THE MERGER-DRIVEN EVOLUTION OF MASSIVE GALAXIES by Robaina, A, Bell, E, van der Wel, A, Somerville, R, Skelton, R, McIntosh, D, Meisenheimer, K, Wolf, C

HISTORY OF GALAXY INTERACTIONS AND THEIR IMPACT ON STAR FORMATION OVER THE LAST 7 Gyr FROM GEMS by Jogee, S, Miller, S, Penner, K, Skelton, R, Conselice, C, Somerville, R, Bell, E, Zheng, X, Rix, H, Robaina, A, Barazza, F, Barden, M, Borch, A, Beckwith, S, Caldwell, J, Peng, C, Heymans, C, McIntosh, D, Haeussler, B, Jahnke, K, Meisenheimer, K, Sanchez, S, Wisotzki, L, Wolf, C, Papovich, C

AGN host galaxies at redshift z~0.7: peculiar or not? by Boehm, A, Wisotzki, L, Bell, E, Jahnke, K, Wolf, C, Bacon, D, Barden, M, Gray, M, Hoeppe, G, Jogee, S, McIntosh, D, Peng, C, Robaina, A, Balogh, M, Barazza, F, Caldwell, J, Heymans, C, Haeussler, B, Kampen, E, Lane, K, Meisenheimer, K, Sanchez, S, Taylor, A, Zheng, X

Exploring the Impact of Galaxy Interactions over Seven Billion Years with CAS by Miller, S, Jogee, S, Conselice, C, Penner, K, Bell, E, Zheng, X, Papovich, C, Skelton, R, Somerville, R, Rix, H, Barazza, F, Barden, M, Borch, A, Beckwith, S, Caldwell, J, Haeussler, B, Heymans, C, Jahnke, K, McIntosh, D, Meisenheimer, K, Peng, C, Robaina, A, Sanchez, S, Wisotzki, L, Wolf, C

Obscured star formation in intermediate-density environments: A Spitzer study of the Abell 901/902 supercluster by Gallazzi, A, Bell, E, Wolf, C, Gray, M, Papovich, C, Barden, M, Peng, C, Meisenheimer, K, Heymans, C, Kampen, E, Gilmour, R, Balogh, M, McIntosh, D, Bacon, D, Barazza, F, Boehm, A, Caldwell, J, Haeussler, B, Jahnke, K, Jogee, S, Lane, K, Robaina, A, Sanchez, S, Taylor, A, Wisotzki, L

LESS THAN 10 PERCENT OF STAR FORMATION IN z similar to 0.6 MASSIVE GALAXIES IS TRIGGERED BY MAJOR INTERACTIONS by Robaina, A, Bell, E, Skelton, R, McIntosh, D, Somerville, R, Zheng, X, Rix, H, Bacon, D, Balogh, M, Barazza, F, Barden, M, Boehm, A, Caldwell, J, Gallazzi, A, Gray, M, Haeussler, B, Heymans, C, Jahnke, K, Jogee, S, van Kampen, E, Lane, K, Meisenheimer, K, Papovich, C, Peng, C, Sanchez, S