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Clustering of Extremely Red Objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS1 and Subaru
Jae-Woo Kim, Alastair C. Edge, David A. Wake +11
We measure the angular clustering of 33 415 extremely red objects (EROs) in the Elais-N1 field covering 5.33 deg, which cover the redshift range to . This sample w…
The WIRCam Deep Survey II: Mass Selected Clustering
R. M. Bielby, V. Gonzalez-Perez, H. J. McCracken +7
We present an analysis of the clustering of galaxies from z ~ 2 to the present day using the WIRCam Deep Survey (WIRDS). WIRDS combines deep near-infrared data with the deep optica…
Which galaxies dominate the neutral gas content of the Universe?
Claudia del P. Lagos, C. M. Baugh, M. A. Zwaan +5
We study the contribution of galaxies with different properties to the global densities of star formation rate (SFR), atomic (HI) and molecular hydrogen (H2) as a function of redsh…
Modelling the relative velocities of isolated pairs of galaxies
V. Gonzalez-Perez, E. Jennings, M. -C. Cousinou +3
We study the comoving relative velocities, v12, of model isolated galaxy pairs at z=0.5. For this purpose, we use the predictions from the GALFORM semi-analytical model of galaxy f…
A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
V. Gonzalez-Perez, C. G. Lacey, C. M. Baugh +4
We present a new release of the GALFORM semi-analytical model of galaxy formation and evolution, which exploits a Millennium Simulation-class N-body run performed with the WMAP7 co…
Single Colour Diagnostics of the Mass-to-light Ratio: Predictions from Galaxy Formation Models
Stephen M. Wilkins, Violeta Gonzalez-Perez, Carlton M. Baugh +2
Accurate galaxy stellar masses are crucial to better understand the physical mechanisms driving the galaxy formation process. We use synthetic star formation and metal enrichment h…