Images of asteroid (596) Scheila have been acquired at various dates after the discovery of the 2010 outburst. Assuming a short-duration event scenario, as...
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Publication(596) Scheila in Outburst: A Probable Collision Event in the Main Asteroid Belt
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Publication(65) Cybele: detection of small silicate grains, water-ice, and organics
Context. (65) Cybele is the most representative member of a population of primitive asteroids in the outer edge of the main belt, the Cybele asteroids. Recent...
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Publication37 new validated planets in overlapping K2 campaigns
We analysed 68 candidate planetary systems first identified during Campaigns 5 and 6 (C5 and C6) of the NASA K2 mission. We set out to validate these systems by...
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Publication3C A Multi-Wavelength database for the future GTC cosmological surveys
The 3C Database aims to provide complete multi-wavelength information over different cosmological fields, such as GOODS, Groth or Sa68 allowing detailed studies...
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Publication3D simulations identifying the effects of varying the twist and field strength of an emerging flux tube
Aims.We investigate the effects of varying the magnetic field strength and the twist of a flux tube as it rises through the solar interior and emerges into the...
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Publication5-14 μm Spitzer spectra of Themis family asteroids
Context. The Themis collisional family is one of the largest and best established families in the main belt. Composed of primitive asteroids, there is evidence...
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Publication55 Cancri e's occultation captured with CHEOPS
Past occultation and phase-curve observations of the ultra-short period super-Earth 55 Cnc e obtained at visible and infrared wavelengths have been challenging...
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PublicationA 33-GHz interferometer for cosmic microwave background observations on Tenerife
We describe a new high-sensitivity experiment for observing cosmic microwave background (CMB) anisotropies. The instrument is a two-element interferometer...
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PublicationA binary merger origin for inflated hot Jupiter planets
We hypothesize that hot Jupiters with inflated sizes represent a separate planet formation channel, the merging of two low-mass stars. We show that the...