Mid-infrared galaxy morphology from the Spitzer Survey of Stellar Structure in Galaxies (s4g): The imprint of the de Vaucouleurs revised hubble-sandage classification system at 3.6μm
Ronald J. Buta, Kartik Sheth, Michael Regan, Joannah L. Hinz, Armando Gil De Paz, Karin Menéndez-Delmestre, Juan Carlos Munoz-Mateos, Mark Seibert, Eija Laurikainen, Heikki Salo, Dimitri A. Gadotti, E. Athanassoula, Albert Bosma, Johan H. Knapen, Luis C. Ho, Barry F. Madore, Debra M. Elmegreen, Karen L. Masters, Sebastien Comerón, Manuel AravenaTaehyun Kim
Dive into the research topics of 'Mid-infrared galaxy morphology from the Spitzer Survey of Stellar Structure in Galaxies (s4g): The imprint of the de Vaucouleurs revised hubble-sandage classification system at 3.6μm'. Together they form a unique fingerprint.