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Large Scale Structure and Precision Cosmology


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.

Current KICC researchers involved in this theme are:

Researchers previously based in this Kavli group:

KICC Annual Report 2019

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Galaxies in the Infant Universe Were Surprisingly Mature

Oct 27, 2020

Massive galaxies were already much more mature in the early universe than previously expected. This was shown by an international team of astronomers—including researchers from the Kavli Institute for Cosmology (KICC) and the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) — who studied 118 distant galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA).

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