Tipo de publicación: Sin árbitro

  • Publicación
    Tracing the Coronal Line Region in AGN with VLT/NACO: The Very First Results
    The coronal line region in AGN is an intermediate zone between the broad- and the narrow-line regions where lines with ionization potentials, IP >50 eV, are...
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    Tracing the current SFR of the Local Universe and beyond
    Not Available
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    Tracing the Star Formation Rate in the Local Universe: The UCM Survey
    Not Available
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    Tracking Stars with the Fluorescence Detector of the Pierre Auger Observatory
    Recording tracks of stars traversing the field of view of the Auger's fluorescence detector (FD) is a powerful to ol to monitor various FD parameters. For...
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    Tracking the Clumping in OB Stars from UV to radio
    We review different line and continua diagnostics from the UV to radio, which can be utilized to simultaneously constrain the clumping structure throughout the...
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    Transformations between the 2MASS, SDSS, and BV I photometric systems for late-type giants
    We present colour transformations from Two Micron All Sky Survey (2MASS) photometric system to Johnson-Cousins system and to Sloan Digital Sky Survey (SDSS)...
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    Transient and multi-messenger astrophysics with the Cherenkov Telescope Array
    The Cherenkov Telescope Array (CTA) will be the next generation ground-based very-high-energy (VHE) gamma-ray observatory. The first of the Large Size...
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    Transit light curves of WASP-10 b (Maciejewski+, 2011)
    Light curves of four WASP-10 b's transits observed in 2010 are given. Data were collected with the Calar Alto Faint Object Spectrograph (CAFOS) on the 2.2-m...
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    Transit Photometry as an Exoplanet Discovery Method
    Photometry with the transit method has arguably been the most successful exoplanet discovery method to date. A short overview about the rise of that method to...