Now showing items 1-1 of 1

    • GLACE survey: OSIRIS/GTC tuneable filter H$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue 

      Sánchez-Portal, M.; Pintos-Castro, I.; Pérez-Martínez, R.; Cepa, J.; Pérez García, A.~M.; Domínguez-Sánchez, H.; Bongiovanni, A.; Serra, A.~L.; Alfaro, E.; Altieri, B.; Aragón-Salamanca, A.; Balkowski, C.; Biviano, A.; Bremer, M.; Castander, F.; Castañeda, H.; Castro-Rodríguez, N.; Chies-Santos, A.~L.; Coia, D.; Diaferio, A.; Duc, P.~A.; Ederoclite, A.; Geach, J.; González-Serrano, I.; Haines, C.~P.; McBreen, B.; Metcalfe, L.; Oteo, I.; Pérez-Fournón, I.; Poggianti, B.; Polednikova, J.; Ramón-Pérez, M.; Rodríguez-Espinosa, J.~M.; Santos, J.~S.; Smail, I.; Smith, G.~P.; Temporin, S.; Valtchanov, I. (2015-06-01)
      The cores of clusters at 0 ≲ z ≲ 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type galaxies. Clusters grow through the accretion of galaxies and groups from the ...