no code implementations • 11 Jan 2021 • G. Vilella-Rojo, R. Logroño-García, C. López-Sanjuan, K. Viironen, J. Varela, M. Moles, A. J. Cenarro, D. Cristóbal-Hornillos, A. Ederoclite, C. Hernández-Monteagudo, A. Marín-Franch, H. Vázquez Ramió, L. Galbany, R. M. González Delgado, A. Hernán-Caballero, A. Lumbreras-Calle, P. Sánchez-Blázquez, D. Sobral, J. M. Vílchez, J. Alcaniz, R. E. Angulo, R. A. Dupke, L. Sodré Jr
The derived star formation rate density at d < 75 Mpc is log rho_SFR = -2. 10 +- 0. 11, with red galaxies accounting for 15% of the SFRD.
Astrophysics of Galaxies
2 code implementations • 15 Jul 2020 • P. O. Baqui, V. Marra, L. Casarini, R. Angulo, L. A. Díaz-García, C. Hernández-Monteagudo, P. A. A. Lopes, C. López-Sanjuan, D. Muniesa, V. M. Placco, M. Quartin, C. Queiroz, D. Sobral, E. Solano, E. Tempel, J. Varela, J. M. Vílchez, R. Abramo, J. Alcaniz, N. Benitez, S. Bonoli, S. Carneiro, A. J. Cenarro, D. Cristóbal-Hornillos, A. L. de Amorim, C. M. de Oliveira, R. Dupke, A. Ederoclite, R. M. González Delgado, A. Marín-Franch, M. Moles, H. Vázquez Ramió, L. Sodré, K. Taylor
As input for the ML algorithms we use the magnitudes from the 60 filters together with their errors, with and without the morphological parameters.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
1 code implementation • 19 Sep 2017 • J. Matthee, D. Sobral, F. Boone, H. Röttgering, D. Schaerer, M. Girard, A. Pallottini, L. Vallini, A. Ferrara, B. Darvish, B. Mobasher
The two most luminous components in [CII] coincide with the brightest UV components (A and B), blue-shifted by $\approx 150$ km s$^{-1}$ with respect to the peak of Ly$\alpha$ emission.
Astrophysics of Galaxies