Tipo de publicación: Sin árbitro

  • Publicación
    Too Few to be Relevant: Major Merger Statistics up to z ˜ 1
    We study the evolution of galaxy structure and of the major merger fraction since z ˜ 1 to present in GOODS-S field for MB ≤ -20 and M* ≥ 1010 Msun selected...
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    Tools for Transit and Radial Velocity Modeling and Analysis
    An overview over analysis or modelling tools related to the radial velocity and transit methods for exoplanet detection and characterization is given, with over...
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    Toward a comprehensive characterization of L subdwarfs
    Subsolar metallicity L subdwarfs was discovered over a decade ago, but remain poor understood due to lack of known objects. We started to search for L subdwarfs...
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    Toward a detailed, reliable and comprehensive star formation history of the Small Magellanic Cloud
    The Small Magellanic Cloud is a crucial galaxy to understand many aspects of the formation and evolution of galaxies. We propose to collect deep photometry in...
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    Towards a Comprehensive View of the Carina Nebula Through the Spectroscopic Study of Its O-Star Population
    The Carina Nebula is one of the major and more massive regions of our Galaxy that contains a large number of massive O-type stars that can be analyzed...
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    Towards a fully automated eclipsing binary solver for Gaia
    Gaia, an ESA cornerstone mission, will obtain of the order of 100 high-precision photometric observations and lower precision radial velocity measurements over...
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    Towards a fully automatic and robust DIMM (DIMMA)
    Quantitative seeing measurements have been provided at the Canarian Observatories since 1990 by differential image motion monitors (DIMMs). Image quality needs...
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    Towards a Global Picture of OB Associations
    In this contribution we present our on-going project about the understanding of the evolution of galactic OB associations and the implications on the global...
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    Towards a New Classification of Early-type Galaxies: An Integral-field View
    In this proceedings paper we make use of the two-dimensional stellar kinematics of a representative sample of E and S0 galaxies obtained with the SAURON...