RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S<sup>4</sup>G IRAC 3.6 AND 4.5 μm IMAGES. I. CORRECTING FOR CONTAMINATION BY POLYCYCLIC AROMATIC HYDROCARBONS, HOT DUST, AND INTERMEDIATE-AGE STARS

Sharon E. Meidt(Max Planck Institute for Astronomy), S. Comerón(University of Oulu), J. H. Knapen(University of Hertfordshire), Dennis Zaritsky(University of Arizona), H. Salo(University of Oulu), A. Gil de Paz(Universidad Complutense de Madrid), Trisha Mizusawa(Florida Institute of Technology), Bruce G. Elmegreen(IBM (United States)), Barry F. Madore(Carnegie Institution for Science), Eva Schinnerer(Max Planck Institute for Astronomy), A. Bosma(Centre National de la Recherche Scientifique), J. L. Hinz, D. M. Elmegreen(Vassar College), Luis C. Ho(Peking University), Dimitri A. Gadotti, E. Athanassoula(Laboratoire d’Astrophysique de Marseille), 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), Mark Seibert(Carnegie Observatories), Juan-Carlos Muñoz-Mateos(European Southern Observatory), E. Laurikainen(University of Turku)
The Astrophysical Journal
December 7, 2011
Cited by 200


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