Table 3.

The difference between mean |$\lambda _{\rm {\it R}_{\rm e}}$| and concentration (C) for different morphological or SFR-defined classes.

|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔCSignificanceFrac. DF
log (M*)(S0-eSp)(S0-eSp)|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC
All Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.099 ± 0.0200.341 ± 0.039−5.08.70.560.24
10.5–11.0−0.130 ± 0.0180.419 ± 0.040−7.310.50.420.20
11.0–11.5−0.288 ± 0.0440.598 ± 0.075−6.67.90.190.14
All−0.132 ± 0.0130.417 ± 0.026−10.416.10.420.20
No-SR Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.097 ± 0.0170.352 ± 0.039−5.79.00.560.23
10.5–11.0−0.098 ± 0.0160.409 ± 0.040−6.210.10.560.20
11.0–11.5−0.220 ± 0.0370.596 ± 0.079−5.97.60.250.14
All−0.104 ± 0.0110.409 ± 0.026−9.615.50.530.20
No-SR SFR (INT-SF)
9.5–10.0−0.026 ± 0.0330.100 ± 0.054−0.81.82.140.91
10.0–10.5−0.066 ± 0.0180.194 ± 0.036−3.65.40.850.47
10.5–11.0−0.084 ± 0.0190.301 ± 0.045−4.36.60.670.30
11.0–11.5−0.210 ± 0.0380.403 ± 0.104−5.53.90.270.23
All−0.081 ± 0.0110.309 ± 0.026−7.312.10.690.29
No-SR SFR (PAS-SF)
9.5–10.0−0.105 ± 0.0220.272 ± 0.042−4.76.40.530.34
10.0–10.5−0.194 ± 0.0120.445 ± 0.026−15.916.80.290.20
10.5–11.0−0.191 ± 0.0160.517 ± 0.035−12.314.80.290.18
11.0–11.5−0.307 ± 0.0370.603 ± 0.098−8.36.10.180.15
All−0.187 ± 0.0080.506 ± 0.019−22.626.80.300.18
|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔCSignificanceFrac. DF
log (M*)(S0-eSp)(S0-eSp)|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC
All Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.099 ± 0.0200.341 ± 0.039−5.08.70.560.24
10.5–11.0−0.130 ± 0.0180.419 ± 0.040−7.310.50.420.20
11.0–11.5−0.288 ± 0.0440.598 ± 0.075−6.67.90.190.14
All−0.132 ± 0.0130.417 ± 0.026−10.416.10.420.20
No-SR Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.097 ± 0.0170.352 ± 0.039−5.79.00.560.23
10.5–11.0−0.098 ± 0.0160.409 ± 0.040−6.210.10.560.20
11.0–11.5−0.220 ± 0.0370.596 ± 0.079−5.97.60.250.14
All−0.104 ± 0.0110.409 ± 0.026−9.615.50.530.20
No-SR SFR (INT-SF)
9.5–10.0−0.026 ± 0.0330.100 ± 0.054−0.81.82.140.91
10.0–10.5−0.066 ± 0.0180.194 ± 0.036−3.65.40.850.47
10.5–11.0−0.084 ± 0.0190.301 ± 0.045−4.36.60.670.30
11.0–11.5−0.210 ± 0.0380.403 ± 0.104−5.53.90.270.23
All−0.081 ± 0.0110.309 ± 0.026−7.312.10.690.29
No-SR SFR (PAS-SF)
9.5–10.0−0.105 ± 0.0220.272 ± 0.042−4.76.40.530.34
10.0–10.5−0.194 ± 0.0120.445 ± 0.026−15.916.80.290.20
10.5–11.0−0.191 ± 0.0160.517 ± 0.035−12.314.80.290.18
11.0–11.5−0.307 ± 0.0370.603 ± 0.098−8.36.10.180.15
All−0.187 ± 0.0080.506 ± 0.019−22.626.80.300.18

Notes. This is shown in mass intervals for the difference between S0 (mtype = 1) and eSp (mtype = 2) galaxies, the different between INT and SF galaxies, and the difference between PAS and SF galaxies. Samples listed as ’No-SR’ do not include slow rotators (which lie within the region defined by Cappellari 2016). We also list the significance of the difference and the fractional difference that can be contributed by disc fading. For the disc fading contribution, we compare to the model results averaged over all B/T and inclination values, of |$\Delta \lambda _{\rm {\it R}_{\rm e}}=-0.056$| and ΔC = 0.091. The last row for each sample contains the results for the full mass range between log (M*/M) = 9.5 and 11.5, based on an inverse variance weighted average of the individual mass bins.

Table 3.

