CO(1–0) and (2–1) emission lines of LARS galaxies obtained with the IRAM 30m telescope, shown on the T_MB scale in milli Kelvin. The beam sizes for the transitions are shown in Col. (1) on top of our HST Hα narrow band images: white: CO(1–0), and red: CO(2–1). CO(1–0) and CO(2–1) spectra are shown in Cols. (2) and (4) respectively. Single or double Gaussian fits were performed to calculate the line flux. They are shown as cyan solid lines. The residuals after subtraction of the fits from the data are given in Cols. (3) and (5).