A&A 591, A1 (2016) Astronomy DOI: 10.1051/0004-6361/201628093 & c ESO 2016 Astrophysics Morphological classification of local luminous infrared galaxies A. Psychogyios1, V. Charmandaris1; 2, T. Diaz- Santos3, L. Armus4, S. Haan5, J. Howell6, E. Le Floc’h7, S. M. Petty8, and A. S. Evans9; 10 1 Department of Physics, University of Crete, 71003 Heraklion, Greece e-mail:
[email protected] 2 IAASARS, National Observatory of Athens, 15236 Penteli, Greece 3 Núcleo de Astronomía de la Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército Libertador 441, Santiago, Chile 4 Spitzer Science Center, Calfornia Institute of Technology, MS 220-6, Pasadena, CA 91125, USA 5 CSIRO Astronomy and Space Science, ATNF, PO Box 76, Epping 1710, Australia 6 Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA 7 CEA Saclay, DSM/Irfu/Service d’Astrophysique, Orme des Merisiers, 91191 Gif-sur-Yvette Cedex, France 8 Department of Physics, Virginia Tech, Blacksburg, VA 24061, USA 9 Department of Astronomy, University of Virginia, Charlottesville, VA 22904, USA 10 National Radio Astronomy Observatory, Charlottesville, VA 22903, USA Received 8 January 2016 / Accepted 22 February 2016 ABSTRACT We present analysis of the morphological classification of 89 luminous infrared galaxies (LIRGs) from the Great Observatories All-sky LIRG Survey (GOALS) sample, using non-parametric coefficients and compare their morphology as a function of wavelength. We rely on images that were obtained in the optical (B- and I-band) as well as in the infrared (H-band and 5.8 µm). Our classification is based on the calculation of Gini and the second order of light (M20) non-parametric coefficients, which we explore as a function of stellar mass (M?), infrared luminosity (LIR), and star formation rate (SFR).