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Table 1.

Characteristics of DP galaxy sample.

ID SDSS designation z log(M*/M) SFR F150 MHz F1.4 GHz F3 GHz D25 i

(M yr−1) (mJy) (mJy) (mJy) (arcsec) (°)
DP-1a J153457.21+233013.3 0.0181 10.9 4.7 316.1 242.8 90.8
DP-2 J143117.98+075640.7 0.0269 11.0 7.7 5.8 3.1 65.8 66
DP-3 J142129.76+050423.6 0.0271 10.5 3.9 5.4 2.8 82.2 61
DP-4 J130702.99+130429.3 0.0274 10.5 3.5 5.0 2.3 61.6 58
DP-5 J141721.07+265126.8 0.0367 11.1 13.4 21.0 10.6 60.9
DP-6 J141916.59+261755.0 0.0368 11.1 7.4 9.7 8.1 59.7 50
DP-7 J160457.92+140815.3 0.0372 10.5 5.8 2.6 1.8 43.5 51
DP-8 J143713.73+143954.5 0.0379 10.9 10.1 9.1 5.4 25.2
DP-9 J141238.95+273740.7 0.0386 10.7 9.3 2.7 1.6 44.6 64
DP-10 J090007.20+600458.1 0.0390 11.0 43.5 8.5 4.8 2.9 38.5 52
DP-11 J132357.46+120233.3 0.0390 11.0 7.3 4.1 41.4 56
DP-12 J135309.67+143920.9 0.0405 11.2 7.4 18.0 3.9 47.0
DP-13b J020359.16+141837.3 0.0427 10.9 12.3 3.3 47.4 62
DP-14 J105716.67+283230.0 0.0457 10.9 10.4 8.4 1.6 1.8 43.7 56
DP-15 J113507.51+295327.7 0.0462 11.0 7.2 15.2 3.3 2.8 49.6 -
DP-16 J145415.59+254121.3 0.0479 10.8 24.8 3.3 1.9 25.3 48
DP-17b J091954.54+325559.8 0.0490 10.4 9.1 36.4 22.3 7.8 65.8
DP-18 J094142.69+283555.6 0.0538 11.1 7.5 10.7 2.8 2.0 45.2 58
DP-19c J233455.24+141731.1 0.0621 11.0 21.5 1.7 27.5 -
DP-20 J120854.47+472833.3 0.0677 10.7 17.0 7.2 2.4 19.6 36
DP-21 J134316.22+524742.5 0.0690 11.1 36.7 6.0 5.1 2.8 27.1 46
DP-22 J110428.21+560131.4 0.0702 11.0 10.5 15.8 4.7 2.6 33.1 42
DP-23 J110746.31+552633.3 0.0715 10.9 25.2 6.9 2.9 1.2 25.2
DP-24d J121346.08+024841.5 0.0731 10.6 17.5 24.6 17.0 4.5
DP-25d J102142.79+130656.1 0.0763 11.1 19.8 16.4 7.1 19.4
DP-26 J120437.97+525717.2 0.0815 10.9 22.4 10.4 5.2 1.4 31.0
DP-27c J221938.11+134213.9 0.0835 11.1 11.7 33.4
DP-28 J114325.16+505154.7 0.0844 11.0 28.0 10.1 4.0 2.1 22.6 39
DP-29 J131943.32+515255.8 0.0902 11.1 18.5 18.8 4.1 2.2 23.2 61
DP-30 J114050.50+561335.3 0.1065 10.8 43.7 6.9 1.1 19.3
DP-31d J135609.99+290535.1 0.1087 11.2 55.8 13.1 10.7 5.2 20.1
DP-32 J150439.86+501100.4 0.1124 10.8 15.2 7.8 1.5 15.0 45
DP-33 J150911.71+482041.2 0.1194 10.8 12.7 5.6 1.9 18.2 40
DP-34 J124406.54+503940.3 0.1211 10.8 23.7 8.4 2.0 13.2
DP-35 J130704.53+485845.5 0.1230 11.2 80.6 8.7 1.7 1.2 13.8 39
DP-36 J130847.69+504259.8 0.1244 11.0 35.6 8.7 3.5 14.6 29
DP-37 J143616.57+554822.0 0.1400 11.1 63.8 11.5 2.1 1.2 12.2
DP-38 J135705.89+523532.3 0.1437 11.1 36.5 5.4 2.8 1.0 19.0
DP-39 J113703.72+504420.7 0.1601 10.8 47.1 4.8 1.0 15.3 61
DP-40 J141803.61+534104.0 0.1638 11.1 65.9 10.9 2.2 1.0 14.1 39
DP-41c J100518.63+052544.2 0.1657 10.8 47.1 9.8
DP-42c J105527.19+064015.0 0.1731 11.0 44.1 11.9
DP-43c J091426.24+102409.6 0.1762 11.5 61.5 1.1 9.8
DP-44c J114649.18+243647.7 0.1767 11.1 106.1 6.7
DP-45c J134322.28+181114.1 0.1781 11.3 67.7 10.0
DP-46 J144017.35+563503.7 0.1801 11.4 19.3 5.3 1.6 19.3 21
DP-47c J223528.64+135812.7 0.1830 11.4 88.2 0.0 15.7
DP-48 J110333.10+475932.7 0.1906 11.0 21.1 6.5 1.4 9.9 42
DP-49c J002353.97+155947.9 0.1918 11.3 54.6 13.6
DP-50 J143211.77+495535.8 0.1938 10.7 11.4 3.1 1.5 9.8
DP-51c J092831.94+252313.9 0.2830 11.2 25.4 14.8
DP-52c J132047.14+160643.7 0.3124 11.5 64.9 10.2

Notes. DP emission-line galaxy sample consisting of 52 galaxies, observed in CO and lying more than 0.3 dex above the MS. We conducted CO observations for 35 galaxies and mark observations from the literature for the remaining 17. We note galaxies taken from Solomon et al. (1997) with the footnote a, from Saintonge et al. (2017) with b, from Bauermeister et al. (2013) with c, and from Chung et al. (2009) with d. We show the SDSS designation, redshift, stellar mass (Kauffmann et al. 2003), and SFR (Brinchmann et al. 2004). Radio fluxes at 150 MHz are taken from Shimwell et al. (2019), those at 1.4 GHz are taken from White et al. (1997), and those at 3 GHz are taken from Lacy et al. (2020). D25 is the optical diameter at the 25 mag isophote taken from the NASA/IPAC Extra galactic Database (NED) (https://ned.ipac.caltech.edu/). We used the radii computed from the SDSS r-band observation or, if available, from a photometric B-band observation. We further present the galaxy inclination calculated from a 2D Sérsic profile fit, as described in detail in Sect. 3.2.2.

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