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KiDS-450: testing extensions to the standard cosmological model

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471:2 (2017) 1259-1279

Authors:

S Joudaki, A Mead, C Blake, A Choi, J de Jong, T Erben, IF Conti, R Herbonnet, C Heymans, H Hildebrandt, H Hoekstra, B Joachimi, D Klaes, F Kohlinger, K Kuijken, J McFarland, L Miller, P Schneider, M Viola
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KiDS-450: tomographic cross-correlation of galaxy shear with Planck lensing

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471:2 (2017) 1619-1633

Authors:

J Harnois-Deraps, T Troster, NE Chisari, C Heymans, L van Waerbeke, M Asgari, M Bilicki, A Choi, T Erben, H Hildebrandt, H Hoekstra, S Joudaki, K Kuijken, J Merten, L Miller, N Robertson, P Schneider, M Viola
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The prevalence of core emission in faint radio galaxies in the SKA Simulated Skies

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471:1 (2017) 908-913

Authors:

IH Whittam, MJ Jarvis, DA Green, I Heywood, JM Riley
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HI properties and star formation history of a fly-by pair of blue compact dwarf galaxies⋆

Astronomy & Astrophysics EDP Sciences 605 (2017) a54

Authors:

Jinhyub Kim, Aeree Chung, O Ivy Wong, Bumhyun Lee, Eon-Chang Sung, Lister Staveley-Smith
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Galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation

Monthly Notices of the Royal Astronomical Society (2017)

Authors:

NE Chisari, N Koukoufilippas, A Jindal, S Peirani, RS Beckmann, S Codis, J Devriendt, L Miller, Y Dubois, C Laigle, A Slyz, C Pichon

Abstract:

Intrinsic alignments of galaxies are a significant astrophysical systematic affecting cosmological constraints from weak gravitational lensing. Obtaining numerical predictions from hydrodynamical simulations of expected survey volumes is expensive, and a cheaper alternative relies on populating large dark matter-only simulations with accurate models of alignments calibrated on smaller hydrodynamical runs. This requires connecting the shapes and orientations of galaxies to those of dark matter haloes and to the large-scale structure. In this paper, we characterise galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation. We compare the shapes and orientations of galaxies in the redshift range $0
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