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Table 2
GSMF in low- and high-density regions: Schechter parameters resulting from the STY method, when applied to different galaxy populations at different redshifts.
| Galaxy sample | α | log ℳ⋆ | Φ⋆ | α | log ℳ⋆ | Φ⋆ |
|
|
|
|
|||
| 0.51 <z< 0.65 | low density | high density | ||||
| Total |
|
|
|
|
|
|
| Passive |
|
|
|
|
|
|
| Active |
|
|
|
|
|
|
| 0.65 <z< 0.80 | low density | high density | ||||
| Total |
|
|
|
|
|
|
| Passive |
|
|
|
|
|
|
| Active |
|
|
|
|
|
|
| 0.80 <z< 0.90 | low density | high density | ||||
| Total | − 0.52 |
|
|
− 0.80 |
|
|
| Passive | − 0.14 |
|
|
− 0.40 |
|
|
| Active | − 1.26 |
|
|
− 0.91 |
|
|
Notes. Before fitting data at 0.8 <z< 0.9, α has been fixed to the value of the previous z-bin.
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