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μ<SUB>⋆</SUB> masses: weak-lensing calibration of the Dark Energy Survey Year 1 redMaPPer clusters using stellar masses |
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Hace 2 months 1 week |
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Relations among structural parameters in barred galaxies with a direct measurement of bar pattern speed |
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HORuS transmission spectroscopy of 55 Cnc e |
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SMASHing the low surface brightness SMC |
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Testing two-component models on very high-energy gamma-ray-emitting BL Lac objects |
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Planck 2018 results. II. Low Frequency Instrument data processing |
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TESS asteroseismology of the known planet host star λ<SUP>2</SUP> Fornacis |
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NIHAO XXIV: rotation- or pressure-supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics |
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Atmospheric characterization of the ultra-hot Jupiter MASCARA-2b/KELT-20b. Detection of Ca II, Fe II, Na I, and the Balmer series of H (Hα, Hβ, and Hγ) with high-dispersion transit spectroscopy (Corrigendum) |
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Hace 2 months 1 week |
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K2-280 b - a low density warm sub-Saturn around a mildly evolved star |
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Historical Perspectives on the Concept of Galaxy Size |
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Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra |
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Cold molecular gas and PAH emission in the nuclear and circumnuclear regions of Seyfert galaxies |
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The CARMENES search for exoplanets around M dwarfs. Measuring precise radial velocities in the near infrared: The example of the super-Earth CD Cet b |
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HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away |
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Determining the dynamics and magnetic fields in He I 10830 Å during a solar filament eruption |
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The Black Hole Mass-Color Relations for Early- and Late-type Galaxies: Red and Blue Sequences |
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TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet |
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Numerical determination of the cutoff frequency in solar models |
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Searching for electromagnetic counterparts to gravitational-wave merger events with the prototype Gravitational-Wave Optical Transient Observer (GOTO-4) |
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Phosphorus-rich stars with unusual abundances are challenging theoretical predictions |
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The age-chemical abundance structure of the Galactic disc - II. α-dichotomy and thick disc formation |
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The Multiplanet System TOI-421 |
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Gas and dust cooling along the major axis of M 33 (HerM33es). Herschel/PACS [C II] and [O I] observations |
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OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk |
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Hace 2 months 1 week |
