My research career began in 1999 at the Astrophysics Research Institute in the Liverpool John Moores University, studying the distribution of gas in clusters of nearby galaxies through X-ray observations (ROSAT, XMM-Newton and Chandra). The development of my doctoral thesis (2001-2005, Univ. Granada) also included the detailed study of the dynamics of central regions of star-forming galaxies as a useful tool for the study of gas flows (and therefore magnetic field) and stellar material to and from the intergalactic environment.
My postdoctoral research has focused on the study of populations of nearby star-forming galaxies using advanced 2D spectroscopy techniques in the visible: (1) understanding the interaction between galaxies and the intergalactic medium has been a topic to which I have dedicated part of my postdoctoral research, with the detection and analysis of galactic winds (INTEGRAL in WHT), (2) study of luminous, compact and blue galaxies: their kinematics, current rhythm of stellar formation, dust distribution and metallicity (PPAK in 3.5m@CAHA), to understand the mechanisms that give rise to intense star formation in this type of galaxies, (3) two-dimensional study of the rate of stellar formation based on the corrected H emission of extinction in the sample of CALIFA galaxies.