Galaxy And Mass Assembly (GAMA): Spectroscopic analysis by Hopkins, A, Driver, S, Brough, S, Owers, MS, Bauer, A, Gunawardhana, M, Cluver, M, Colless, M, Foster, C, Lara-Lopez, M, Roseboom, I, Sharp, R, Steele, O, Thomas, D, Baldry, I, Brown, M, Liske, J, Norberg, P, Robotham, A, Bamford, S, Bland-Hawthorn, J, Drinkwater, M, Loveday, J, Meyer, M, Peacock, J

“…The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spectra for up to ~300000 galaxies over 280 square degrees, to a limiting magnitude of r_pet < 19.8 mag. …”

Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, design and target catalogue by Davies, L, Robotham, A, Driver, S, Lagos, C, Cortese, L, Mannering, E, Foster, C, Lidman, C, Hashemizadeh, A, Koushan, S, O’Toole, S, Baldry, I, Bilicki, M, Bland-Hawthorn, J, Bremer, M, Brown, M, Bryant, J, Catinella, B, Croom, S, Grootes, M, Holwerda, B, Jarvis, M, Maddox, N, Meyer, M, Moffett, A, Phillipps, S, Taylor, E, Windhorst, R, Wolf, C

“…The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a large spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near and distant Universe by producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3 < z < 1.0). …”

The SAMI Galaxy Survey: The cluster redshift survey, target selection and cluster properties by Owers, MS, Allen, JT, Baldry, I, Bryant, JJ, Cecil, GN, Cortese, L, Croom, SM, Driver, SP, Fogarty, LMR, Green, AW, Helmich, E, de Jong, JTA, Kuijken, K, Mahajan, S, McFarland, J, Pracy, MB, Robotham, AGS, Sikkema, G, Sweet, S, Taylor, EN, Kleijn, G, Bauer, AE, Bland-Hawthorn, J, Brough, S, Colless, M, Couch, WJ, Davies, RL, Drinkwater, MJ, Goodwin, M, Hopkins, AM, Konstantopoulos, IS, Foster, C, Lawrence, JS, Lorente, NPF, Medling, AM, Metcalfe, N, Richards, SN, van de Sande, J, Scott, N, Shanks, T, Sharp, R, Thomas, AD, Tonini, C

“…We have conducted a redshift survey of these clusters using the AAOmega multi-object spectrograph on the 3.9-m Anglo-Australian Telescope. The redshift survey is used to determine cluster membership and to characterize the dynamical properties of the clusters. …”