@misc{DolezalovaKubatovaKubatetal.2019,
  author    = {Dolezalova, Barbora and Kubatova, Brankica and Kubat, Jiri and Hamann, Wolf-Rainer},
  title     = {The Quasi-WR Star HD 45166 Revisited},
  series = {Radiative signatures from the cosmos},
  volume    = {519},
  journal   = {Radiative signatures from the cosmos},
  publisher = {Astronomical soc pacific},
  address   = {San Fransisco},
  isbn      = {978-1-58381-925-8},
  issn      = {1050-3390},
  pages     = {197 -- 200},
  year      = {2019},
  abstract  = {We studied the wind of the quasi Wolf-Rayet (qWR) star HD 45166. As a first step we modeled the observed UV spectra of this star by means of the state-of-the-art Potsdam Wolf-Rayet (PoWR) atmosphere code. We inferred the wind parameters and compared them with previous findings.},
  language  = {en}
}
@misc{GruendePaterShowalteretal.2006,
  author    = {Gr{\"u}n, Eberhard and de Pater, Imke and Showalter, Mark and Spahn, Frank and Srama, Ralf},
  title     = {Physics of dusty rings: History and perspective},
  series = {Planetary and space science},
  volume    = {54},
  journal   = {Planetary and space science},
  number    = {9-10},
  publisher = {Elsevier},
  address   = {Oxford},
  issn      = {0032-0633},
  doi       = {10.1016/j.pss.2006.05.005},
  pages     = {837 -- 843},
  year      = {2006},
  language  = {en}
}
@misc{Goychuk2019,
  author    = {Goychuk, Igor},
  title     = {Comment on "Anomalous Escape Governed by Thermal 1/f Noise" Reply (R. K. Singh)},
  series = {Physical review letters},
  volume    = {123},
  journal   = {Physical review letters},
  number    = {23},
  publisher = {American Physical Society},
  address   = {College Park},
  issn      = {0031-9007},
  doi       = {10.1103/PhysRevLett.123.238902},
  pages     = {1},
  year      = {2019},
  language  = {en}
}
@misc{CestnikAbel2019,
  author    = {Cestnik, Rok and Abel, Markus},
  title     = {Erratum: Inferring the dynamics of oscillatory systems using recurrent neural networks (Chaos : an interdisciplinary journal of nonlinear science. - 29 (2019) 063128)},
  series = {Chaos : an interdisciplinary journal of nonlinear science},
  volume    = {29},
  journal   = {Chaos : an interdisciplinary journal of nonlinear science},
  number    = {8},
  publisher = {American Institute of Physics},
  address   = {Melville},
  issn      = {1054-1500},
  doi       = {10.1063/1.5122803},
  pages     = {1},
  year      = {2019},
  language  = {en}
}
@misc{JavanainenMartinezSearaMetzleretal.2017,
  author    = {Javanainen, Matti and Martinez-Seara, Hector and Metzler, Ralf and Vattulainen, Ilpo Tapio},
  title     = {Diffusion of Proteins and Lipids in Protein-Rich Membranesa},
  series = {Biophysical journal},
  volume    = {114},
  journal   = {Biophysical journal},
  number    = {3},
  publisher = {Cell Press},
  address   = {Cambridge},
  issn      = {0006-3495},
  doi       = {10.1016/j.bpj.2017.11.3009},
  pages     = {551A -- 551A},
  year      = {2017},
  language  = {en}
}
@misc{GudowskaNowakLindenbergMetzler2017,
  author    = {Gudowska-Nowak, Ewa and Lindenberg, Katja and Metzler, Ralf},
  title     = {Preface: Marian Smoluchowski's 1916 paper—a century of inspiration},
  series = {Journal of physics : A, Mathematical and theoretical},
  volume    = {50},
  journal   = {Journal of physics : A, Mathematical and theoretical},
  number    = {38},
  publisher = {IOP Publ. Ltd.},
  address   = {Bristol},
  issn      = {1751-8113},
  doi       = {10.1088/1751-8121/aa8529},
  pages     = {8},
  year      = {2017},
  language  = {en}
}
@misc{ParsonsSchuesslerGarrigouxetal.2017,
  author    = {Parsons, R. D. and Sch{\"u}ssler, F. and Garrigoux, T. and Balzer, A. and F{\"u}ssling, Matthias and Hoischen, Clemens and Holler, M. and Mitchell, A. and P{\"u}hlhofer, G. and Rowell, G. and Wagner, S. and Bissaldi, E. and Tam, P. H. T.},
  title     = {The HESS II GRB Observation Scheme},
  series = {AIP conference proceedings / American Institute of Physics},
  volume    = {1792},
  journal   = {AIP conference proceedings / American Institute of Physics},
  number    = {1},
  publisher = {American Institute of Physics},
  address   = {Melville},
  organization    = {HESS Collaboration},
  isbn      = {978-0-7354-1456-3},
  issn      = {0094-243X},
  doi       = {10.1063/1.4968980},
  pages     = {5},
  year      = {2017},
