Now showing items 1-5 of 5

    • Mialon, M.; Pérez, E.; Corvalán, C.; Monteiro, C.; Jaime, P.; Baeza Scagliusi, F. (Oxford, 2020)
    • Galbany, Lluis; Stanishev, Vallery; Mourão, A. M.; Rodrigues, M.; Flores, H.; Walcher, C. J.; Sánchez, S. F.; García Benito, R.; Mast, D.; Badenes, Carles; González Delgado, R. M.; Kehrig, C.; Lyubenova, Mariyana; Marino, R. A.; Mollá, M.; Meidt, Sharon; Pérez, E.; van de Ven, G.; Vílchez, J. M. (EDP Sciences, 2016)
      The metallicity of a supernova progenitor, together with its mass, is one of the main parameters that can rule the progenitor's fate. We present the second study of nearby supernova (SN) host galaxies (0.005 < z < 0.03) ...
    • Sánchez, S. F.; Pérez, E.; Sánchez Blázquez, P.; García Benito, R.; Ibarra-Mede, H. J.; González, J.J.; Rosales Ortega, F.; Sánchez Menguiano, L.; Ascasibar, Y.; Bitsakis, T.; Law, D.; Cano-Díaz, M.; López-Cobá, C.; Marino, R.A.; Gil de Paz, A.; López Sánchez, Ángel R.; Barrera Ballesteros, J. K.; Galbany, Lluis; Mast, D.; Abril-Melgarejo, V.; Roman-Lopes, A. (Universidad Nacional Autónoma de México, 2016-04)
      We present PIPE3D, an analysis pipeline based on the FIT3D fitting tool, developed to explore the properties of the stellar populations and ionized gas of integral field spectroscopy (IFS) data. PIPE3D was created to provide ...
    • Sánchez Menguiano, L.; Sánchez, S. F.; Pérez, I.; García Benito, R.; Husemann, B.; Mast, D.; Mendoza, A.; Ruiz Lara, T.; Ascasibar, Y.; Bland-Hawthorn, J.; Cavichia, O.; Díaz, A. I.; Florido, E.; Galbany, Lluis; Gónzalez Delgado, R. M.; Kehrig, C.; Marino, R. A.; Márquez, I.; Masegosa, J.; Méndez Abreu, J.; Mollá, M.; Olmo, A. del; Pérez, E.; Sánchez-Blázquez, P.; Stanishev, V.; Walcher, C. J.; López Sánchez, Ángel R. (ESO, 2016-03)
      We measured the gas abundance profiles in a sample of 122 face-on spiral galaxies observed by the CALIFA survey and included all spaxels whose line emission was consistent with star formation. This type of analysis allowed ...
    • González Delgado, R. M.; Cid Fernandes, R.; Pérez, E.; García Benito, R.; López Fernández, R.; Lacerda, E. A. D.; Cortijo Ferrero, C.; de Amorim, A. L.; Vale Asari, N.; Sánchez, S. F.; Walcher, C. J.; Wisotzki, Lutz; Mast, D.; Alves, J.; Ascasibar, Y.; Bland Hawthorn, J.; Galbany, Lluis; Kennicutt, R. C.; Márquez, I.; Masegosa Ataz, Jose; Mollá, M.; Sánchez Blázquez, P.; Vílchez, J. M. (EDP Sciences, 2016)
      The spatially resolved stellar population content of today's galaxies holds important information for understanding the different processes that contribute to the star formation and mass assembly histories of galaxies. The ...