,
, FIGURE 2.1-De gauche à droite : mosaïques, cartes de poids et cartes des mauvais pixels en bandes J (haut) et
, (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
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
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
SFR) est assez voire très incertaine, mais semble indiquer des starbursts progéniteurs des amas locaux les plus massifs, La dérivation des paramètres physiques ,
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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