Table 2: The derived properties of the combined galaxies.
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17)
mass s2 ratio ne (cm-3) o2 ratio $T_{{\rm e}}$([O  II]) (K) $T_{{\rm e}}$([O  III]) (K) OH $_{T_{\rm e}}$ AV logR23 log O32 OH aR23 OH bR23 P OHP N2 OHN2 log( ${\rm N}\over {\rm O}$)
8.70 1.36 58.97 44.25 $\pm$ 0.95 11423 $\pm$ 153 12034 $\pm$ 219 8.05 $\pm$ 0.03 0.18 0.77 0.08 8.48 8.63 0.54 8.39 -1.08 8.28 -1.29
8.71 1.38 39.36 51.32 $\pm$ 2.76 10641 $\pm$ 341 10916 $\pm$ 487 8.23 $\pm$ 0.07 0.42 0.82 -0.05 8.34 8.58 0.47 8.29 -0.94 8.36 -1.31
8.81 1.43 3.58 47.38 $\pm$ 2.39 11491 $\pm$ 370 12130 $\pm$ 528 8.06 $\pm$ 0.07 0.38 0.78 -0.11 8.47 8.63 0.44 8.31 -0.94 8.36 -1.24
8.91 1.41 14.06 63.38 $\pm$ 0.29 9703 $\pm$ 22 9576 $\pm$ 32 8.35 $\pm$ 0.01 0.35 0.75 -0.21 8.56 8.67 0.38 8.32 -0.88 8.40 -1.31
9.01 1.40 24.83 62.37 $\pm$ 2.23 9701 $\pm$ 182 9572 $\pm$ 260 8.36 $\pm$ 0.05 0.39 0.75 -0.22 8.54 8.66 0.38 8.31 -0.86 8.41 -1.29
9.11 1.37 50.84 64.91 $\pm$ 2.75 9328 $\pm$ 202 9039 $\pm$ 289 8.41 $\pm$ 0.06 0.36 0.72 -0.24 8.62 8.70 0.36 8.34 -0.80 8.44 -1.25
9.21 1.39 33.32 69.04 $\pm$ 0.80 9168 $\pm$ 51 8812 $\pm$ 72 8.44 $\pm$ 0.02 0.41 0.71 -0.28 8.64 8.71 0.34 8.34 -0.77 8.46 -1.23
9.31 1.38 40.24 69.45 $\pm$ 0.39 9096 $\pm$ 24 8709 $\pm$ 34 8.43 $\pm$ 0.01 0.40 0.68 -0.31 8.70 8.75 0.33 8.36 -0.74 8.48 -1.19
9.405 1.36 57.15 63.03 $\pm$ 0.50 9422 $\pm$ 38 9174 $\pm$ 54 8.35 $\pm$ 0.01 0.47 0.66 -0.36 8.73 8.77 0.30 8.37 -0.72 8.49 -1.14
9.4505 1.39 37.63 73.34 $\pm$ 1.29 8883 $\pm$ 74 8404 $\pm$ 105 8.48 $\pm$ 0.02 0.53 0.68 -0.39 8.71 8.75 0.29 8.35 -0.69 8.50 -1.18
9.505 1.42 13.25 92.13 $\pm$ 0.91 8169 $\pm$ 34 7384 $\pm$ 49 8.67 $\pm$ 0.01 0.59 0.67 -0.39 8.73 8.77 0.29 8.36 -0.70 8.50 -1.25
9.5505 1.42 10.81 76.59 $\pm$ 2.96 8878 $\pm$ 164 8397 $\pm$ 235 8.47 $\pm$ 0.05 0.59 0.66 -0.40 8.73 8.77 0.29 8.36 -0.67 8.52 -1.14
9.605 1.40 29.90 75.72 $\pm$ 0.09 8801 $\pm$ 5 8287 $\pm$ 7 8.46 $\pm$ 0.00 0.54 0.63 -0.42 8.80 8.81 0.27 8.40 -0.63 8.54 -1.09
9.6505 1.38 41.11 79.67 $\pm$ 0.77 8534 $\pm$ 37 7906 $\pm$ 53 8.52 $\pm$ 0.01 0.67 0.62 -0.46 8.81 8.82 0.26 8.40 -0.63 8.54 -1.11
9.705 1.39 32.46 83.36 $\pm$ 1.99 8414 $\pm$ 90 7735 $\pm$ 128 8.55 $\pm$ 0.03 0.66 0.62 -0.45 8.81 8.82 0.26 8.40 -0.62 8.55 -1.11
9.7505 1.38 39.36 77.80 $\pm$ 1.99 8636 $\pm$ 102 8051 $\pm$ 146 8.47 $\pm$ 0.03 0.68 0.59 -0.50 8.84 8.84 0.24 8.42 -0.59 8.57 -1.04
9.805 1.38 39.36 76.95 $\pm$ 1.50 8679 $\pm$ 75 8112 $\pm$ 108 8.42 $\pm$ 0.03 0.74 0.55 -0.50 8.89 8.88 0.24 8.45 -0.58 8.57 -0.99
9.8505 1.38 42.86 89.25 $\pm$ 1.48 8114 $\pm$ 58 7305 $\pm$ 83 8.59 $\pm$ 0.02 0.77 0.57 -0.54 8.88 8.87 0.22 8.43 -0.56 8.58 -1.05
