Galaxy Merger Fractions in Two Clusters at Using the Hubble Space Telescope

We measure the fraction of galaxy–galaxy mergers in two clusters at z ∼ 2 using imaging and grism observations from the Hubble Space Telescope. The two galaxy cluster candidates were originally identified as overdensities of objects using deep mid-infrared imaging and observations from the Spitzer Space Telescope, and were subsequently followed up with HST/WFC3 imaging and grism observations. We identify galaxy–galaxy merger candidates using high-resolution imaging with the WFC3 in the F105W, F125W, and F160W bands. Coarse redshifts for the same objects are obtained with grism observations in G102 for the z ∼ 1.6 cluster (IRC0222A) and G141 for the z ∼ 2 cluster (IRC0222B). Using visual classifications as well as a variety of selection techniques, we measure merger fractions of in IRC0222A and in IRC0222B. In comparison, we measure a merger fraction of for field galaxies at z ∼ 2. Our study indicates that the galaxy–galaxy merger fraction in clusters at z ∼ 2 is enhanced compared to the field population, but note that more cluster measurements at this epoch are needed to confirm our findings.