RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S<sup>4</sup>G IRAC 3.6 AND 4.5 μm IMAGES. II. THE CONVERSION FROM LIGHT TO MASS
Sharon E. Meidt(Max Planck Institute for Astronomy), Trisha Mizusawa(Florida Institute of Technology), J. H. Knapen(University of Hertfordshire), Dennis Zaritsky(University of Arizona), H. Salo(University of Oulu), S. Comerón(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), Mauricio Cisternas(Universidad de La Laguna), R. F. Peletier(University of Groningen), Miguel Querejeta(European Southern Observatory), 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), R. Buta(University of Alabama), Michael W. Regan(Space Telescope Science Institute), Taehyun Kim(Seoul National University), Ramin Skibba(University of Arizona), Juan-Carlos Muñoz-Mateos(European Southern Observatory), Mark Seibert(Carnegie Observatories), S. Erroz–Ferrer(Consejo Superior de Investigaciones Científicas), E. Laurikainen(University of Turku)
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