Optical Characterisation of the Planck PSZ1 Galaxy Cluster Catalogue: Building a Reference Sample for CosmologyAntonio Ferragamo102019
Pioneering the Use of a Plenoptic Adaptive Optics System for Free Space Optical CommunicationsNOELIA MARTÍNEZ REY
Near-infrared Spectroscopy of Three Nearby L Dwarfs
Not Available Based on observations collected at the European Southern Observatory.Lodieu, Nicolas et al.
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-like oscillations have been detected in about 540 stars. The question of why no oscillations were detected in the remaining stars is still open. Previous works explained the non-detectionMathur, Savita et al.
All-sky angular power spectra from cleaned WISE×SuperCOSMOS galaxy number counts
Aiming to extract cosmological information from linear scales of the WISE×SuperCOSMOS photometric redshift catalog, we perform a characterization of the systematic effects associated with stellar content, evidencing the presence of contamination and obscuration. We create an integrated model for these effects (which together we call "usurperXavier, H. S. et al.
FIRTEZ-dz. A forward and inverse solver of the polarized radiative transfer equation under Zeeman regime in geometrical scale
We present a numerical code that solves the forward and inverse problem of the polarized radiative transfer equation in geometrical scale under the Zeeman regime. The code is fully parallelized, making it able to easily handle large observational and simulated datasets. We checked the reliability of the forward and inverse modules through differentPastor Yabar, A. et al.