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SPIRE imaging of M 82: Cool dust in the wind and tidal streams |
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Herschel reveals a Tdust-unbiased selection of z ~ 2 ultraluminous infrared galaxies |
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The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images |
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On the origin of M81 group extended dust emission |
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HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations |
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Submillimetre galaxies reside in dark matter haloes with masses greater than 3×1011 solar masses |
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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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Observations and Implications of Large-amplitude Longitudinal Oscillations in a Solar Filament |
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GRIS: The GREGOR Infrared Spectrograph |
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The GREGOR Fabry-Pérot Interferometer |
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Biosignatures as revealed by spectropolarimetry of Earthshine |
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Photometric Variability of the Disk-integrated Thermal Emission of the Earth |
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Analysis of Quiet-Sun Internetwork Magnetic Fields Based on Linear Polarization Signals |
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Polar Field Reversal Observations with Hinode |
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Chromospheric activities and kinematics for solar type dwarfs and subgiants: analysis of the activity distribution and the AVR |
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On the Extreme Positive Star Formation Feedback Condition in Scuba Sources |
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On the Origin of the Type II Spicules: Dynamic Three-dimensional MHD Simulations |
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The star formation history and dust content in the far outer disc of M31 |
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The Carina Project. V. The Impact of NLTE Effects on the Iron Content |
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The ACS Survey of Galactic Globular Clusters. IX. Horizontal Branch Morphology and the Second Parameter Phenomenon |
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Sodium-Oxygen Anticorrelation and Neutron-capture Elements in Omega Centauri Stellar Populations |
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The two metallicity groups of the globular cluster M 22: a chemical perspective |
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Multiple Stellar Populations in 47 Tucanae |
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The C+N+O Abundance of ω Centauri Giant Stars: Implications for the Chemical-enrichment Scenario and the Relative Ages of Different Stellar Populations |
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Hace 1 month 1 week |