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QUIJOTE scientific results - III. Microwave spectrum of intensity and polarization in the Taurus Molecular Cloud complex and L1527 |
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5 hours 13 minutes ago |
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MuSCAT2: four-color simultaneous camera for the 1.52-m Telescopio Carlos Sánchez |
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HD 219666 b: a hot-Neptune from TESS Sector 1 |
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Diagnostic potential of the Ca II 8542 Å line for solar filaments |
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Spectral analysis of the barium central star of the planetary nebula Hen 2-39 |
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Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation |
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Back to the Lithium Plateau with the [Fe/H] < -6 Star J0023+0307 |
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A planetesimal orbiting within the debris disc around a white dwarf star |
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The metallicity-period-mass diagram of low-mass exoplanets |
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Physical properties and transmission spectrum of the WASP-74 planetary system from multiband photometry |
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Multiwavelength spectroscopy of the black hole candidate MAXI J1813-095 during its discovery outburst |
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A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015 |
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A compact jet at the infrared heart of the prototypical low-luminosity AGN in NGC 1052 |
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A search for red giant solar-like oscillations in all Kepler data |
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4MOST: Project overview and information for the First Call for Proposals |
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The Proper-motion Field along the Magellanic Bridge: A New Probe of the LMC–SMC Interaction |
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Chemical Abundances of Main-sequence, Turnoff, Subgiant, and Red Giant Stars from APOGEE Spectra. II. Atomic Diffusion in M67 Stars |
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Chemical Cartography with APOGEE: Multi-element Abundance Ratios |
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Exploring the Very Extended Low-surface-brightness Stellar Populations of the Large Magellanic Cloud with SMASH |
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Gaia DR 2 and VLT/FLAMES search for new satellites of the LMC |
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From kpcs to the central parsec of NGC 1097: feeding star formation and a black hole at the same time |
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The CARMENES search for exoplanets around M dwarfs. Chromospheric modeling of M 2-3 V stars with PHOENIX |
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The Arches cluster revisited. III. An addendum to the stellar census |
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Ca line formation in late-type stellar atmospheres. I. The model atom |
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The Weakening Outburst of the Young Eruptive Star V582 Aur |
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