Table 1: Limiting values. These are the values of the limits of the morphological classes. The values are valid for the SDSS g and r bands. The value for the i band is the same as in the other filters for $\varepsilon$ . For CI it is slightly higher because i is more sensitive for the dominant redder bulge stars. In this case one should add a value of 0.1 to the numbers of the CI in this table. In general, note that the galaxies near boundaries have the least certain classification.
Class $\varepsilon$ CI

lower limit upper limit lower limit upper limit

Sa(f) - < 0.55 ${\geq} 2.70$ -

Sb(f) ${\geq} 0.55$ - ${\geq} 2.70$ -

Sc(f) - < 0.75 ${\geq} 2.15$ < 2.70

Scd(f) ${\geq} 0.75$ < 0.80 ${\geq} 2.15$ < 2.70

Sd(f) ${\geq} 0.80$ - - < 2.70

Irr(f) - < 0.80 - < 2.15

**Table 1:** Limiting values. These are the values of the limits of the morphological classes. The values are valid for the SDSS g and r bands. The value for the i band is the same as in the other filters for $\varepsilon$ . For CI it is slightly higher because i is more sensitive for the dominant redder bulge stars. In this case one should add a value of 0.1 to the numbers of the CI in this table. In general, note that the galaxies near boundaries have the least certain classification.
Class	$\varepsilon$	CI
	lower limit	upper limit	lower limit	upper limit
Sa(f)	-	< 0.55	${\geq} 2.70$	-
Sb(f)	${\geq} 0.55$	-	${\geq} 2.70$	-
Sc(f)	-	< 0.75	${\geq} 2.15$	< 2.70
Scd(f)	${\geq} 0.75$	< 0.80	${\geq} 2.15$	< 2.70
Sd(f)	${\geq} 0.80$	-	-	< 2.70
Irr(f)	-	< 0.80	-	< 2.15

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