no code implementations • 29 Jan 2021 • C. López-Sanjuan, H. Yuan, H. Vázquez Ramió, J. Varela, D. Cristóbal-Hornillos, P. -E. Tremblay, A. Marín-Franch, A. J. Cenarro, A. Ederoclite, E. J. Alfaro, A. Alvarez-Candal, S. Daflon, A. Hernán-Caballero, C. Hernández-Monteagudo, F. M. Jiménez-Esteban, V. M. Placco, E. Tempel, J. Alcaniz, R. E. Angulo, R. A. Dupke, M. Moles, L. Sodré Jr
We conclude that photometric calibration with the stellar locus technique is prone to significant systematic bias along the Milky Way location for passbands bluer than lambda = 4500 A.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
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