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5 papers · 2 filters
Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
Avery Meiksin, James S. Bolton, Eric R. Tittley
We perform cosmological simulations of the intergalactic medium (IGM) at redshift z ~ 3 using the numerical gravity-hydrodynamics codes GADGET-3 and Enzo for the purpose of modelli…
AzTEC/ASTE 1.1 mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimeter galaxies
H. Umehata, Y. Tamura, K. Kohno +22
We present the results from a 1.1 mm imaging survey of the SSA22 field, known for having an overdensity of z=3.1 Lyman-alpha emitting galaxies (LAEs), taken with the AzTEC camera o…
Constraining chameleon models with cosmology
Lucas Lombriser
Chameleon fields may modify gravity on cluster scales while recovering general relativity locally. This article reviews signatures of chameleon modifications in the nonlinear cosmo…
A new method for classifying galaxy SEDs from multi-wavelength photometry
Vivienne Wild, Omar Almaini, Michele Cirasuolo +7
We present a new method to classify the broad band optical-NIR spectral energy distributions (SEDs) of galaxies using three shape parameters (super-colours) based on a Principal Co…
Herschel-ATLAS/GAMA:How does the far-IR luminosity function depend on galaxy group properties?
Qi Guo, Cedric Lacey, Peder Norberg +14
We use the Herschel ATLAS (H-ATLAS) Phase I data to study the conditional luminosity function of far-IR (250 um) selected galaxies in optically-selected galaxy groups from the GAMA…