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Modeling of the HerMES Submillimeter Source Lensed by a Dark Matter Dominated Foreground Group of Galaxies |
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The suppression of star formation by powerful active galactic nuclei |
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HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background |
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A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy |
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The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals |
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GRIS: The GREGOR Infrared Spectrograph |
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Polar Field Reversal Observations with Hinode |
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Qualitative Interpretation of Galaxy Spectra |
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The star formation history and dust content in the far outer disc of M31 |
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The ACS Survey of Galactic Globular Clusters. IX. Horizontal Branch Morphology and the Second Parameter Phenomenon |
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