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A hybrid type Ia supernova with an early flash triggered by helium-shell detonation |
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Target Selection for the SDSS-IV APOGEE-2 Survey |
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Tests and Problems of the Standard Model in Cosmology |
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Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere |
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Red Supergiants as Cosmic Abundance Probes: Massive Star Clusters in M83 and the Mass–Metallicity Relation of Nearby Galaxies |
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Effect of the stellar absorption line centre-to-limb variation on exoplanet transmission spectrum observations |
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Sardinia Radio Telescope observations of Abell 194. The intra-cluster magnetic field power spectrum |
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DeepVel: Deep learning for the estimation of horizontal velocities at the solar surface |
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Numerical simulations of quiet Sun magnetic fields seeded by the Biermann battery |
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Formation of S0 galaxies through mergers. Evolution in the Tully-Fisher relation since z ∼ 1 |
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Metallicity effect on stellar granulation detected from oscillating red giants in open clusters |
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Spectroscopy of 10 γ-Ray BL Lac Objects at High Redshift |
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Adding the s-Process Element Cerium to the APOGEE Survey: Identification and Characterization of Ce ii Lines in the H-band Spectral Window |
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APOGEE Chemical Abundances of the Sagittarius Dwarf Galaxy |
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The Apache Point Observatory Galactic Evolution Experiment (APOGEE) |
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Performance of the MAGIC telescopes under moonlight |
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The Radial Distribution of Mono-metallicity Populations in the Galactic Disk as Evidence for Two-phase Disk Formation |
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The Mass Function of GX 339–4 from Spectroscopic Observations of Its Donor Star |
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The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA |
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Atypical Mg-poor Milky Way Field Stars with Globular Cluster Second-generation-like Chemical Patterns |
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A mid-infrared statistical investigation of clumpy torus model predictions |
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Observational constraints to boxy/peanut bulge formation time |
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Dynamical dark energy in light of the latest observations |
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The Physics and Diagnostic Potential of Ultraviolet Spectropolarimetry |
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VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35 |
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