Team Organisation

The WALLABY Principle Investigators (PIs) are B. Koribalski and L. Staveley-Smith. Listed below are the revised technical and science working groups.

Technical Working Groups

TWG1 Numerical Simulations & Mock Surveys Abate, Baugh, Bekki, Blake, Colless, Crain, Duffy, Ford, Frenk, Glazebrook, Gupta, Hendry, Jones, Kilborn, H. Kim, Lagos, Oosterloo, Popping, Power, Staveley-Smith, Webster, Whiting, Zwaan
TWG2 Survey Strategy & Field Selection Catinella, Dénes, Koribalski, Lee-Waddell, Madrid, Staveley-Smith, Wang, Westmeier, Wong
TWG3 Data Processing, Imaging & Postage Stamps Bekiaris, Elagali, For, Heald, Kleiner, Koribalski, Lee-Waddell, Madrid, Meurer, Meyer, Ord, Popping, Reynolds, Rhee, Rozgonyi, Spekkens, Staveley-Smith, Westmeier, Whiting, Wong
TWG4 Source Finding & Cataloguing Giese, Józsa, Jurek, Koribalski, Meyer, Popping, Serra, Staveley-Smith, van der Hulst, Westmeier, Winkel
TWG5 Kinematics Pipeline Bekiaris, de Blok, Bryant, Elson, Giese, Józsa, Kamphuis, Koribalski, Oh, Serra, Staveley-Smith, Spekkens, van der Hulst, Verheijen, Wang
TWG6 Data Visualisation Bekiaris, For, Koribalski, Lee-Waddell, Popping, Serra, Staveley-Smith, Wong
TWG7 Postage Stamps Merged with TWG3
TWG8 Flagging, Data Validation & Quality Control Staveley-Smith
TWG9 ES Field Selection Merged with TWG2

 

Science Working Groups

SWG1 Local Group Bouchard, For, Jerjen, Koribalski, Meurer, Oosterloo, Putman, Ryan-Weber, Wakker, Wilcots, Zucker
SWG2 Local Universe de Blok, Bigiel, Bosma, Bouchard, da Cunha, Driver, Dunne, Emonts, English, For, Ford, Gereb, Hopkins, Jerjen, Jozsa, Karachentsev, Koribalski, Leeuw, Lopez-Sanchez, Masci, Meurer, Morganti, Nakanishi, Oh, Oosterloo, Putman, Rhee, Ryder, Saikia, Schawinski, Serra, Spekkens, Westmeier, Wilcots, Wong, Taylor
SWG3 Galaxy Environments Ben Bekhti, Bigiel, Blake, Bosma, Bouchard, Colless, Boselli, da Cunha, Denes, Gereb, English, For, Ford, Henning, Hess, Jerjen, Jozsa, Karachentsev, Kilborn, Koribalski, Kraan-Korteweg, Lagos, Lee-Waddell, Lopez-Sanchez, Meurer, Oosterloo, Popping, Radchaudhury, Rhee, Saikia, Schawinski, Spekkens, van der Hulst, Westmeier, Wilcots, Winkel, Wong, Taylor
SWG4 Intergalactic HI Ben Bekhti, Bekki, Gupta, Hess, Koribalski, Lagos, Lee-Waddell, Meurer, Oosterloo, Popping, Ryan-Weber, Saikia, Wakker, Wilman, Winkel, Zwaan
SWG5 HI Mass Function Blake, Dunne, Glazebrook, Henning, Kilborn, H. Kim, Lagos, Meyer, Power, Spekkens, Staveley-Smith, Zwaan
SWG6 Large-scale structure Abate, Baugh, Blake, Bosma, S. Brown, Colless, Courtois, Davis, Duffy, Glazebrook, Jarrett, Jones, Karachentsev, H. Kim, Kraan-Korteweg, Lagos, Meyer, Mould, Power, Raychaudhury, Schmidt, Springob, Staveley-Smith, Webster, Wilman, Yun
SWG7 Galaxy clusters S. Brown, Edge, Kilborn, Boselli, Gereb, Hess, Putman, Serra, Verheijen, Wilcots
SWG8 Galactic HI & HVCs Ben Bekhti, Dickey, For, Ford, Kerp, Muller, Putman, Thompson, Wakker, Westmeier, Winkel, Yun
SWG9 ASKAP Survey Synergies Koribalski & Staveley-Smith (WALLABY), Norris & Hopkins (EMU), Sadler (FLASH), Meyer (DINGO), Dickey (GASKAP), Murphy (VAST), Hess, Oosterloo (Apertif HI surveys), de Blok, Serra, Heywood (MeerKat), etc
SWG10 Multi-frequency synergies Koribalski & Staveley-Smith (WALLABY), Schmidt, Wolf (SkyMapper), Meurer (PanStarrs), Colless, Jones & da Cunha, Pimbblet, Taylor, (TAIPAN, 6dF), Bryant (HECTOR), Jarrett & Masci (2MASS, WISE), Driver (VISTA VHS), Nakanishi, Yun (molecular), Dunne (Herschel ATLAS, FIR-submm), etc.