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Browsing General science, engineering & technology by Subject "Galaxies"

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  • Raccanelli, A; Zhao, G-B; Bacon, DJ; Jarvis, MJ; Percival, WJ; Norris, RP; Rottgering, H; Abdalla, FB; Cress, CM; Kubwimana, J-C; Lindsay, S; Nichol, RC; Santos, MG; Schwarz, DJ (Royal Astronomical Society, 2012-08)
    We present forecasts for constraints on cosmological models that can be obtained using the forthcoming radio continuum surveys: the wide surveys with the Low Frequency Array (LOFAR) for radio astronomy, theAustralian ...
  • Raccanelli, A; Zhao, G-B; Bacon, DJ; Jarvis, MJ; Percival, WJ; Norris, RP; Rottgering, H; Abdalla, FB; Cress, CM; Kubwimana, J-C; Lindsay, S; Nichol, RC; Santos, MG; Schwarz, DJ (Oxford University Press, 2012-08)
    We present forecasts for constraints on cosmological models that can be obtained using the forthcoming radio continuum surveys: the wide surveys with the Low Frequency Array (LOFAR) for radio astronomy, theAustralian ...
  • Cunnama, D; Andrianomena, S; Cress, CM; Faltenbacher, A; Gibson, BK; Theuns, T (Oxford University Press (OUP), 2014-01)
    We use the Galaxies-Intergalactic Medium Interaction Calculation (GIMIC) cosmological hydrodynamic simulation at z = 0 to study the distribution and environmental dependence of neutral hydrogen (Hi) gas in the outskirts ...
  • Randriamampandry, SM; Crawford, SM; Cress, CM; Hess, KM; Vaccari, M; Wilcots, EM; Bershady, MA; Wirth, GD (Oxford University Press, 2014-12)
    We present a multi-wavelength analysis of star-forming galaxies in the massive cluster MS0451.6-0305 at z ~ 0.54 to shed new light on the evolution of the far-infrared-radio relationship in distant rich clusters. We have ...
  • Sembolini, F; Yepes, CG; Pearce, FR; Knebe, A; Kay, ST; Power, C; Cui, W; Beck, AM; Borgani, S; Vecchia, CD; Dave, R; Elahi, PJ; February, S; Huang, S; Hobbs, A; Katz, N; Lau, E; McCarthy, IG; Murante, G; Nagai, D; Nelson, K; Newton, RDA; Puchwein, E; Read, JI; Saro, A; Schaye, J; Thacker, RJ (Oxford University Press, 2016-02)
    We have simulated the formation of a galaxy cluster in a cold dark matter universe using 13 different codes modelling only gravity and non-radiative hydrodynamics (RAMSES, ART, AREPO, HYDRA and nine incarnations of ...
  • Mguda, Z; Faltenbacher, A; Van der Heyden, K; Gottlöber, S; Cress, C; Vaisanen, P; Yepes, G (Oxford University Press, 2015-01)
    In this paper we use the MareNostrum Universe Simulation, a large scale, hydrodynamic, non-radiative simulation in combination with a simple abundance matching approach to determine the ram pressure statistics for bent ...

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