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The Bulk of the Black Hole Growth Since z ~ 1 Occurs in a Secular Universe: No Major Merger-AGN Connection |
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Secular Evolution and a Non-evolving Black-hole-to-galaxy Mass Ratio in the Last 7 Gyr |
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The Chandra COSMOS Survey. III. Optical and Infrared Identification of X-Ray Point Sources |
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Far-infrared properties of submillimeter and optically faint radio galaxies |
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Building the cosmic infrared background brick by brick with Herschel/PEP |
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Infrared astronomical characteristics of the Roque de los Muchachos Observatory: precipitable water vapour statistics |
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On the mass of the neutron star in Cyg X-2 |
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A first catalogue of automatically selected ultraviolet-excess sources from the UVEX survey |
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On the binary nature of the γ-ray sources AGL J2241+4454 (= MWC 656) and HESS J0632+057 (= MWC 148) |
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Chemical abundance analysis of the open clusters Cr 110, NGC 2099 (M 37), NGC 2420, NGC 7789, and M 67 (NGC 2682) |
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Metallicities, Age-Metallicity Relationships, and Kinematics of Red Giant Branch Stars in the Outer Disk of the Large Magellanic Cloud |
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Chemical abundance analysis of the open clusters Berkeley 32, NGC 752, Hyades, and Praesepe |
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Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters . Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266 |
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Mapping the properties of blue compact dwarf galaxies: integral field spectroscopy with PMAS |
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The Distance, Mass, and Radius of the Neutron Star in 4U 1608-52 |
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Scattering Polarization of the Ca II IR Triplet for Probing the Quiet Solar Chromosphere |
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Scattering Polarization and Hanle Effect in Stellar Atmospheres with Horizontal Inhomogeneities |
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The star-formation rates of 1.5 < z < 2.5 massive galaxies |
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Star formation in AGN hosts in GOODS-N |
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Herschel unveils a puzzling uniformity of distant dusty galaxies |
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Dissecting the cosmic infra-red background with Herschel/PEP |
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The far-infrared/radio correlation as probed by Herschel |
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PACS Evolutionary Probe (PEP) - A Herschel key program |
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On Star Formation Rates and Star Formation Histories of Galaxies Out to z ~ 3 |
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A Herschel view of the far-infrared properties of submillimetre galaxies |
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