Publicación
Confidence levels of evolutionary synthesis models
The stochastic nature of the IMF in young stellar clusters implies that clusters of the same mass and age do not present the same unique values of their...
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PublicaciónConfidence levels of evolutionary synthesis models. II. On sampling and Poissonian fluctuationsIn terms of statistical fluctuations, stellar population synthesis models are only asymptotically correct in the limit of a large number of stars, where...
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PublicaciónConfidence Limits of Evolutionary Synthesis ModelsThe probabilistic nature of the IMF in stellar systems implies that clusters of the same mass and age do not present the same unique values of their observed...
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PublicaciónConfidence limits of evolutionary synthesis models. III. On time-integrated quantitiesEvolutionary synthesis models are a fundamental tool to interpret the properties of observed stellar systems. In order to achieve a meaningful comparison...
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PublicaciónConfidence limits of evolutionary synthesis models. IV. Moving forward to a probabilistic formulationContext: .Synthesis models predict the integrated properties of stellar populations. Several problems exist in this field, mostly related to the fact that...
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PublicaciónConfirmation and characterisation of three giant planets detected by TESS from the FIES/NOT and Tull/McDonald spectrographsWe report the confirmation and characterisation of TOI-1820 b, TOI-2025 b, and TOI-2158 b, three Jupiter-sized planets on short-period orbits around G-type...
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PublicaciónConfirmation and refutation of very luminous galaxies in the early UniverseDuring the first 500 million years of cosmic history, the first stars and galaxies formed, seeding the Universe with heavy elements and eventually reionizing...
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PublicaciónConfirmation of a Kinematic Diagnostic for Face-On Box/Peanut-shaped BulgesWe present the results of high-resolution absorption-line spectroscopy of three face-on galaxies, NGC 98, NGC 600, and NGC 1703, with the aim of searching for...
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PublicaciónConfirmation of a Sub-Saturn-size Transiting Exoplanet Orbiting a G Dwarf: TOI-1194 b and a Very Low Mass Companion Star: TOI-1251 B from TESSWe report the confirmation of a sub-Saturn-size exoplanet, TOI-1194 b, with a mass of about ${0.456}_{-0.051}^{+0.055}$ M J, and a very low mass companion star...