Table 4.
TFR zero-point difference between various reference samples and the MAGIC final kinematic sample, with a mass threshold of 109 M⊙, using similar slopes.
Sample | TFR | Tracer | α | Δ log M | Δ log V | ||
---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
ORELSE | smTFR | Vr22 | 3.18 | 0.38 | 0.23 | −0.119 | −0.072 |
KROSS rotdom | smTFR | Vr22 | 3.61 | 0.79 | 0.64 | −0.219 | −0.177 |
KROSS disky | smTFR | Vr22 | 4.42 | 0.45 | 0.30 | −0.102 | −0.068 |
ORELSE | smTFR | Vc22 | 3.24 | 0.31 | 0.16 | −0.096 | −0.049 |
KMOS3D | smTFR | Vc22 | 2.91 | 0.27 | 0.12 | −0.093 | −0.041 |
KMOS3D | smTFR | Vc22 | 3.60 (b) | 0.24 | 0.09 | −0.067 | −0.025 |
KMOS3D (a) | smTFR | Vc22 | 2.91 | 0.11 | −0.04 | −0.038 | 0.014 |
KMOS3D (a) | smTFR | Vc22 | 3.60 (b) | 0.12 | −0.03 | −0.033 | 0.008 |
KMOS3D | bmTFR | Vc22 | 2.21 | 0.31 | 0.16 | −0.140 | −0.072 |
KMOS3D | bmTFR | Vc22 | 3.75 (c) | 0.26 | 0.11 | −0.069 | −0.029 |
KMOS3D (a) | bmTFR | Vc22 | 2.21 | 0.15 | 0.00 | −0.068 | 0.000 |
KMOS3D (a) | bmTFR | Vc22 | 3.75 (c) | 0.19 | 0.04 | −0.051 | −0.011 |
Notes. (1) Identification of the comparison sample. (2) Type of TFR studied. (3) Tracer used to infer the TFR. (4) Value of the slope used. Zero-point difference in mass / velocity: (5)/(7) with no correction; (6)/(8) taking into account the −0.15 dex offset for the correction of stellar masses within R22.
These lines correspond to the difference between the KMOS3D sample and the MAGIC sample with a mass threshold of 1010 M⊙.
Value from Reyes et al. (2011) used in Übler et al. (2017) to compare with local Universe.
Value from Lelli et al. (2016) used in Übler et al. (2017) to compare with local Universe.
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