Publication type: Refereed

  • Publication
    How to plan your astronomy research paper in ten steps
    Scientific writing is an important skill for a career as a professional astrophysicist. However, very few researchers receive any formal training in how to...
  • Publication
    How to prepare competitive proposals and job applications
    Writing proposals and job applications is arguably one of the most important tasks in the career of a scientist. The proposed ideas must be scientifically...
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    How to write and develop your astronomy research paper
    Writing is a vital component of a modern career in scientific research. But how to write correctly and effectively is often not included in the training that...
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    How well can we unravel the accreted constituents of the Milky Way stellar halo?: A test on cosmological hydrodynamical simulations
    Context. One of the primary goals of Galactic Archaeology is to reconstruct the Milky Way's accretion history. To achieve this, significant efforts have been...
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    HR 10 as seen by CHEOPS and TESS: Revealing δ Scuti pulsations, granulation-like signal and hint for transients
    Context. HR 10 has only recently been identified as a binary system. Previously thought to be an A-type shell star, it appears that both components are fast...
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    HS 0139+0559, HS 0229+8016, HS 0506+7725, and HS 0642+5049: four new long-period cataclysmic variables
    We present time-resolved optical spectroscopy and photometry of four relatively bright (V˜14.0-15.5) long-period cataclysmic variables (CVs) discovered in the...
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    HS 0943+1404, a true intermediate polar
    We have identified a new intermediate polar, HS 0943+1404, as part of our ongoing search for cataclysmic variables in the Hamburg Quasar Survey. The orbital and...
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    HS 1857+5144: a hot and young pre-cataclysmic variable
    Aims:We report the discovery of a new white dwarf/M dwarf binary, HS 1857+5144, identified in the Hamburg Quasar Survey (HQS). Methods: Time-resolved optical...
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    HS 2325+8205 - An Ideal Laboratory for Accretion Disk Physics
    We identify HS 2325+8205 as an eclipsing, frequently outbursting, dwarf nova with an orbital period of Porb = 279.841731(5) minutes. Spectroscopic observations...