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Table A.2

Derived spectroscopic parameters for galaxies observed at Loiano with red-channel grism.

HRS Mass gi Hα correction HαEW HαEW corr [NII](6583)EW rms WHAN
M mag count
(1) (2) (3) (4) (5) (6) (7) (8) (9)
9 10.08 1.081 1.82 1.69 3.51 3.12 0.04 wAGN
32 9.46 1.044 1.91 −1.28 0.63 0.85 0.02 RET
38 9.1 0.572 2.25 13.1 15.35 4.00 0.16 HII
45 10.25 1.248 1.82 0.23 2.05 1.70 0.05 wAGN
52 9.11 0.933 1.91 3.63 5.54 2.34 0.02 HII
58 8.94 0.661 2.44 3.89 6.33 1.99 0.10 HII
77 10.54 0.938 1.82 0.68 2.5 1.36 0.02 wAGN
84 9.39 0.851 1.91 −0.28 1.63 1.87 0.05 wAGN
124 9.52 0.732 2.25 4.96 7.21 0.18 HII
134 9.96 0.797 2.25 −1.12 1.13 0.11 HII
164 9.91 1.061 1.91 −1.48 0.43 0.02 PAS
171 9.69 0.75 2.25 14.92 17.17 5.07 0.07 HII
185 10.06 1.171 1.82 −2.61 -0.79 0.91 0.07 RET
249 9.01 0.688 2.25 1.86 4.11 1.63 0.11 HII
258 11.1 1.12 1.82 −0.31 1.51 1.16 0.06 wAGN
270 10.93 1.151 1.82 1.48 0.04 RET
282 9.3 1.055 1.91 −2.27 −0.36 0.05 PAS
289 10.31 0.281 0.49 5.322 5.81 2.26 0.07 HII
291 9.86 1.075 1.91 −1.22 0.69 0.51 0.02 RET

Notes. Columns are: (1): HRS name; (2): log of stellar mass M* (M), from B15; (3): gi color index; (4): Absorption continuum correction toHα EW; (5): Observed Hα EW (positive EW means emission); (6): Corrected Hα EW (positive EW means emission); (7): Observed [NII] EW (λ6583 Å) (positive EW means emission); (8): rms near Hα; (9): Nuclear spectral classification (from WHAN).

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