Publication type: Non-refereed

  • Publication
    The Galaxy-wide IMF - from Star Clusters to Galaxies
    Over the past years observations of young and populous star clusters have shown that the stellar initial mass function (IMF) can be conveniently described by a...
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    The gamma-ray bright BL Lac object RX J1211+2242
    RX J1211+2242 is an optically faint (B ≃ 19.2 mag) but X-ray bright (f2 - 10 keV = 5 × 10-12 erg cm-2 s-1) AGN, which has been shown to be a BL Lac object at...
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    The Gamow Explorer: a Gamma-Ray Burst Observatory to study the high redshift universe and enable multi-messenger astrophysics
    The Gamow Explorer will use Gamma Ray Bursts (GRBs) to: 1) probe the high redshift universe (z < 6) when the first stars were born, galaxies formed and Hydrogen...
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    The gas-star cycle in nearby early-type galaxies insights from UV, optical, and mm
    Not Available
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    The GCS Data Processing Kit
    As part of the GTC Control System (GCS) a data processing package is being developed. We will describe the perfomance of the Data Processing Kit (DPK), using...
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    The Generation and Transfer of Polarized Radiation in Stellar Atmospheres
    The standard Non-LTE problem consists in calculating the atomic level populations that are consistent with the intensity of the radiation field generated within...
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    The GEO-HF project
    The GEO 600 gravitational wave detector uses advanced technologies including signal recycling and monolithic fused-silica suspensions to achieve a sensitivity...
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    The Ghost Light of Abell 2744
    Originally thought to explore the high redshift Universe, the extreme depth of the Frontier Fields survey provides also an excellent opportunity to explore with...
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    The giant bubble Hubble III.
    This paper presents the results of the authors' study on the giant (radius = 60 pc) extragalactic H II region Hubble III in NGC 6822. Based on the observational...