Browsing by Author "e07199ba-ad17-45fd-9593-79789957b439"

Now showing items 1-5 of 5

    • Pipe3D, a pipeline to analyse integral field spectroscopy data: II. Analysis sequence and califa dataproducts 
      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 ...
    • Shape of the oxygen abundance profiles in CALIFA face-on spiral galaxies 
      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 ...
    • Spatially resolved star formation main sequence of galaxies in the califa survey 
      Cano-Díaz, M.; Sánchez, S. F.; Zibetti, S.; Ascasibar, Y.; Bland-Hawthorn, J.; Ziegler, B.; González Delgado, R. M.; Walcher, C. J.; García Benito, R.; Mast, D.; Mendoza-Pérez, M. A.; Falcón Barroso, J.; Galbany, Lluis; Husemann, B.; Kehrig, C.; Marino, R. A.; Sánchez-Blázquez, P.; López-Cobá, C.; López Sánchez, Ángel R.; Vilchez, J. M. (The American Astronomical Society, 2016-04)
      The "main sequence of galaxies"-defined in terms of the total star formation rate psi versus the total stellar mass M-*-is a well-studied tight relation that has been observed at several wavelengths and at different ...
    • Star formation along the Hubble sequence Radial structure of the star formation of CALIFA galaxies 
      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 ...
    • The dependence of oxygen and nitrogen abundances on stellar mass from the CALIFA survey 
      Pérez Montero, E.; García Benito, R.; Vilchez, J. M.; Sánchez, S. F.; Kehrig, C.; Husemann, B; Duarte Puertas, S.; Iglesias Paramo, J.; Galbany, Lluis; Molla, M.; Walcher, C. J.; Ascasibar, Y.; González Delgado, R. M.; Marino, R. A.; Masegosa, J.; Peréz, E.; Rosales Ortega, F.; Sánchez Blázquez, P.; Bland Hawthorn, J.; Bomans, D.; López Sánchez, R.; Ziegler, B (EDP Sciences, 2016)
      Context. The study of the integrated properties of star-forming galaxies is central to understand their formation and evolution. Some of these properties are extensive and therefore their analysis require totally covering ...