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Klever

Klever

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Overview

KLEVER (Kmos LEnsed Velocity and Emission line Review) is an ESO Large Programme exploiting the multi-IFU near-IR spectrograph KMOS at the Very Large Telescope. The goal is to obtain 3D spectra (i.e. spatially resolved spectroscopy) of a sample of about 200 galaxies, in the redshift range z~1-2.5, in all three primary near-IR bands (J, H, K) so to map all of the primary optical nebular lines redshifted into the near-IR bands ([OII], [NeIII], He II, Hβ, [OIII], Hα, [NII], [SII], [SIII]). The combination of these multiple lines will enable us to investigate in detail the physical properties of the ISM in galaxies (excitation mechanism, chemical enrichment, ionization parameter, density, etc...) with an accuracy that has not been possible in previous large surveys (due to the lack of appropriate diagnostics), spatially resolved and with a statistically sound sample.

Sample

The sample consists of spectroscopically confirmed galaxies at z~1-2.5, specifically selected to have the primary nebular lines redshifted into the main near-IR bands. Half of the sample consists of galaxies in GOODS-South and in COSMOS, while half of the sample consists of gravitationally lensed galaxies in six lensing clusters from the CLASH survey (these will enable to achieve a higher projected spatial resolution and to access fainter, low-mass galaxies).

Team

Co-PIs: Michele Cirasuolo and Roberto Maiolino

Co-Is: Mirko Curti, Matt Bothwell, Giovanni Cresci, Max Pettini, Filippo Mannucci, Alessandro Marconi, Massimo Meneghetti, Tohru Nagao, Paulina Troncoso, Yingjie Peng, James Dunlop, Ross McLure, Italo Balestra, Simon Lilly, Claudia Cicone, Piero Rosati, Rob Ivison, Michele Cappellari, Mark Swinbank, Fergus Cullen, Owen Turner, Kazuaki Ota

Data release

Data products will be released on this site and on an ESO mirror site.

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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