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QUIJOTE scientific results - V. The microwave intensity and polarization spectra of the Galactic regions W49, W51 and IC443 |
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Mineralogical analysis of 14 PHAs from ViNOS data |
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Lightcurve analysis of near-Earth objects from the IMPACTON project: Evidence of binary systems and cohesion strength |
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Fitting of supernovae without dark energy |
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Hunting for anti-solar differentially rotating stars using the Rossby number. An application to the Kepler field |
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Ambipolar Diffusion in the Lower Solar Atmosphere: Magnetohydrodynamic Simulations of a Sunspot |
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TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star |
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First light of NIRPS, the near-infrared adaptive-optics assisted high resolution spectrograph for the ESO 3.6m |
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Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT-34b, CoRoT-35b, and CoRoT-36b |
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A Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence |
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Asteroid Lightcurves from the MOA-II Survey: a pilot study |
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The Pristine survey - XVIII. C-19: tidal debris of a dark matter-dominated globular cluster? |
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Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. I. Evidence for Thermal Energy Anisotropy Using Oriented Stacking |
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Generalized Fluid Models of the Braginskii Type |
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Plenoptic wavefront sensor for free-space optical communications |
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Multicomponent scalar dark matter at high-intensity proton beam experiments |
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Probing for the host galaxies of the fast X-ray transients XRT 000519 and XRT 110103 |
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Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves. II. Period-Fourier-Metallicity Relations for First Overtone RR Lyrae |
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The TESS-Keck Survey: Science Goals and Target Selection |
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A comprehensive study of the opposition effect on 15 NEOs |
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Is Terzan 5 the remnant of a building block of the Galactic bulge? Evidence from APOGEE |
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Limits on the Hard X-Ray Emission From the Periodic Fast Radio Burst FRB 180916.J0158+65 |
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SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO/Virgo Event GW190814 |
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From Naked Spheroids to Disky Galaxies: How Do Massive Disk Galaxies Shape Their Morphology? |
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Dark Energy Survey Year 3 results: galaxy sample for BAO measurement |
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Hace 3 months 1 week |