"Using high resolution spectroscopic data obtained with Magellan Inamori Kyocera Echelle (MIKE) at the Magellan telescope at Las Campanas Observatory it was...
Resolved stellar populations in dSphs. What can they tell us about galaxy evolution?
We present a comprehensive photometric study of the Fornax and the Andromeda II dwarf spheroidal (dSph) galaxies. It is based on the up-to-date deepest...
Resolving molecular gas to ~500 pc in a unique star forming disk galaxy at z~2
We have resolved molecular gas in a 'typical' star forming disk galaxy at z>2 down to the scale of ~500 pc. Previous observations of CO and [CI] lines on larger...
Despite the great developments that have been achieved in the last decade in disentangling most relevant stellar population parameters, in particular with the...
Resolving the Cosmic Infrared Background with ISOCAM
The discovery in the COBE all-sky maps of a bright isotropic background in the far-IR/sub-mm, of likely extragalactic origin (CIRB), with a proeminent hump at a...
Resolving the Host Galaxies of Quasars at z = 2.5 with VLT + NACO.
Based on the most widely accepted model for structure formation in the Universe, the massive galaxies we see today are the result of the merging of smaller...