Now showing items 1-4 of 4

    • Dunne, L.; Gomez, H. L.; da Cunha, E.; Charlot, S.; Dye, S.; Eales, S.; Maddox, S. J.; Rowlands, K.; Smith, D. J.B.; Auld, R.; Baes, M.; Bonfield, D. G.; Bourne, N.; Buttiglione, S.; Cava, A.; Clements, D. L.; Coppin, K. E.K.; Cooray, A.; Dariush, A.; de Zotti, G.; Driver, S (2011)
      We present the first direct and unbiased measurement of the evolution of the dust mass function of galaxies over the past 5 billion years of cosmic history using data from the Science Demonstration Phase of the ...
    • 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 ...
    • 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 ...
    • Molina, J.; Ibar, Edo; Villanueva, V.; Escala, A.; Cheng, C.; Baes, M.; Messias, H.; Yang, C.; Bauer, F. E.; van der Werf,; Leiton, R.; Aravena, M.; Swinbank, A. M.; Michalowski, M. J.; Muñoz-Arancibia, A. M.; Orellana, G.; Hughes, T. M.; Farrah, D.; De Zotti, G.; Lara-Lóp (Oxford University Press, 2019)
      © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.We present Atacama Large Millimeter/submillimeter Array (ALMA) resolved observations of molecular gas in galaxies up ...