Publicación
Chapter 4 : The Evolution of Oxygen in Galaxies
Not Available
-
-
PublicaciónChapuzón cósmico: astronomical workshops for childrenWe present a set of six Astronomy outreach workshops for children called ''Chapuzón cósmico''. These workshops took place at the Museo de la Ciencia y el Cosmos...
-
PublicaciónCharacterisation of the upper atmosphere of HD 209458 b by means of helium triplet absorption spectra.The upper atmosphere of HD 209458 b undergoes hydrodynamic escape that is the most atmospheric efficient mass-loss process. Previous works on its...
-
PublicaciónCharacterising the atmosphere of ultra hot Jupiters: MASCARA-2bUltra hot Jupiters orbit very close to their host star and consequently receive strong irradiation that makes their atmospheric chemistry different from the...
-
PublicaciónCharacterising the colour and vertical structure of Saturn's haze using observations from the VLT/MUSE instrumentSaturn's atmosphere is characterised by a thick yellow haze that envelopes its entire surface. What causes this haze to be yellow, however, remains unknown. We...
-
PublicaciónCharacteristics and Performance of the GAW Experiment for a Large Field of View Cerenkov Gamma-ray TelescopeOne of the intents of the ground-based gamma-ray astronomy is to obtain a sky survey in the TeV energy region, and nowadays this target can be reached with...
-
PublicaciónCharacteristics and performance of the GAW experiment for a large field of view Cerenkov γ rays telescopeThe GAW project aims to test the feasibility of a new generation of Imaging Atmospheric Cherenkov Telescopes that join high flux sensitivity with Large Field of...
-
PublicaciónCharacterization of a Large Sample of Be-type Emission-line Stars with SDSS-III/APOGEEIn just one year of operation, the SDSS-III/APOGEE survey has amassed the largest collection ever of high-resolution, H-band spectra for Be-type emission-line...
-
PublicaciónCharacterization of AGN and their hosts in the Extended Groth StripWe have employed a reliable technique of classification of AGN based on the fit of their spectral energy distributions with a complete set of AGN types and...