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Table A.1.

Main properties of the galaxy sample.

Galaxy R.A.(J2000) Dec.(J2000) z D Re ellipticity PA i log(M⋆) log(MH I) yeff SFR 12 + log(O/H) ∇r [O/H]
- degrees degrees - Mpc kpc - degrees degrees log(M⊙) log(M⊙) - log(M⊙yr−1) - dex/Re
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)
AGC191702 137.15226 5.29078 0.001994 12.21 0.78 0 0 0 7.12 7.74 −2.29 −2.15 7.81 0.115±0.085
AGC193816 140.36375 7.36639 0.004633 21.47 1.18 0 0 0 8.55 8.33 −2.43 −1.45 8.36 −0.057±0.036
CGCG007-025 146.0078 −0.64227 0.004810 23.05 1.05 0.501 159.7 62 8.1 - - −0.74 7.68 0.019±0.01
CGCG035-007 143.68627 6.42563 0.0018 4.92 0.41 0.24 63 41 7.6 7.69 −2.62 −2.85 7.96 0.061±0.022
ESO115-021 39.41943 −61.3517 0.0017 4.99 1.06 0.72 41.0 74 8.2 8.66 −2.46 −2.48 7.82 −0.12±0.024
ESO119-016 72.87165 −61.65094 0.0032 10.08 2.62 0.48 26 58 8.4 7.9 −2.83 −2.14 8.05 0.088±0.06
ESO158-003 71.57227 −57.34378 0.0040 10.20 1.48 0.14 0 30 8.76 6.47 −2.99 −1.22 8.24 −0.025±0.005
ESO184-82 293.76842 −52.84389 0.008685 28.576 1.79 0.305 137.6 47 8.95 8.9 −2.42 −0.71 8.23 −0.102±0.002
ESO483-013 63.17129 −23.15887 0.0027 10.68 1.36 0.28 125.0 46 8.81 7.62 −3.06 −1.1 8.11 −0.058±0.005
ESO486-021 75.83203 −25.42293 0.0029 9.11 0.64 0.14 90 30 8.26 8.38 −2.67 −1.69 7.88 −0.072±0.003
FCC090 52.78442 −36.29014 0.006048 19.23 1.1 0.256 154.5 43 8.95 7.77 −2.78 −1.13 8.43 −0.094±0.007
FCC113 53.27854 −34.80811 0.004631 16.14 1.6 0.213 164.9 39 8.16 8.16 −2.52 −2.13 8.13 0.063±0.007
FCC119 53.39101 −33.57332 0.004583 20.14 1.45 0.15 47.7 32 8.8 - - −2.61 8.55 0.038±0.077
FCC263 55.38583 −34.88833 0.005751 12.59 1.06 0.54 3.6 65 8.71 8.22 −2.65 −1.24 8.29 −0.035±0.002
FCC285 55.75914 −36.27337 0.002955 9.16 1.67 0.39 105 54 8.11 8.15 −2.59 −1.85 8.02 −0.151±0.005
FCC306 56.43916 −36.34653 0.002955 9.74 0.39 0.287 41.1 46 7.61 8.03 −2.33 −2.42 7.97 −0.011±0.007
FCC308 56.47854 −36.35697 0.004995 8.68 1.47 0.643 6.4 72 8.34 8.38 −2.19 −2.07 8.43 −0.026±0.003
IC1959 53.30246 −50.41425 0.002131 6.85 1.27 0.732 149.6 80 8.16 8.37 −2.54 −1.69 7.93 −0.054±0.001
IC2828 171.79559 8.73105 0.003451 14.20 0.7 0.539 60.5 65 8.37 7.83 −2.87 −1.24 8.03 −0.011±0.001
IC3476 188.17452 14.05044 −0.00053 13.80 1.97 0.312 27.6 48 8.74 8.42 −2.35 −0.74 8.42 −0.085±0.001
IC4247 201.68539 −30.3628 0.0014 4.97 0.47 0.40 153.0 53 7.74 7.3 −3.04 −2.75 7.91 0.029±0.043
IC4870 294.40667 −65.81183 0.00292 8.51 1.04 0.452 131.4 59 8.49 8.76 −2.56 −1.07 7.84 0.066±0.003
MCG-03-34-002 196.98617 −16.6892 0.0031 7.90 0.69 0.38 140.0 52 8.41 7.32 −3.25 −2.11 8.0 −0.074±0.016
NGC0059 3.85488 −21.4445 0.0013 5.30 0.74 0.30 122.0 47 8.52 6.95 −3.33 −1.76 8.0 0.037±0.018
NGC853 32.92161 −9.30599 0.005014 21.00 2.24 0.450 70.9 59 9.25 8.79 −2.57 −0.51 8.33 −0.103±0.002
NGC1311 50.029 −52.18553 0.0019 5.45 0.87 0.53 36 62 8.22 7.96 −2.87 −2.0 7.96 0.076±0.011
NGC1522 61.533 −52.66842 0.0030 9.54 0.84 0.34 37 49 8.53 - - −1.47 8.05 −0.148±0.015
NGC1705 73.55625 −53.36106 0.00211 5.10 0.43 0.286 48.6 46 8.24 8.02 −2.88 −1.52 7.89 −0.007±0.001
NGC1796 75.67729 −61.14006 0.003381 10.60 1.31 0.526 101.1 64 9.14 8.33 −2.35 −0.99 8.76 −0.09±0.001
NGC1800 76.60717 −31.95422 0.00272 8.01 0.83 0.524 112.2 64 8.67 8.27 −2.77 −1.3 8.13 −0.032±0.002
NGC2915 141.54804 −76.62633 0.00156 4.29 0.32 0.422 125 56 8.2 8.28 −2.6 −1.77 7.98 −0.039±0.001
