Browsing by Author "80857c9a-f79a-4196-8e4e-47851cb5b1f5"

Now showing items 1-3 of 3

    • Polarization in Monte Carlo radiative transfer and dust scattering polarization signatures of spiral galaxies 
      Peest, C.; Camps, P.; Stalevski, Marko; Baes, M.; Siebenmorgen, R. (EDP Sciences, 2017-05)
      Polarization is an important tool to further the understanding of interstellar dust and the sources behind it. In this paper we describe our implementation of polarization that is due to scattering of light by spherical ...
    • The EAGLE simulations of galaxy formation: Public release of halo and galaxy catalogues 
      McAlpine, S.; Helly, J. C.; Schaller, M.; Trayford, J. W.; Qu, Y.; Furlong, M.; Bower, R. G.; Crain, R. A,; Schaye, J.; Theuns, T.; Dalla Vecchia, C.; Frenk, C. S.; McCarthy, I. G.; Jenkins, A.; Rosas Guevara, Y.; White, S. D. M.; Baes, Maarten; Camps, P.; Lemson, G. (Elsevier, 2016)
      We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of cosmological hydrodynamical simulations of galaxy formation. These simulations were performed with an enhanced version of ...
    • The high-redshift SFR–M∗ relation is sensitive to the employed star formation rate and stellar mass indicators: ... 
      Katsianis, A.; González, V.; Barrientos, D.; Yang, X.; Lagos, C. D. P.; Schaye, J.; Camps, P.; Trcka, A.; Baes, M.; Stalevski, M.; Blanc, G. A.; Theuns, T. (Oxford University Press, 2020)
      There is a severe tension between the observed star formation rate (SFR)-stellar mass (M,) relations reported by different authors at z = En addition, the observations have not been successfully reproduced by state-of-the-art ...