THE <i>SPITZER</i> SURVEY OF STELLAR STRUCTURE IN GALAXIES (S <sup>4</sup> G): PRECISE STELLAR MASS DISTRIBUTIONS FROM AUTOMATED DUST CORRECTION AT 3.6 <i>μ</i> m
Miguel Querejeta(European Southern Observatory), S. Comerón(University of Oulu), J. H. Knapen(University of Hertfordshire), Sharon E. Meidt(Max Planck Institute for Astronomy), Dennis Zaritsky(University of Arizona), H. Salo(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), Mauricio Cisternas(Universidad de La Laguna), R. F. Peletier(University of Groningen), Mark A. Norris(University of Leeds), Trisha Mizusawa(Florida Institute of Technology), Brent Groves(Australian National University), Eva Schinnerer(Max Planck Institute for Astronomy), A. Bosma(Centre National de la Recherche Scientifique), J. L. Hinz, Glenn van de Ven(Institute of Astronomy), Luis C. Ho(Peking University), Dimitri A. Gadotti, E. Athanassoula(Laboratoire d’Astrophysique de Marseille), Benne W. Holwerda, Karín Menéndez‐Delmestre(Universidade Federal do Rio de Janeiro), Jarkko Laine(University of Oulu), Kartik Sheth(National Radio Astronomy Observatory), Michael W. Regan(Space Telescope Science Institute), Taehyun Kim(Seoul National University), Santiago Erroz-Ferrer(Universidad de La Laguna), Mark Seibert(Carnegie Observatories), J. C. Muñoz-Mateos(European Southern Observatory), E. Laurikainen(University of Turku)
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