Spectral type | Population (%) | u-r |
![]() |
||
no ev. | ref. | cons. | |||
-Early-type | |||||
---|---|---|---|---|---|
BCG | 4.3 | 4.0 | 4.2 | - | 0.12 |
E/S0 | 65.4 | 61.5 | 63.3 | - | 0.12 |
(Tot. early-type) | (69.7) | (65.5) | (67.5) | ||
-Late-type | |||||
Sa | 4.4 | 5.1 | 6.5 | >2.2 | 2.36 |
Sb | 9.6 | 10.7 | 11.7 | 1.8-2.2 | 13.82 |
Sc | 15.8 | 18.2 | 14.1 | 1.0-1.8 | 33.80 |
Starburst | 0.5 | 0.5 | 0.2 | <1.0 | 73.16 |
(Tot. late-type) | (30.3) | (34.5) | (32.5) |
Notes. The fraction (in percentile) of each type of
galaxies in the three population models is shown: without redshift
evolution, in our reference model and for the conservative scenario
(second to fourth column, respectively). The fifth column shows the
corresponding intrinsic u-r color intervals used
for the modelisation of the spirals (early-type galaxies are taken
directly from the SDSS-maxBCG catalogue). The last column shows the
values of the ratio
for each template.
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