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Large Scale Structure and Precision Cosmology

LSS

Research interests in Large Scale Structure and Precision Cosmology at KICC cover a wide array of physical phenomena, spanning a large range of astrophysical scales and epochs - from the present day properties of the Universe going back in time to the surface of  last scattering and the Planck scale era.

Both theoretical modelling and exploitation of data from large scale surveys are being exploited. Within this context KICC scientist are involved in several projects such as DES, DESI, LSST and Euclid.

KICC people involved in this theme are:

KICC Annual Report 2018

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Metallicity gradients in high redshift galaxies via multi-band, near-infrared integral field spectroscopy

Jan 10, 2020

Galaxies at the ‘cosmic noon’ are often characterised by the absence of strong radial gradients in the spatial distribution of metals, consistent with strong feedback mechanisms in place, but is this always reflecting a real spatial homogeneity ? New insights from the KLEVER Survey.

The Detection of a Molecular Outflow in a Primeval Starburst Galaxy

Dec 13, 2019

The Detection of a Molecular Outflow in a Primeval Starburst Galaxy

Roberto Maiolino appointed Honorary Professor of University College London

Dec 02, 2019

Roberto Maiolino, Director of the Kavli Institute, has been appointed Honorary Professor of University College London in the Department of Physics and Astronomy.

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