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Table 4.

Best-fit Saunders parameters of the observed Hα LF fits in two redshift bins, 0.02 < z < 0.12 (top) and 0.12 < z < 0.22 (bottom), to better understand their evolution.

Saunders Hα (observed LF)

log(Φ/[Mpc−3dex−1]) log(L/[erg s−1 ]) α σ
0.02 < z < 0.12
Full sample –2.21±0.02 40.20±0.16 –0.07±0.13 0.65±0.01 0.2
SF sSFR –2.27±0.03 40.10±0.10 0.08±0.19 0.65±0.01 0.2
SF BPT+WHAN –2.42±0.04 40.00±0.01 0.25±0.19 0.64±0.01 0.3
LINERs –3.27±0.21 40.00±0.79 –0.10±0.92 –0.47±0.05 1.3
Composite –2.73±0.13 40.00±0.39 –0.32±0.24 0.75±0.03 0.8
Seyfert –4.31±0.12 40.72±0.31 –0.17±0.25 0.53±0.05 2.7
Passive –3.92±0.53 41.29±0.90 –0.47±0.25 0.43±0.12 3.4

0.12 < z < 0.22
Full sample –3.61±0.42 40.00±1.66 2.12±0.16 –0.52±0.07 4.8
SF sSFR –3.29±0.73 40.34±0.56 1.30±0.45 0.51±0.04 2.8
SF BPT+WHAN –3.85±0.31 40.00±1.50 1.71±1.08 0.53±0.09 4.0
LINERs –3.84±0.51 40.00±0.23 0.81±0.72 0.45±0.18 4.5
Composite –5.12±0.37 42.59±0.30 –1.14±0.06 0.20±0.08 0.6
Seyfert –4.92±0.90 40.55±0.76 1.19±0.48 0.49±0.23 10.6
Passive

Notes. There are no passive galaxies above the completeness threshold LHα = 1041.1 erg s−1, in the high-z bin.

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