NGC3125 151.63905 −29.93486 0.003712 15.00 0.82 0.385 111.8 54 9.17 8.62 −2.72 −0.18 8.11 −0.009±0.001
NGC3593 168.65417 12.81767 0.002075 8.95 2.02 0.591 87.5 69 9.64 8.33 −2.33 −0.15 8.82 −0.145±0.002
NGC4383 186.35635 16.47013 0.005704 17.94 1.24 0.427 26.4 57 9.38 9.44 −2.18 −0.32 8.4 −0.112±0.001
NGC4592 189.82807 −0.53201 0.003566 11.64 3.04 0.410 88.2 55 8.88 9.74 −1.75 −0.88 8.14 −0.214±0.002
NGC4809A 193.71276 2.65409 0.002943 21.90 2.98 0.677 66.1 75 8.96 - - −1.05 7.97 −0.021±0.003
NGC4809B 193.71276 2.65409 0.002943 21.90 2.56 0.577 160.1 68 9.01 - - −1.08 7.9 −0.005±0.002
NGC5253 204.98318 −31.64011 0.001358 3.55 0.7 0.525 26.9 64 8.65 7.97 −2.86 −0.81 8.05 −0.08±0.001
PGC132213 330.78995 −12.37180 0.002750 9.31 0.32 0.296 20.3 46 7.12 - - −2.42 7.74 0.052±0.025
UGC685 16.8435 16.68457 0.0005 4.70 0.83 0.18 122 35 7.95 7.84 −3.03 −2.18 7.7 0.095±0.008
UGC695 16.9435 1.06367 0.0022 10.68 1.5 0.16 0 32 8.04 7.9 −2.99 −1.87 7.75 0.097±0.029
UGC891 20.32915 12.41251 0.0021 11.10 1.38 0.39 42 52 8.39 8.51 −2.32 −2.64 8.24 −0.079±0.127
UGC1056 22.19739 16.6884 0.0020 10.57 1.06 0.06 0 20 8.32 7.77 −3.13 −1.72 7.84 −0.018±0.005
UGC3755 108.465 10.52194 0.00105 6.67 1.21 0.500 160.3 62 8.05 7.94 −2.89 −2.1 7.84 0.075±0.006
UGC5288 147.82105 7.82783 0.0019 11.40 1.48 0.14 151.0 30 8.14 8.28 −2.53 −1.36 7.97 −0.093±0.008
UGC5889 161.84292 14.06944 0.001912 6.89 1.14 0.093 57.9 26 8.27 8.14 −2.52 −2.65 8.24 −0.145±0.014
UGC5923 162.28139 6.91742 0.0024 7.33 0.31 0.38 173.0 52 8.24 7.82 −2.66 −1.62 8.23 0.035±0.026
UGC8041 193.80273 0.11665 0.004416 14.52 3.43 0.223 173.7 40 9.01 9.03 −2.09 −1.22 8.55 −0.203±0.005
UGCA116 88.9275 3.39222 0.002682 14.43 1.06 0.38 131.6 53 9.23 8.92 −2.64 0.11 8.02 0.008±0.002
UGCA193 150.65047 −6.01371 0.0022 9.70 1.28 0.73 14 77 8.28 8.19 −2.57 −1.97 8.15 −0.01±0.005
UGCA442 355.94034 −31.9567 0.0009 4.27 1.14 0.52 43 62 7.86 8.22 −2.44 −2.41 7.92 0.041±0.018
UM461 177.88896 −2.37276 0.003465 19.54 0.63 0.32 90 48 7.71 8.54 −2.3 −1.17 7.58 0.078±0.046
UM462 178.15497 −2.46942 0.003469 19.18 1.07 0.102 60.1 27 8.68 8.59 −2.55 −0.63 8.06 0.036±0.008
VCC0415 185.10538 6.90836 0.008539 24.20 2.08 0.240 63.8 42 8.76 8.37 −2.61 −1.19 8.27 −0.075±0.004
VCC2037 191.56375 10.20556 0.003809 9.63 1.49 0.563 9.6 67 7.56 7.18 −2.98 −2.84 7.93 0.194±0.031

Notes. Col(1):Galaxy name. (2)-(4): Celestial coordinates in J2000 and redshift of galaxy from NED Database. (5) galaxy distance from several sources: HyperLeda Database, Marasco et al. (2023), Kourkchi & Tully (2017) or, when not available, calculated from redshift. (6)-(9): the morphological properties as determined in this work. The zero value of ellipticity and PA means that the galaxies are too irregular or faint to be measured correctly in our program. (10) Stellar mass. (11) HI mass. Six galaxies in our sample do not have HI observations or detections are left with a single bar. (12) Effective Yield of Oxygen. (13) Star formation rate. (14) Metallicity derived from integrated MUSE spectra, using N2S2Hα method (Dopita et al. 2016). (15): Radial gradient of gas-phase metallicities. Note: NGC4809A and NGC4809B are two galaxies in the early stage of interaction in a single MUSE exposure, and we divided them into two single galaxies to measure their properties respectively.

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