The ability of any Machine Learning method to classify the spectra of galaxies depending on the properties of the stellar component rests on the information...
The Environment of Nearby Blue Compact Dwarf Galaxies
We are obtaining deep multiwavelength data of a sample of nearby blue compact dwarf galaxies (BCDGs) combining broad-band optical/NIR and Hα photometry, optical...
We are currently performing a new analysis of the close environment of star-forming dwarf galaxies and its effects on their star-forming activity. For a sample...
The Epeakrest E correlation in GRBs in the BATSE catalog
The energy emission involved in a Gamma-Ray Burst evidently can be estimated only provided that we know the distance to the source. The same is true for the...
The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey
The study of the Extremly Red Objects (EROs), is the importance for setting constraints on the first epoch of massive galaxy formation, for exploring the...
The ESO Diffuse Interstellar Band Large Exploration Survey (EDIBLES)
The ESO Diffuse Interstellar Band Large Exploration Survey (EDIBLES) is a Large Programme that is collecting high-signal-to-noise (S/N) spectra with UVES of a...