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Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm (2012)
Journal Article
Driver, S., Robotham, A., Kelvin, L., Alpaslan, M., Baldry, I., Bamford, S., …Wilkins, S. (2012). Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm. Monthly Notices of the Royal Astronomical Society, 427(4), 3244-3264. https://doi.org/10.1111/j.1365-2966.2012.22036.x

We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugr... Read More about Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm.

Constraining extended gamma-ray emission from galaxy clusters (2012)
Journal Article
Han, J., Frenk, C., Eke, V., Gao, L., White, S., Boyarsky, A., …Ruchayskiy, O. (2012). Constraining extended gamma-ray emission from galaxy clusters. Monthly Notices of the Royal Astronomical Society, 427(2), 1651-1665. https://doi.org/10.1111/j.1365-2966.2012.22080.x

Cold dark matter models predict the existence of a large number of substructures within dark matter haloes. If the cold dark matter consists of weakly interacting massive particles, their annihilation within these substructures could lead to diffuse... Read More about Constraining extended gamma-ray emission from galaxy clusters.

Rotation rates, sizes and star formation efficiencies of a representative population of simulated disc galaxies (2012)
Journal Article
McCarthy, I., Schaye, J., Font, A., Theuns, T., Frenk, C., Crain, R., & Dalla Vecchia, C. (2012). Rotation rates, sizes and star formation efficiencies of a representative population of simulated disc galaxies. Monthly Notices of the Royal Astronomical Society, 427(1), 379-392. https://doi.org/10.1111/j.1365-2966.2012.21951.x

We examine the rotation rates, sizes and star formation (SF) efficiencies of a representative population of simulated disc galaxies extracted from the Galaxies–Intergalactic Medium Interaction Calculation (GIMIC) suite of cosmological hydrodynamic si... Read More about Rotation rates, sizes and star formation efficiencies of a representative population of simulated disc galaxies.

Satellite galaxy number density profiles in the Sloan Digital Sky Survey (2012)
Journal Article
Guo, Q., Cole, S., Eke, V., & Frenk, C. (2012). Satellite galaxy number density profiles in the Sloan Digital Sky Survey. Monthly Notices of the Royal Astronomical Society, 427(1), 428-441. https://doi.org/10.1111/j.1365-2966.2012.21882.x

We study the spatial distribution of satellite galaxies around isolated primaries using the Sloan Digital Sky Survey (SDSS) spectroscopic and photometric galaxy catalogues. We select isolated primaries from the spectroscopic sample and search for pot... Read More about Satellite galaxy number density profiles in the Sloan Digital Sky Survey.

Scaling relations for galaxy clusters in the Millennium-XXL simulation (2012)
Journal Article
Angulo, R., Springel, V., White, S., Jenkins, A., Baugh, C., & Frenk, C. (2012). Scaling relations for galaxy clusters in the Millennium-XXL simulation. Monthly Notices of the Royal Astronomical Society, 426(3), 2046-2062. https://doi.org/10.1111/j.1365-2966.2012.21830.x

We present a very large high-resolution cosmological N-body simulation, the Millennium-XXL or MXXL, which uses 303 billion particles to represent the formation of dark matter structures throughout a 4.1 Gpc box in a Λ cold dark matter cosmology. We c... Read More about Scaling relations for galaxy clusters in the Millennium-XXL simulation.

Space-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO) (2012)
Journal Article
Rhodes, J., Dobke, B., Booth, J., Massey, R., Liewer, K., Smith, R., Amara, A., Aldrich, J., Berge, J., Bezawada, N., Brugarolas, P., Clark, P., Dubbeldam, C., Ellis, R., Frenk, C., Gallie, A., Heavens, A., Henry, D., Jullo, E., Kitching, T., …Wu, J. (2012). Space-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO). Astroparticle Physics, 38, 31-40. https://doi.org/10.1016/j.astropartphys.2012.05.015

The contribution of star-forming galaxies to fluctuations in the cosmic background light (2012)
Journal Article
Kim, H., Lacey, C., Cole, S., Baugh, C., Frenk, C., & Efstathiou, G. (2012). The contribution of star-forming galaxies to fluctuations in the cosmic background light. Monthly Notices of the Royal Astronomical Society, 425(4), 2674-2687. https://doi.org/10.1111/j.1365-2966.2012.21641.x

Star-forming galaxies which are too faint to be detected individually produce intensity fluctuations in the cosmic background light. This contribution needs to be taken into account as a foreground when using the primordial signal to constrain cosmol... Read More about The contribution of star-forming galaxies to fluctuations in the cosmic background light.

The journey of QSO haloes from z ∼ 6 to the present (2012)
Journal Article
Angulo, R., Springel, V., White, S., Cole, S., Jenkins, A., Baugh, C., & Frenk, C. (2012). The journey of QSO haloes from z ∼ 6 to the present. Monthly Notices of the Royal Astronomical Society, 425(4), 2722-2730. https://doi.org/10.1111/j.1365-2966.2012.21783.x

We apply a recently developed scaling technique to the Millennium-XXL, one of the largest cosmological N-body simulations carried out to date (3 × 1011 particles within a cube of volume ∼70 Gpc3). This allows us to investigate the cosmological parame... Read More about The journey of QSO haloes from z ∼ 6 to the present.

Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts (2012)
Journal Article
Christodoulou, L., Eminian, C., Loveday, J., Norberg, P., Baldry, I., Hurley, P., …Wijesinghe, D. (2012). Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts. Monthly Notices of the Royal Astronomical Society, 425(2), 1527-1548. https://doi.org/10.1111/j.1365-2966.2012.21434.x

We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4 mag from the Sloan Digital Sky Survey (SDSS) as a function of photometric redshift, absolute magnitude and colour down to Mr − 5 log h = −14 mag. Pho... Read More about Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts.