Table 2.
Classification criteria for simulated and observed galaxy samples.
TNG100 simulations | |||
---|---|---|---|
SubhaloFlag=True; N⋆ > 200; NDM > 200 | |||
Class | Selection criteria | Snapshots | Number |
nETGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; log sSFR × yr−1 < −11; log σ/km s−1 > 1.9 and log M⋆/M⊙ > 10.1 | z = 0.00 − 0.10 | 70 859 |
dETGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; log sSFR × yr−1 < −11; log σ/km s−1 < 1.9 and log M⋆/M⊙ < 10.1 | z = 0.00 − 0.10 | 21 416 |
LTGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; log sSFR × yr−1 > −11 | z = 0.00 − 0.10 | 247 229 |
TNG_all | nETGs+dETGs+LTGs | z = 0.00 − 0.10 | 339 504 |
Observations | |||
Class | Selection criteria | Redshifts range | Number |
SPIDER/nETGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; Mtot(r1/2) > M⋆(r1/2); log σ/km s−1 > 1.9 and log M⋆/M⊙ > 10.1 | z = 0.05 − 0.095 | 3592 |
DynPoP/nETGs | as SPIDER/nETGs + Qual ≥ 1 and (DynPop_E or DynPop_S0) | z = 0.01 − 0.10 | 1271 |
DynPop/LTGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; Mtot(r1/2) > M⋆(r1/2); Qual ≥ 1 and DynPop_S | z = 0.01 − 0.10 | 2846 |
Fornax/dETGs | r1/2 > 2Rp; log M⋆/M⊙ > 8.3; Mtot(r1/2) > M⋆(r1/2); log σ/km s−1 < 1.9 and log M⋆/M⊙ < 10.1 | z = 0.00 | 9+6 |
Where we have defined (see text): | |||
DynPop_E | (PLTG < 0.5) and (T-Type < 0) and (PS0 < 0.5) and (VC = 1) and (VF = 0) | ||
DynPop_S0 | (PLTG < 0.5) and (T-Type < 0) and (PS0 > 0.5) and (VC = 2) and (VF = 0) | ||
DynPop_S | (PLTG < 0.5) and (T-Type > 0) and (VC = 3) and (VF = 0) |
Notes. The Plummer radius is Rp = 0.74 kpc as mentioned in Sect. 2.2. For the observed dwarf sample (SAMI-Fornax) we add a more relaxed selection (r1/2 > 1 kpc) for the size to enlarge the predictive sample, but use this as secondary test sample (1 kpc < r1/2 < 2Rp).
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