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Autor Papaderos, P. |
Documentos disponibles escritos por este autor (6)
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Iglesias Páramo, J. ; Vílchez, J. M. ; Galbany, L. ; Sánchez, S. F. ; Rosales Ortega, F. F. ; Mast, D. ; García Benito, R. ; Husemann, B. ; Aguerri, J. A. L. ; Alves, J. ; Bekeraite, S. ; Bland-Hawthorn, J. ; Catalán Torrecilla, Cristina ; Amorim, A. L. de ; Lorenzo Cáceres, A. de ; Ellis, S. ; Falcón Barroso, J. ; Flores, H. ; Florido, E. ; Gallazzi, A. ; Gomes, J. M. ; González Delgado, R. M. ; Haines, T. ; Hernández Fernández, J. D. ; Kehrig, C. ; López Sánchez, A. R. ; Lyubenova, M. ; Marino, Raffaella Anna ; Mollá, M. ; Monreal Ibero, A. ; Mour?o, A. ; Papaderos, P. ; Rodrigues, M. ; Sánchez Blázquez, P. ; Spekkens, K. ; Stanishev, V. ; van de Ven, G. ; Walcher, C. J. ; Wisotzki, L. ; Zibetti, S. ; Ziegler, B. | EDP Sciencies | 2013-05This work investigates the effect of the aperture size on derived galaxy properties for which we H alpha ve spatially-resolved optical spectra. We focus on some indicators of star formation activity and dust attenuation for spiral galaxies that [...]texto impreso
Gil de Paz, Armando ; Madore, B. F. ; Noeske, K. ; Cairós, L. M. ; Papaderos, P. ; Silich, S. A. | American Astronomical Society | 2003-10-20We report the discovery of a double ring of emission-line regions around the nucleus of the blue compact dwarf galaxy Mrk 409 as seen by deep, ground-based H? images. Echelle spectroscopy obtained at Magellan I with MIKE shows the presence of io[...]texto impreso
Sánchez, S. F. ; Pérez, E. ; Rosales Ortega, F. F. ; Miralles Caballero, D. ; López Sánchez, A. R. ; Iglesias Páramo, J. ; Marino, Raffaella Anna ; Sánchez Menguiano, L. ; García Benito, R. ; Mast, D. ; Mendoza, M. A. ; Papaderos, P. ; Ellis, S. ; Galbany, L. ; Kehrig, C. ; Monreal Ibero, A. ; González Delgado, R. ; Mollá, M. ; Ziegler, B. ; de Lorenzo Cáceres, A. ; Méndez Abreu, J. ; Bland-Hawthorn, J. ; Bekeraite, S. ; Roth, M. M. ; Pasquali, A. ; Diaz, A. ; Bomans, D. ; van de Ven, G. ; Wisotzki, L. | EDP Sciencies | 2015-02Context. H II regions in galaxies are the sites of star formation, so they are special places for understanding the build-up of stellar mass in the universe. The line ratios of this ionized gas are frequently used to characterize the ionization [...]texto impreso
Noeske, K. G. ; Koo, D. C. ; Phillips, A. C. ; Willmer, C. N. A. ; Melbourne, J. ; Gil de Paz, Armando ; Papaderos, P. | American Astronomical Society | 2006-04-01We analyze 26 luminous compact blue galaxies (LCBGs) in the Hubble Space Telescope ACS Ultra Deep Field (UDF) at z ~ 0.2-1.3, to determine whether these truly are small galaxies or, rather, bright central starbursts within existing or forming la[...]texto impreso
Galbany, L. ; Stanishev, V. ; Mourão, A. M. ; Rodrigues, M. ; Flores, H. ; García Benito, R. ; Mast, D. ; Mendoza, M. A. ; Sánchez, S. F. ; Badenes, C. ; Barrera Ballesteros, J. ; Bland-Hawthorn, J. ; Falcón Barroso, J. ; García Lorenzo, B. ; Gomes, J. M. ; González Delgado, R. M. ; Kehrig, C. ; Lyubenova, M. ; López Sánchez, A. R. ; Lorenzo Cáceres, A. de ; Marino, Raffaella Anna ; Meidt, S. ; Mollá, M. ; Papaderos, P. ; Pérez Torres, M. A. ; Rosales Ortega, F. F. ; van de Ven, G. | EDP Sciencies | 2014-12We use optical integral field spectroscopy (IFS) of nearby supernova (SN) host galaxies (0.005texto impreso
Sánchez Blázquez, P. ; Rosales Ortega, F. F. ; Méndez Abreu, J. ; Pérez, I. ; Sánchez, S. F. ; Zibetti, S. ; Aguerri, J. A. L. ; Bland-Hawthorn, J. ; Catalán Torrecilla, Cristina ; Cid Fernandes, R. ; de Amorim, A. ; de Lorenzo Cáceres, A. ; Falcón Barroso, J. ; Galazzi, A. ; García Benito, R. ; Gil de Paz, Armando ; González Delgado, R. ; Husemann, B. ; Iglesias Paramo, Jorge ; Jungwiert, B. ; Marino, Raffaella Anna ; Márquez, I. ; Mast, D. ; Mendoza, M. A. ; Mollá, M. ; Papaderos, P. ; Ruiz Lara, T. ; van de Ven, G. ; Walcher, C. J. ; Wisotzki, L. | EDP Sciencies | 2014-10While studies of gasphase metallicity gradients in disc galaxies are common, very little has been done towards the acquisition of stellar abundance gradients in the same regions. We present here a comparative study of the stellar metallicity and[...]