  abstract  = {Gamma-ray bursts (GRBs) are some of the Universe's most enigmatic and exotic events. However, at energies above 10 GeV their behaviour remains largely unknown. Although space based telescopes such as the Fermi-LAT have been able to detect GRBs in this energy range, their photon statistics are limited by the small detector size. Such limitations are not present in ground based gamma-ray telescopes such as the H.E.S.S. experiment, which has now entered its second phase with the addition of a large 600 m2 telescope to the centre of the array. Such a large telescope allows H.E.S.S. to access the sub 100-GeV energy range while still maintaining a large effective collection area, helping to potentially probe the short timescale emission of these events. We present a description of the H.E.S.S. GRB observation programme, summarising the performance of the rapid GRB repointing system and the conditions under which GRB observations are initiated. Additionally we will report on the GRB follow-ups made during the 2014-15 observation campaigns.},
  language  = {en}
}
@misc{AnguenerAharonianBordasetal.2017,
  author    = {Ang{\"u}ner, Ekrem Oǧuzhan and Aharonian, Felix A. and Bordas, Pol and Casanova, Sabrina and Hoischen, Clemens and Oya, I. and Ziegler, A.},
  title     = {HESS J1826-130},
  series = {AIP conference proceedings / American Institute of Physics},
  volume    = {1792},
  journal   = {AIP conference proceedings / American Institute of Physics},
  number    = {1},
  publisher = {American Institute of Physics},
  address   = {Melville},
  organization    = {HESS Collaboration},
  isbn      = {978-0-7354-1456-3},
  issn      = {0094-243X},
  doi       = {10.1063/1.4968928},
  pages     = {6},
  year      = {2017},
  abstract  = {HESS J1826-130 is an unidentified hard spectrum source discovered by H.E.S.S. along the Galactic plane, the spectral index being Gamma = 1.6 with an exponential cut-off at about 12 TeV. While the source does not have a clear counterpart at longer wavelengths, the very hard spectrum emission at TeV energies implies that electrons or protons accelerated up to several hundreds of TeV are responsible for the emission. In the hadronic case, the VHE emission can be produced by runaway cosmic-rays colliding with the dense molecular clouds spatially coincident with the H.E.S.S. source.},
  language  = {en}
}
@misc{ThoelertHoermannAntreichetal.2017,
  author    = {Thoelert, Steffen and H{\"o}rmann, Ulrich and Antreich, Felix and Meurer, Michael},
  title     = {Ionospheric effects on high gain antenna GNSS measurements},
  series = {Proceedings of the 30th International Technical Meeting of the Satellite Division of The Institute of Navigation (ION GNSS+ 2017)},
  journal   = {Proceedings of the 30th International Technical Meeting of the Satellite Division of The Institute of Navigation (ION GNSS+ 2017)},
  publisher = {Instituite of Navigation},
  address   = {Washington},
  issn      = {2331-5911},
  doi       = {10.33012/2017.15343},
  pages     = {3368 -- 3374},
  year      = {2017},
  abstract  = {The ionospheric delay of global navigation satellite systems (GNSS) signals typically is compensated by adding a single correction value to the pseudorange measurement of a GNSS receiver. Yet, this neglects the dispersive nature of the ionosphere. In this context we analyze the ionospheric signal distortion beyond a constant delay. These effects become increasingly significant with the signal bandwidth and hence more important for new broadband navigation signals. Using measurements of the Galileo E5 signal, captured with a high gain antenna, we verify that the expected influence can indeed be observed and compensated. A new method to estimate the total electron content (TEC) from a single frequency high gain antenna measurement of a broadband GNSS signal is proposed and described in detail. The received signal is de facto unaffected by multi-path and interference because of the narrow aperture angle of the used antenna which should reduce the error source of the result in general. We would like to point out that such measurements are independent of code correlation, like in standard receiver applications. It is therefore also usable without knowledge of the signal coding. Results of the TEC estimation process are shown and discussed comparing to common TEC products like TEC maps and dual frequency receiver estimates.},
  language  = {en}
}
@misc{Metzler2017,
  author    = {Metzler, Ralf},
  title     = {Gaussianity Fair},
  series = {Biophysical journal},
  volume    = {112},
  journal   = {Biophysical journal},
  number    = {3},
  publisher = {Cell Press},
  address   = {Cambridge},
  issn      = {0006-3495},
  doi       = {10.1016/j.bpj.2016.12.019},
  pages     = {413 -- 415},
  year      = {2017},
  language  = {en}
}