THE MERGER-DRIVEN EVOLUTION OF MASSIVE GALAXIES af 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 af 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? af 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 af 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 af 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 af 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