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The GAPS Programme at TNG. XXXI. The WASP-33 system revisited with HARPS-N |
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5 months 2 weeks ago |
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The PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey |
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OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf |
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Bayesian Evidence for a Nonlinear Damping Model for Coronal Loop Oscillations |
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Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering |
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Assessing the Stellar Population and the Environment of an H II Region on the Far Side of the Galaxy |
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Temporal evolution of small-scale internetwork magnetic fields in the solar photosphere |
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Progress Report on the Large-Scale Polarization Explorer |
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Dynamical modelling of CXOGBS J175553.2-281633: a 10 h long orbital period cataclysmic variable |
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Final assembly, metrology, and testing of the WEAVE fibre positioner |
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Intensity interferometry with MAGIC |
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The ORP on-sky community access program for adaptive optics instrumentation development |
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Using radial velocities to reveal black holes in binaries: A test case |
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Robust asteroseismic properties of the bright planet host HD 38529 |
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Studying star-forming processes at core and clump scales: the case of the young stellar object G29.862-0.0044 |
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The absolute proper motions of the Arches and Quintuplet clusters |
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HST Survey of the Orion Nebula Cluster in the H<SUB>2</SUB>O 1.4 μm Absorption Band. III. The Population of Substellar Binary Companions |
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HELP project - a dreamed-of multiwavelength dataset for SED fitting: The influence of used models for the main physical properties of galaxies |
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MASTER Transient Discovery Report for 2020-05-23 |
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SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data |
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Can we detect the stellar differential rotation of WASP-7 through the Rossiter-McLaughlin observations? |
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The OTELO survey. A case study of [O III] λ4959,5007 emitters at ⟨z⟩ = 0.83 |
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Thermal emission from the amorphous dust: An alternative possibility of the origin of the anomalous microwave emission |
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Kinematic and metallicity properties of the Aquarius dwarf galaxy from FORS2 MXU spectroscopy⋆ |
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A hydrodynamical study of outflows in starburst galaxies with different driving mechanisms |
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