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 MASSSharon E. Meidt, Trisha Mizusawa, A. Gil de Paz et al.|The Astrophysical Journal|2014Cited by 275
ARRAKIS: atlas of resonance rings as known in the S<sup>4</sup>GS. Comerón, Luis C. Ho, H. Salo et al.|Astronomy and Astrophysics|2013Cited by 124
THE BARYONIC TULLY-FISHER RELATIONSHIP FOR S<sup>4</sup>G GALAXIES AND THE “CONDENSED” BARYON FRACTION OF GALAXIESDennis Zaritsky, Benne W. Holwerda, H. M. Courtois et al.|The Astronomical Journal|2014Cited by 92
Morphology and environment of galaxies with disc breaks in the S4G and NIRS0SJarkko Laine, Kartik Sheth, E. Laurikainen et al.|Monthly Notices of the Royal Astronomical Society|2014Cited by 79
MORPHOLOGICAL PARAMETERS OF A<i>SPITZER</i>SURVEY OF STELLAR STRUCTURE IN GALAXIESBenne W. Holwerda, Nor Pirzkal, J. C. Muñoz-Mateos et al.|The Astrophysical Journal|2013Cited by 44