shapes of disk galaxies can give a more accurate SBF and color gradient than circular masks. The purpose of this study is to measure the discrepancies between the SBF distances using the two types of masks. For giant elliptical galaxies, the two methods give similar results ($\leq$ 2\%). For disk galaxies, the discrepancies are bigger (up to 6\% difference).