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Table 5

Values of the predicted stellar mass-to-blue-light ratios in various theoretical models.

code BC PEGASE IP13 IP13 IP13 CvD12 CvD12

IMF Salpeter Salpeter Kroupa1 Kroupa2 Salpeter var. Kroupa MW
metallicity 0.02 0.02 ≤ 0.03 ≤ 0.03 ≤ 0.03 ~ 0.02 ~ 0.02
SFH SSP SSP CSP CSP CSP SSP SSP
(1) (2) (3) (4) (5) (6) (7) (8)

NGC 1400 6.0 6.6 3.9 4.3 7.4
NGC 1407 7.4 8.1 5.0 5.7 9.8
NGC 2768 6.4 7.0 4.2 4.7 8.2 1.41 1.48
NGC 3115 6.2 6.8 4.0 4.5 7.8
NGC 3377 4.8 5.2 2.9 3.1 5.4 3.27 2.81
NGC 4278 6.2 6.8 4.0 4.5 7.8 7.51 4.06
NGC 4365 6.9 7.6 4.6 5.2 9.0
NGC 4486 6.7 7.3 4.4 5.0 8.5 1.28 0.68
NGC 4494 5.3 5.8 3.2 3.6 6.2
NGC 5846 7.1 7.8 4.8 5.5 9.4 3.95 2.22

Notes. Column (1): name of the galaxy. Column (2): SPS Bruzual & Charlot (BC) model with Salpeter IMF for Z = 0.02. Column (3): SPS PEGASE model with Salpeter IMF for Z = 0.02. Column (4): the exponential SFH model with the Kroupa IMF (Into & Portinari 2013). Column (5): the disc galaxy model based on the Kroupa IMF (Into & Portinari 2013). Column (6): the disc galaxy model based on the Salpeter IMF (Into & Portinari 2013). Column (7): Conroy & van Dokkum (2012) model allowing for IMF variation. Column (8): Conroy & van Dokkum (2012) model assuming a fixed MW (Kroupa) IMF. See text for details.

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