Browsing by Author "Haussler, B."

Now showing items 1-4 of 4

    • 3D-HST+CANDELS : the evolution of the galaxy size-mass distribution since z=3 

      van der Wel, A.; Franx, M.; van Dokkum, P.G.; Skelton, R.E.; Momcheva, I.G.; Whitaker, K.E.; Brammer, G.B.; Bell, Eric F.; Rix, H-W.; Wuyts, Stijn; Ferguson, H. C.; Holden, B.P.; Barro, G.; Koekemoer, A. M.; Chang, Yu-Yen; McGrath, E.J.; Haussler, B.; Dekel, A.; Behroozi, P.; Fumagalli, M.; Leja, J.; Lundgren, B.F.; Maseda, M.V.; Nelson, E.J.; Wake, D.A.; Patel, S.G.; Labbe, I.; Faber, Sandra M.; Grogin, N. A.; Kocevski, D.D. (2014-06-10)
      Spectroscopic+photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging to determine the galaxy size-mass distribution ...

    • Bar evolution over the last 8 billion years: A constant fraction of strong bars in th GEMS Survey 

      Jogee, S.; Barazza, F.D.; Rix, H-W.; Shlosman, I.; Barden, M.; Wolf, C.; Davies, J.; Heyer, I.; Beckwith, S.; Bell, E.F.; Caldwell, J.A.R.; Conselice, J.; Dahlen, T.; Haussler, B.; Heymans, C.; Jahnke, K.; Knapen, J.; Laine, S.; Lubell, G.M.; Mobasher, B.; McIntosh, D.; Meisenheimar, K.; Peng, C.Y.; Sanchez, S.F.; Somerville, R.S.; Wisotzki, L. (2004-11)
      One-third of present-day spirals host optically visible strong bars that drive their dynamical evolution. However, the fundamental question of how bars evolve over cosmological times has yet to be resolved, and even the ...

    • MegaMorph - multiwavelength measurement of galaxy structure: Physically meaningful bulge-disc decomposition of galaxies near and far 

      Vika, Marina; Bamford, Steven P.; Haussler, B.; Rojas, Alex L. (2014-11-11)

    • Radio-quiet quasars in the VIDEO survey : evidence for AGN-powered radio emission at S-1.4 GHz<1 mJy 

      White, S. V.; Jarvis, M.J.; Haussler, B.; Maddox, N. (2015-04-11)
      Understanding the interplay between black-hole accretion and star formation, and how to disentangle the two, is crucial to our understanding of galaxy formation and evolution. To investigate, we use a combination of optical ...