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Table I.2.

Continuation of linear model parameters for each galaxy.

1 12 13 14 15 16 17 18 19
Galaxy R25 ∇(O/H) (O/H)0 ∇(O/H) (O/H)0 ∇(O/H)1 ∇(O/H)2 Breakpoint
no DIG no DIG with DIG with DIG no DIG no DIG no DIG
[arcsec] [dex/Reff] [dex/Reff] [dex/Reff] [dex/Reff] [Reff,  NUV]
DDO 53
DDO 154 57.56 −0.12 ± 0.27 7.83 ± 0.26 −0.12 ± 0.27 7.83 ± 0.26
Holmberg I 97.70 0.64 ± 0.27 7.38 ± 0.18 0.28 ± 0.25 7.60 ± 0.17
M81 DwB
Holmberg II 224.47 −0.31 ± 0.08 7.79 ± 0.03 −0.30 ± 0.06 7.80 ± 0.03
NGC 2366 −0.05 ± 0.08 −0.55 ± 0.03 0.95 ± 0.04
NGC 4214 206.27 −0.089 ± 0.009 8.214 ± 0.003 −0.10 ± 0.01 8.202 ± 0.004
NGC 1569 119.43 −0.08 ± 0.02 8.153 ± 0.006 −0.05 ± 0.02 8.145 ± 0.008
IC 2574 386.75 −0.42 ± 0.06 8.08 ± 0.04 −0.40 ± 0.06 8.07 ± 0.04
NGC 4449 137.51 −0.071 ± 0.003 8.260 ± 0.003 −0.062 ± 0.004 8.254 ± 0.003
NGC 2976 217.72 −0.13 ± 0.02 8.366 ± 0.006 −0.22 ± 0.02 8.384 ± 0.008
NGC 3077 162.84 −0.24 ± 0.03 8.464 ± 0.007 −0.39 ± 0.03 8.488 ± 0.009
NGC 2403 470.54 −0.295 ± 0.009 8.442 ± 0.003 −0.339 ± 0.009 8.442 ± 0.003
NGC 925 318.37 −0.203 ± 0.009 8.35 ± 0.004 −0.202 ± 0.009 8.35 ± 0.004
NGC 3198 194.31 −0.298 ± 0.009 8.603 ± 0.004 −0.306 ± 0.009 8.605 ± 0.004
NGC 4826 −0.03 ± 0.09 −0.14 ± 0.36 1.63 ± 0.09
NGC 4736 232.60 −0.082 ± 0.013 8.582 ± 0.004 −0.262 ± 0.020 8.617 ± 0.007
NGC 3184 221.13 −0.165 ± 0.009 8.575 ± 0.004 −0.171 ± 0.009 8.575 ± 0.004
NGC 5457 719.65 −0.523 ± 0.009 8.596 ± 0.002 −0.602 ± 0.01 8.602 ± 0.002
NGC 6946 342.61 −0.172 ± 0.004 8.598 ± 0.002 −0.175 ± 0.004 8.599 ± 0.002 −0.115 ± 0.002 0.12 ± 0.03 1.13 ± 0.02
NGC 5055 355.35 −0.074 ± 0.008 8.585 ± 0.002 −0.088 ± 0.007 8.588 ± 0.002 −0.010 ± 0.008 −0.055 ± 0.008 0.65 ± 0.06
NGC 5194 232.05 −0.029 ± 0.002 8.607 ± 0.002 −0.035 ± 0.003 8.609 ± 0.002
NGC 3521 249.6 −0.112 ± 0.005 8.633 ± 0.002 −0.14 ± 0.005 8.643 ± 0.002 −0.043 ± 0.003 −0.14 ± 0.02 1.70 ± 0.10
NGC 2841 207.73 −0.074 ± 0.013 8.630 ± 0.008 −0.124 ± 0.014 8.655 ± 0.009
NGC 7331 275.02 −0.149 ± 0.007 8.614 ± 0.005 −0.156 ± 0.008 8.616 ± 0.005

Notes. Each column shows information as follows: 1) galaxy designation; 12) isophotal radius; 13) and 14) linear model parameters and errors without DIG-dominated fibres with isophotal radius normalisation; 15) and 16) linear model parameters and errors with all fibres with isophotal radius normalisation. Each linear model was fitted using a Bayesian MCMC routine. Columns 17), 18), 19) respectively show the slopes and breakpoint for the piecewise linear fits for the NUV-band normalisation for those galaxies where a change in the tendency of their metallicity distribution was spotted.

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