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Gran Telescopio Canarias observations of an overdense region of Lyman α emitters at z = 6.5 |
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Uncertainties in the solar photospheric oxygen abundance |
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Early-type massive stars in Carina Nebula within the Gaia-ESO Survey. |
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Creating lenticular galaxies with mergers |
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Non-Vestoid candidate asteroids in the inner main belt |
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HADES RV Programme with HARPS-N at TNG. II. Data treatment and simulations<xref ref-type="fn" rid="FN1"> |
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On the Dearth of Ultra-faint Extremely Metal-poor Galaxies |
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A very dark stellar system lost in Virgo: kinematics and metallicity of SECCO 1 with MUSE |
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On the determination of the He abundance distribution in globular clusters from the width of the main sequence |
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EELT-HIRES the high-resolution spectrograph for the E-ELT |
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Commissioning and first observations with Wide FastCam at the Telescopio Carlos Sánchez |
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Massive Stars: Some Open Questions and the Role of Multi-Object Spectroscopy |
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HADES RV program with HARPS-N at the TNG GJ 3998: An early M-dwarf hosting a system of super-Earths |
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A search for hydrogenated fullerenes in fullerene-containing planetary nebulae |
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Roche tomography of cataclysmic variables - VII. The long-term magnetic activity of AE Aqr |
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Recent SFR calibrations and the constant SFR approximation |
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The featureless and non-variable optical spectral energy distribution of AXP 4U 0142+61 |
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VLT FORS2 optical imaging and spectroscopy of nine luminous type 2 AGN at 0.3 < z < 0.6 - I. Ionized gas nebulae |
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Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes |
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Chromospheric Diagnosis with Ca II Lines: Forward Modeling in Forward Scattering. I |
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Asteroseismology of OB stars with hundreds of single snapshot spectra (and a few time-series of selected targets) |
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Defocused transmission spectroscopy: a potential detection of sodium in the atmosphere of WASP-12b |
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Very low-luminosity Class I/flat outflow sources in σ Orionis |
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Brown dwarfs of the Galactic halo. |
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Physical properties of simulated galaxy populations at z = 2 - II. Effects of cosmology, reionization and ISM physics |
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