Clusters And LENsing of Distant Sources

Objectif

Some of the primary questions in extragalactic astronomy concern the formation and evolution of galaxies in the distant Universe. In particular, little is known about the less luminous (and therefore less massive) galaxy populations, which are currently missed from large observing surveys and could contribute significantly to the overall star formation happening at early times. One way to overcome the current observing limitations prior to the arrival of the future James Webb Space Telescope or the European Extremely Large Telescopes is to use the natural magnification of strong lensing clusters to look at distant sources with an improved sensitivity and resolution.

The aim of CALENDS is to build and study in great details a large sample of accurately-modelled, strongly lensed galaxies at high redshift (1We will look for scaling relations between the stellar, gas and dust parameters, and compare them with known relations for lower redshift and more massive galaxy samples. For the most extended sources, we will be able to spatially resolve their inner properties, and compare the results of individual regions with predictions from simulations. We will look into key physical processes: star formation, gas accretion, inflows and outflows, in these distant sources.

Champ scientifique

Régime de financement

ERC-SG - ERC Starting Grant

Institution d’accueil

UNIVERSITE LYON 1 CLAUDE BERNARD

Contribution de l’UE

€ 1 450 992,00

Adresse

BOULEVARD DU 11 NOVEMBRE 1918 NUM43
69622 Villeurbanne Cedex
France

Région

Auvergne-Rhône-Alpes Rhône-Alpes Rhône

Type d’activité

Higher or Secondary Education Establishments

Contact administratif

Javier Olaiz (Dr.)

Chercheur principal

Johan Pierre Richard (Dr.)

Liens

Contacter l’organisation Site web

Coût total

Aucune donnée

Bénéficiaires (1)