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Table 2.

CO(2–1) observations of the sample.

Object
θmaj × θmin θm PA Sensitivity Project Mosaics MRS SINFONI
Galaxy name IRAS name [″] [″] [″, pc] [°] [mJy beam−1] PI [″]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
ESO 297-G011 F01341−3735 0.21 × 0.16 0.19, 67 −72 0.53 MPS 9.4
NGC 1614 F04315−0840 0.22 × 0.15 0.19, 62 −74 0.43 MPS 10.8
NGC 2369 F07160−6215 0.24 × 0.21 0.22, 53 88 0.51 MPS 8.8
NGC 3110 F10015−0614 0.26 × 0.21 0.23, 89 −83 0.35 MPS 8.8
NGC 3256 F10257−4339 0.23 × 0.21 0.22, 48 63 0.43 KS 5.4
ESO 320-G030 F11506−3851 0.30 × 0.24 0.27, 68 63 0.89 LC1 8.7
MCG-02-33-098 W F12596−1529 0.23 × 0.17 0.20, 73 89 0.48 MPS 9.4
MCG-02-33-098 E F12596−1529 0.23 × 0.17 0.20, 72 89 0.48 MPS 9.4
NGC 5135 F13229−2934 0.31 × 0.22 0.26, 82 63 0.21 LC2 9.4
IC 4518 W F14544−4255 0.23 × 0.20 0.21, 75 −86 0.46 MPS 10.3
IC 4518 E F14544−4255 0.23 × 0.20 0.21, 73 −87 0.47 MPS 10.3
... F17138−1017 0.26 × 0.22 0.24, 87 −62 0.75 MPS 7.6
IC 4734 F18341−5732 0.25 × 0.21 0.23, 75 −73 0.77 TDS 2.7
NGC 7130 F21453−3511 0.36 × 0.29 0.32, 105 69 0.29 MPS 9.9
IC 5179 F22132−3705 0.40 × 0.34 0.37, 82 44 0.45 MPS 9.8
NGC 7469 F23007+0836 0.23 × 0.18 0.21, 65 −39 0.29 TDS 2.8

Notes. Column (1): Galaxy name. Column (2): IRAS denomination from Sanders et al. (2003). Column (3): Major (θmaj) and minor (θmin) FWHM beam sizes. Column (4): Mean FWHM beam size (θm) in arcseconds and parsecs. Column (5): Position angle (PA) in degrees. Column (6): 1σ line sensitivity of the CO(2–1) observations. Column (7): Principal investigator of the ALMA project: MPS: Miguel Pereira-Santaella (2017.1.00255.S), KS: Kazimierz Sliwa (2015.1.00714.S), LC1: Luis Colina (2013.1.00271.S), LC2: Luis Colina (2013.1.00243.S), TDS: Tanio Díaz-Santos (2017.1.00395.S). Column (8): ✓galaxies with mosaics data. Column (9): Maximum recoverable scales. Column (10): ✓galaxies with SINFONI data.

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