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Extinction curve template for intrinsically reddened quasars |
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Hace 4 months |
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Evidence for a metal-poor population in the inner Galactic bulge |
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Hace 4 months |
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Analysis of the acoustic cut-off frequency and high-frequency peaks in six Kepler stars with stochastically excited pulsations |
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Planck intermediate results. XXV. The Andromeda galaxy as seen by Planck |
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The Gaia-ESO Survey: chemical signatures of rocky accretion in a young solar-type star |
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HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies |
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Swift J1357.2-0933: a massive black hole in the Galactic thick disc |
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The WEBT campaign on the BL Lac object PG 1553+113 in 2013. An analysis of the enigmatic synchrotron emission |
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Analysis techniques and performance of the Domino Ring Sampler version 4 based readout for the MAGIC telescopes |
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The Arizona Radio Observatory Survey of Molecular Gas in Nearby Normal Spiral Galaxies I: The Data |
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Surface abundances of ON stars |
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Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible |
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Solar Space Density of the Red Clump Stars and the Scale-Length of the Thin Disc |
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The Role of Bars in AGN Fueling in Disk Galaxies Over the Last Seven Billion Years |
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Determination of the spectroscopic stellar parameters for 257 field giant stars★ |
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Further evidence for a time-dependent initial mass function in massive early-type galaxies |
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Mass constraints to Sco X-1 from Bowen fluorescence and deep near-infrared spectroscopy |
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Homogeneous Photometry VI: Variable Stars in the Leo I Dwarf Spheroidal Galaxy |
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The Na-O anticorrelation in horizontal branch stars. V. NGC 6723 |
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Chemoarchaeological downsizing in a hierarchical universe: impact of a top-heavy IGIMF |
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MAGIC reveals a complex morphology within the unidentified gamma-ray source HESS J1857+026 |
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Planck 2013 results. VI. High Frequency Instrument data processing |
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Planck 2013 results. IV. Low Frequency Instrument beams and window functions |
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The extremely red L dwarf ULAS J222711-004547 - dominated by dust |
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Hace 4 months |
