Publicación
Galaxy Counts at 24 μm in the SWIRE Fields
This paper presents galaxy source counts at 24 μm in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts...
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PublicaciónGalaxy disc heating as a result of minor mergersWe perform a sample of N-body simulations of a minor merger between a Milky Way type galaxy and a satellite, which is density scaled version of the primary...
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PublicaciónGalaxy Disk Heating as a Result of Minor MergersWe perform N-body simulations of a minor merger between a Milky Way like galaxy and a disk-like satellite. In this set of collisionless runs we vary critical...
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PublicaciónGalaxy evolution studies observing Emission Line Galaxies with the GTCEmission line galaxies are the most easily detected and studied objects in the high redshift Universe. They are being used to trace the evolution of the...
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PublicaciónGalaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR SpectroscopyIR spectroscopy in the range 12-230 μm with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes governing the...
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PublicaciónGalaxy interactions are the dominant trigger for local type 2 quasarsThe triggering mechanism for the most luminous, quasar-like active galactic nuclei (AGN) remains a source of debate, with some studies favouring triggering via...
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PublicaciónGalaxy Light Concentration. I. Index Stability and the Connection with Galaxy Structure, Dynamics, and Supermassive Black HolesWe explore the stability of different galaxy light concentration indices as a function of the outermost observed galaxy radius. With a series of analytical...
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PublicaciónGalaxy mass-size segregation in the cosmic web from the CAVITY parent sampleContext. The mass-size relation is a fundamental galaxy scaling relation that is intrinsically linked to galaxy formation and evolution. The physical processes...
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PublicaciónGalaxy merger challenge: A comparison study between machine learning-based detection methodsAims: Various galaxy merger detection methods have been applied to diverse datasets. However, it is difficult to understand how they compare. Our aim is to...