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Hot Jupiters around M dwarfs. A sensitivity analysis of the WFCAM Transit Survey |
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A PCA approach to stellar effective temperatures |
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X-ray luminosity functions of different morphological and X-ray type AGN populations |
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The Herschel census of infrared SEDs through cosmic time |
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Gamma-ray burst science in the era of the Cherenkov Telescope Array |
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On the interpolation of model atmospheres and high-resolution synthetic stellar spectra |
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Searching for the signatures of terrestrial planets in F-, G-type main-sequence stars |
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Microlensing of Quasar Broad Emission Lines: Constraints on Broad Line Region Size |
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IPHAS J062746.41+014811.3: A Deeply Eclipsing Intermediate Polar |
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Automated Unsupervised Classification of the Sloan Digital Sky Survey Stellar Spectra using k-means Clustering |
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Characterizing Two Solar-type Kepler Subgiants with Asteroseismology: KIC 10920273 and KIC 11395018 |
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τ Boötis b: Hunting for reflected starlight |
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A multi-wavelength analysis of M 81: insight on the nature of Arp's loop |
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Herschel ATLAS: The cosmic star formation history of quasar host galaxies |
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Tracking the impact of environment on the galaxy stellar mass function up to z ~ 1 in the 10 k zCOSMOS sample |
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Astrometric search for a planet around VB 10 |
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The pulsations of PG 1351+489 |
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NoMaDS: The Northern Massive Dim Stars Survey |
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The chemical composition of the Orion star forming region. I. Homogeneity of O and Si abundances in B-type stars |
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NGC 1624-2: a slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field |
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Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments |
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VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies. II. Evidence for shock ionization caused by tidal forces in the extra-nuclear regions of interacting and merging LIRGs |
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A Bright Radio HH Object with Large Proper Motions in the Massive Star-forming Region W75N |
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Rayleigh-Taylor Instability in Partially Ionized Compressible Plasmas |
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