The difference between mean |$\lambda _{\rm {\it R}_{\rm e}}$| and concentration (C) for different morphological or SFR-defined classes.

|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔCSignificanceFrac. DF
log (M*)(S0-eSp)(S0-eSp)|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC
All Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.099 ± 0.0200.341 ± 0.039−5.08.70.560.24
10.5–11.0−0.130 ± 0.0180.419 ± 0.040−7.310.50.420.20
11.0–11.5−0.288 ± 0.0440.598 ± 0.075−6.67.90.190.14
All−0.132 ± 0.0130.417 ± 0.026−10.416.10.420.20
No-SR Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.097 ± 0.0170.352 ± 0.039−5.79.00.560.23
10.5–11.0−0.098 ± 0.0160.409 ± 0.040−6.210.10.560.20
11.0–11.5−0.220 ± 0.0370.596 ± 0.079−5.97.60.250.14
All−0.104 ± 0.0110.409 ± 0.026−9.615.50.530.20
No-SR SFR (INT-SF)
9.5–10.0−0.026 ± 0.0330.100 ± 0.054−0.81.82.140.91
10.0–10.5−0.066 ± 0.0180.194 ± 0.036−3.65.40.850.47
10.5–11.0−0.084 ± 0.0190.301 ± 0.045−4.36.60.670.30
11.0–11.5−0.210 ± 0.0380.403 ± 0.104−5.53.90.270.23
All−0.081 ± 0.0110.309 ± 0.026−7.312.10.690.29
No-SR SFR (PAS-SF)
9.5–10.0−0.105 ± 0.0220.272 ± 0.042−4.76.40.530.34
10.0–10.5−0.194 ± 0.0120.445 ± 0.026−15.916.80.290.20
10.5–11.0−0.191 ± 0.0160.517 ± 0.035−12.314.80.290.18
11.0–11.5−0.307 ± 0.0370.603 ± 0.098−8.36.10.180.15
All−0.187 ± 0.0080.506 ± 0.019−22.626.80.300.18
|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔCSignificanceFrac. DF
log (M*)(S0-eSp)(S0-eSp)|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC|$\Delta \lambda _{\rm {\it R}_{\rm e}}$|ΔC
All Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.099 ± 0.0200.341 ± 0.039−5.08.70.560.24
10.5–11.0−0.130 ± 0.0180.419 ± 0.040−7.310.50.420.20
11.0–11.5−0.288 ± 0.0440.598 ± 0.075−6.67.90.190.14
All−0.132 ± 0.0130.417 ± 0.026−10.416.10.420.20
No-SR Morph (S0-eSp)
9.5–10.0−0.006 ± 0.0480.175 ± 0.088−0.12.09.930.47
10.0–10.5−0.097 ± 0.0170.352 ± 0.039−5.79.00.560.23
10.5–11.0−0.098 ± 0.0160.409 ± 0.040−6.210.10.560.20
11.0–11.5−0.220 ± 0.0370.596 ± 0.079−5.97.60.250.14
All−0.104 ± 0.0110.409 ± 0.026−9.615.50.530.20
No-SR SFR (INT-SF)
9.5–10.0−0.026 ± 0.0330.100 ± 0.054−0.81.82.140.91
10.0–10.5−0.066 ± 0.0180.194 ± 0.036−3.65.40.850.47
10.5–11.0−0.084 ± 0.0190.301 ± 0.045−4.36.60.670.30
11.0–11.5−0.210 ± 0.0380.403 ± 0.104−5.53.90.270.23
All−0.081 ± 0.0110.309 ± 0.026−7.312.10.690.29
No-SR SFR (PAS-SF)
9.5–10.0−0.105 ± 0.0220.272 ± 0.042−4.76.40.530.34
10.0–10.5−0.194 ± 0.0120.445 ± 0.026−15.916.80.290.20
10.5–11.0−0.191 ± 0.0160.517 ± 0.035−12.314.80.290.18
11.0–11.5−0.307 ± 0.0370.603 ± 0.098−8.36.10.180.15
All−0.187 ± 0.0080.506 ± 0.019−22.626.80.300.18

Notes. This is shown in mass intervals for the difference between S0 (mtype = 1) and eSp (mtype = 2) galaxies, the different between INT and SF galaxies, and the difference between PAS and SF galaxies. Samples listed as ’No-SR’ do not include slow rotators (which lie within the region defined by Cappellari 2016). We also list the significance of the difference and the fractional difference that can be contributed by disc fading. For the disc fading contribution, we compare to the model results averaged over all B/T and inclination values, of |$\Delta \lambda _{\rm {\it R}_{\rm e}}=-0.056$| and ΔC = 0.091. The last row for each sample contains the results for the full mass range between log (M*/M) = 9.5 and 11.5, based on an inverse variance weighted average of the individual mass bins.

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