9.905 1.39 32.46 69.83 $\pm$ 2.42 9124 $\pm$ 156 8748 $\pm$ 224 8.29 $\pm$ 0.05 0.80 0.53 -0.54 8.91 8.89 0.23 8.47 -0.56 8.58 -0.91
9.9505 1.36 64.48 66.14 $\pm$ 2.55 9156 $\pm$ 177 8794 $\pm$ 253 8.28 $\pm$ 0.05 0.83 0.53 -0.55 8.92 8.90 0.22 8.47 -0.53 8.60 -0.88
10.005 1.37 54.43 88.12 $\pm$ 1.56 8096 $\pm$ 62 7281 $\pm$ 88 8.55 $\pm$ 0.02 0.81 0.52 -0.56 8.92 8.91 0.21 8.48 -0.52 8.60 -0.97
10.0505 1.38 40.24 98.15 $\pm$ 6.10 7813 $\pm$ 210 6876 $\pm$ 299 8.63 $\pm$ 0.09 0.87 0.51 -0.56 8.93 8.92 0.22 8.49 -0.50 8.61 -0.97
10.11 1.34 76.67 76.26 $\pm$ 1.60 8563 $\pm$ 82 7947 $\pm$ 118 8.39 $\pm$ 0.03 0.94 0.49 -0.58 8.95 8.93 0.21 8.50 -0.49 8.62 -0.87
10.21 1.34 75.72 101.92 $\pm$ 2.07 7531 $\pm$ 61 6472 $\pm$ 88 8.70 $\pm$ 0.03 1.06 0.48 -0.61 8.95 8.94 0.20 8.50 -0.47 8.63 -0.96
10.31 1.32 97.12 97.23 $\pm$ 2.54 7579 $\pm$ 77 6542 $\pm$ 110 8.66 $\pm$ 0.04 1.08 0.46 -0.61 8.97 8.96 0.20 8.52 -0.46 8.64 -0.92
10.41 1.33 86.29 81.74 $\pm$ 1.54 8197 $\pm$ 68 7424 $\pm$ 97 8.45 $\pm$ 0.03 1.15 0.45 -0.60 8.97 8.96 0.20 8.53 -0.44 8.65 -0.81
10.51 1.36 57.15 110.86 $\pm$ 1.85 7368 $\pm$ 48 6241 $\pm$ 69 8.76 $\pm$ 0.02 1.22 0.48 -0.60 8.95 8.94 0.20 8.50 -0.44 8.65 -0.95
Notes: Columns (1)-(17) consequently refer to: (1) the mass of the center value of the bin; (2) the ratio of [S  II] $\lambda6717$/[S  II] $\lambda6731$; (3) the electron density; (4) the ratio of [O  II] $\lambda\lambda7320,~7330$/[O  II] $\lambda3727$; (5) the election temperature in low ionization region; (6) the election temperature in high ionization region; (7) the oxygen abundances $12+\log($O/H) derived from election temprature; (8) the dust extinction AV estimated from H$\alpha $/H$\beta $; (9) logarithm of the ratio of ([O  II] $\lambda3727+[$O  III] $\lambda\lambda4959,~5007$)/H$\beta $; (10) logarithm of the ratio of [O  III] $\lambda\lambda4959,~5007$/[O  II] $\lambda3727$; (11) the $12+\log($O/H) abundances obtained by using the R23 calibrations derived from DR4 (Eq. (2)); (12) the $12+\log($O/H) abundances obtained by using the R23 calibrations derived from DR2 (T04); (13) the P parameter [O  III] $\lambda\lambda4959,~5007$)/ ([O  II] $\lambda3727$+[O  III] $\lambda\lambda4959,~5007$); (14) the $12+\log($O/H) abundances obtained by using the P-method calibration of P01; (15) the N2 index (=log([N  II] $\lambda6583$/H$\alpha $)); (16) the $12+\log($O/H) abundances obtained by using the N2 calibration of PP04; (17) the log(N/O) abundance ratios derived from election temperature method.

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