Publication
Zodiacal Light Photometry off the Ecliptic in Quadrature and in Opposition with the Sun
Abstract image available at: http://adsabs.harvard.edu/abs/1973A&A....22..321D
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PublicationZodiacal light photopolarimetry. I - Observations, reductions, disturbing phenomena, accuracy. II - Gradients along the ecliptic and the phase functions of interplanetary matterAbstract image available at: http://adsabs.harvard.edu/abs/1975A&A....38..397D
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PublicationZodiacal Light Photopolarimetry. II. Gradients along the Ecliptic and the Phase Functions of Interplanetary MatterAbstract image available at: http://adsabs.harvard.edu/abs/1975A&A....38..405D
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PublicationZodiacal light photopolarimetry. III - All-sky survey from Teide 1964-1975 with emphasis on off-ecliptic featuresPhotopolarimetric observations of the zodiacal light over a complete solar cycle are used to study the average distribution of brightness and degree of...
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Publication[Mg/Fe] and variable initial mass function: Revision of [α/Fe] for massive galaxiesObservations of nearby massive galaxies have revealed that they are older and richer in metals and magnesium than their low-mass counterparts. In particular...
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Publicationɛ Indi Ba, Bb: a detailed study of the nearest known brown dwarfsThe discovery of ɛ Indi Ba, Bb, a binary brown dwarf system very close to the Sun, makes possible a concerted campaign to characterise the physical parameters...
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Publicationɛ Indi Ba,Bb: The nearest binary brown dwarfWe have carried out high angular resolution near-infrared imaging and low-resolution (R˜1000) spectroscopy of the nearest known brown dwarf, varepsilon Indi B...
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Publicationζ2 Reticuli, its debris disk, and its lonely stellar companion ζ1 Ret. Different Tc trends for different spectraContext. Several studies have reported a correlation between the chemical abundances of stars and condensation temperature (known as Tc trend). Very recently, a...
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Publicationτ Boötis b: Hunting for reflected starlightAims: We attempt to detect starlight reflected from the hot Jupiter orbiting the main-sequence star τ Boo, in order to determine the albedo of the planetary...