Browsing by Author "Kneissl, R."
Now showing 1 - 4 of 4
Results Per Page
Sort Options
- ItemThe ALMA Frontier Fields Survey III. 1.1mm emission line identifications in Abell 2744, MACSJ 0416.1-2403, MACSJ 1149.5+2223, Abell 370, and Abell S1063.(2017) González López, Jorge; Bauer, Franz Erik; Aravena, M.; Laporte, Nicolás; Bradley, L.; Carrasco, M.; Carvajal, R.; Demarco, R.; Infante Lira, Leopoldo; Kneissl, R.; Koekemoer, A. M.; Muñoz Arancibia, S. M.; Troncoso, P.; Villard, E.; Zitrin, A.
- ItemThe ALMA Frontier Fields Survey V. ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223(2020) Carvajal, R.; Bauer, Franz Erik; Bouwens, R. J.; Oesch, P. A.; González López, Jorge; Anguita, T.; Aravena, M.; Demarco, R.; Guaita, Lucía; Infante Lira, Leopoldo; Kim, S.; Kneissl, R.; Koekemoer, A. M.; Messias, H.; Treister, Ezequiel; Villard, E.; Zitrin, A.; Troncoso, P.
- ItemThe ALMA Frontier Fields Survey VI. Lensing-corrected 1.1 mm number counts in Abell 2744, MACSJ0416.1-2403, MACSJ1149.5+2223, Abell 370, and Abell S1063(2023) Arancibia, A. M. Munoz; Gonzalez-Lopez, J.; Ibar, E.; Bauer, F. E.; Anguita, T.; Aravena, M.; Demarco, R.; Kneissl, R.; Koekemoer, A. M.; Troncoso-Iribarren, P.; Zitrin, A.Context. Probing the faint end of the number counts at millimeter wavelengths is important in order to identify the origin of the extragalactic background light in this regime. Aided by strong gravitational lensing, ALMA observations toward massive galaxy clusters have opened a window to probe this origin, allowing us to resolve sub-milliJansky dusty star-forming galaxies.
- ItemThe ALMA Frontier Fields Survey. IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACS J0416.1-2403, and MACS J1149.5+2223 (Corrigendum)(2019) Muñoz Arancibia, A. M.; González-López, J.; Ibar, E.; Bauer, F. E.; Carrasco, M.; Laporte, N.; Anguita, T.; Aravena, M.; Barrientos, F.; Bouwens, R. J.; Demarco, R.; Infante, L.; Kneissl, R.; Nagar, N.; Padilla, N.; Romero-Cañizales, C.; Troncoso, P.; Zitrin, A.