Información del autor
Documentos disponibles escritos por este autor (4)
Añadir el resultado a su cesta Hacer una sugerencia Refinar búsqueda
texto impreso
Arrabal Haro, P. ; Rodríguez Espinosa, J.M. ; Muñoz Tuñón, C. ; Sobral, D. ; Lumbreras Calle, A. ; Boquien, M. ; Hernán Caballero, A. ; Rodríguez Muñoz, L. ; Alcalde Pampliega, Belén | Oxford University Press. | 2020-06Lyman alpha emitters (LAEs) and Lyman break galaxies (LBGs) represent the most common groups of star-forming galaxies at high z, and the differences between their inherent stellar populations (SPs) are a key factor in understanding early galaxy [...]texto impreso
Girard, M. ; Dessauges-Zavadsky, M. ; Schaerer, D. ; Cirasuolo, M. ; Turner, O. J. ; Cava, A. ; Rodríguez Muñoz, L. ; Richard, J. ; Pérez González, Pablo Guillermo | EDP SCIENCES S A | 2018-06-04We present results from the KMOS LENsing Survey (KLENS), which is exploiting gravitational lensing to study the kinematics of 24 star -forming galaxies at 1.4texto impreso
Rodríguez Muñoz, L. ; Rodighiero, G. ; Mancini, C. ; Pérez González, Pablo Guillermo ; Rawle, T.D. ; Egami, E. ; Mercurio, A. ; Rosati, P. ; Puglisi, A. ; Franceschini, A. ; Balestra, I. ; Baronchelli, I. ; Biviano, A. ; Ebeling, H. ; Edge, A,C ; Enia, A.F.M. ; Grillo, C. ; Haines, C.P. ; Iani, E. ; Jones, T. ; Nonino, M. ; Valtchanov, I. ; Vulcani, B. ; Zemcov, M. | Oxford University Press. | 2019-05We quantify the star formation (SF) in the inner cores (R/R_(200) ?0.3) of 24 massive galaxy clusters at 0.2texto impreso
Lumbreras Calle, A. ; Muñoz Tuñón, C. ; Méndez Abreu, J. ; Mas Hesse, J.M. ; Pérez González, Pablo Guillermo ; Alcalde Pampliega, B. ; Arrabal Haro, P. ; Cava, A. ; Domínguez Sánchez, H. ; Eliche Moral, María del Carmen ; Alonso Herrera, A. ; Borlaff, A. ; Gallego Maestro, Jesús ; Hernán Caballero, Antonio ; Koekemoer, A.M. ; Rodríguez Muñoz, L. | EDP SCIENCES S A | 2019-01-08Context. The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift (0 ? z[...]
