QUIJOTE: el estado de la instrumentación CMB en Canarias.
Durante este seminario se hará un recorrido sobre la instrumentación dentro del proyecto QUIJOTE, desde de los instrumentos ya existentes y su problemática...
Dwarf spheroidal (dSph) galaxies are the smallest, closest and most abundant galaxies in the Universe and therefore excellent laboratories to study star...
Reconstructing the history of the Milky Way and probing the dark matter nature in WEAVE and LSST era
At present, our understanding of the formation history of the MW is limited due to the complexity of observing the imprints of accretion events and of...
Recurrent Strong Outbursts of an EXor-like Young Eruptive Star Gaia20eae
We present follow-up photometric and spectroscopic observations, and subsequent analysis of Gaia20eae. This source triggered photometric alerts during 2020...
Revealing planet migration and detection of terrestrial planets with improved spectroscopic tools
Spectroscopic observations of stars do not only provide us with valuable information about the stars themselves, but over the last years such observations have...
Revisiting the impact of stellar magnetic activity on the detection of solar-like oscillations by Kepler
Over 2,000 stars were observed for one month with a high enough cadence in order to look for acoustic modes during the survey phase of the Kepler mission. Solar...
The Sloan Extension for Galactic Understanding and Exploration 2 (SEGUE-2) obtained 128,288 low-resolution spectra (R ~ 1800) of 118,958 unique stars in the...
Single-epoch and Differential Astrometric Microlensing of Quasars
We propose and discuss a new experimental approach to measure the centroid shift induced by gravitational microlensing in the images of lensed quasars...