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An ALMA view of star formation efficiency suppression in early type galaxies after gas rich minor mergers

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Table 1. Properties of our selected galaxies: source identifier, redshift, angular diameter distance, stellar mass, SFR, SFE, and conversion factor from arcsecto kpc
Table 2. Parameters for our ALMA observations: source identifier, date of observation, total observation time, amplitude calibrator, bandpass calibrator, phasecalibrator, beam size, and rms noise in 10 km s−1 channels of each source.
Figure 2. Images of the CO(1–0) data for all six galaxies. Left-hand panels: SDSS r-band image overlaid with ALMA CO(1–0) contours
Figure 3. Spectra of the CO(1–0) data for all six galaxies with our new ALMA data shown in black and previously obtained (lower resolution) IRAM datain red
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