How well does galaxy clustering constrain cosmology?
On the LCDM cosmology, dark matter collapses into virialised objects called haloes. The abundance and distribution of these haloes are a direct consequence of...
Imfit: A fast, flexible new program for fitting galaxy images
I will discuss a new, open-source astronomical image-fitting program, specialized for galaxies, which is fast, flexible, and highly extensible. A key...
In this talk I will review the subject of cosmological inflation, a period of early accelerated expansion. I will discuss Friedmann-Robertson-Walker cosmology...
Is Dark Matter the most valid explanation for the mass which is apparently missing in the Universe?
Two main families of models explain that, at least in appearance, something like 90% of the mass of the Universe is still undetected. One (supported by an...
Large scale structures and galaxy evolution in the COSMOS Survey
The COSMOS survey is the largest high redshift galaxy evolution survey ever done -- imaging 2 square degrees with all major space-based and ground based...
Latest news on Cosmic Microwave Background research
1) Overview on Planck and QUIJOTE. R. Rebolo 15 min. 2) The Galaxy as seen by Planck. R. Génova-Santos 15 min. 3) Planck Cosmological Results. J. A. Rubiño...