C. and .. Photométrique,

, FIGURE 2.1-De gauche à droite : mosaïques, cartes de poids et cartes des mauvais pixels en bandes J (haut) et

. Ks, (bas) du champ G006. Le rectangle vert, basé sur la carte de poids, indique la région du ciel gardée. Le cercle noir indique la position du candidat principal du champ et fait 1 de rayon

, Les sources SPIRE-rouges ont dans ?75% des cas une couleur JKs compatible avec z > 1.5, et dans ?40% des cas avec z > 2

. Chiang, Les candidats sont spatialement étendus (plusieurs arcminutes), ce qui est attendu pour les progéniteurs des amas massifs actuels à z ? 2, 2013.

, 92%) candidats semblent présenter une séquence rouge (J ? Ks vs Ks), indiquant une structure mature

, ]) vs (J ? Ks) sont compatibles avec les 12 modèles principaux de Berta et al. (95% de leur échantillon), tous représentant des galaxies en phase de formation stellaire

, Les surdensités JKs orange (z 1.5) sont en coïncidence angulaire étroite avec les surdensités IRAC-rouges

, Les cartes de densité par tranche de couleur JKs révèlent aussi de nouveaux candidats, non nécessairement vus par IRAC

, Autres résultats individuels majeurs

, Le candidat G124 a une couleur JKs parfaitement compatible avec son redshift spectroscopique z spec = 2.16, ce qui indique la qualité du découpage en couleurs JKs

. Kneissl, Concernant le candidat G073, les observations ALMA semblent indiquer un alignement fortuit avec un avant-plan à z ? 1, 2018.

, Le candidat G180 se révèle être au coeur d'une plus grande structure d'environ 8 de diamètre qui peut être distinctement scindée en deux régions grâce aux couleurs JKs

, En parallèle de l'analyse en proche infrarouge, j'ai fait de l'observation, réduction et analyse de données spectroscopiques EMIR du 30m de l'IRAM). Les principaux résultats sont les suivants : 1. Le candidat G124 contient 2 sources SPIRE, dont l'une avait été observée à z = 2.15 ; j'ai confirmé l'autre au même redshift

, De même pour G176 dont une source SPIRE avait été observée à z = 2.75, j'ai confirmé la seconde au même redshift

T. and L. Ir, SFR) est assez voire très incertaine, mais semble indiquer des starbursts progéniteurs des amas locaux les plus massifs, La dérivation des paramètres physiques

. Enfin, mon travail sur la PSF de l'imageur VIS d'Euclid indique que celle-ci varie assez peu en fonction du type spectral de l'objet et de sa position sur le plan focal de l

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