We analyse a high-resolution, fully cosmological, hydrodynamical disc galaxy simulation, to study the source of the double-exponential light profiles seen in...
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PublicationThe origin of the light distribution in spiral galaxies
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PublicationThe origin of the mid-infrared nuclear polarization of active galactic nuclei
We combine new (NGC 1275, NGC 4151, and NGC 5506) and previously published (Cygnus A, Mrk 231, and NGC 1068) sub-arcsecond resolution mid-infrared (MIR; 8-13 μm...
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PublicationThe Osiris Tunable Imager and Spectrograph: a 2004 Status Report
OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day one instrument for the GTC and the only Spanish Day One...
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PublicationThe OTELO Project
The OTELO Project is an extragalactic survey under way using the tunable filters of the instrument OSIRIS at the GTC. OTELO is already providing the deepest...
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PublicationThe PAU Survey and Euclid: Improving broadband photometric redshifts with multi-task learning
Current and future imaging surveys require photometric redshifts (photo-zs) to be estimated for millions of galaxies. Improving the photo-z quality is a major...
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PublicationThe Photo-Astrometric vertical tracer density of the Milky Way - I. The method
We introduce a method to infer the vertical distribution of stars in the Milky Way using a Poisson likelihood function, with a view to applying our method to...
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PublicationThe photo-astrometric vertical tracer density of the Milky Way - II. Results from Gaia
We use Gaia photometry and astrometry to estimate the vertical spatial structure of the Milky Way at the Solar radius, formally accounting for sample...
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PublicationThe Physics of Twisted Magnetic Tubes Rising in a Stratified Medium: Two-dimensional Results
The physics of a twisted magnetic flux tube rising in a stratified medium is studied using a numerical MHD code. The problem considered is fully compressible...
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PublicationThe PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey
Map-making is an important step for the data analysis of cosmic microwave background (CMB) experiments. It consists of converting the data, which are typically...