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Table 2.

Baryonic bulge-to-total ratio and the number of satellites for sample galaxies.

Name B/T e_B/T N e_N
SAGA

1015 0.237 0.009 2 1.414
1309 0.062 0.004 3 1.732
2543 0.292 0.008 2 1.414
2962 0.265 0.009 3 1.732
2967 0.007 0.001 1 1.000
3689 0.049 0.001 2 1.414
3976 0.557 0.025 2 1.414
4158 0.788 0.040 5 2.236
4454 0.259 0.013 4 2.000
5297 0.103 0.004 7 2.646
5347 0.160 0.004 2 1.414
5448 0.259 0.007 5 2.236
5602 0.309 0.007 5 2.236
5604 0.014 0.001 3 1.732
5633 0.331 0.009 0 0.000
5690 0.530 0.015 3 1.732
5750 0.287 0.006 1 1.000
5792 0.421 0.020 3 1.732
5869 0.657 0.054 0 0.000
5962 0.335 0.020 2 1.414
6181 0.312 0.011 9 3.000
6278 0.420 0.028 9 3.000
6909 0.414 0.016 4 2.000
7029 0.313 0.009 5 2.236
7079 0.248 0.006 4 2.000
7328 0.150 0.014 1 1.000
7541 0.017 0.000 5 2.236
7716 0.242 0.006 2 1.414
68743 0.462 0.013 5 2.236

Javanmardi & Kroupa (2020)

MW 0.200 0.075 5 2.236
M 31 0.320 0.110 8 2.828
M 33 0.010 0.001 0 0.000
M 81 0.460 0.150 13 3.606
Cen A 1.000 0.100 10 3.162
M 94 0.100 0.020 0 0.000
M 101 0.050 0.030 0 0.000

Notes. Baryonic bulge-to-total mass ratio (B/T) and the number of satellites (N) brighter than the SAGA limit are given along with their corresponding errors for: all SAGA galaxies (upper part) labeled with their NGC number with one exception of a single five-digit number that has a PGC prefix (the last SAGA galaxy listed), and nearby galaxies from Javanmardi & Kroupa (2020) (lower part). The number of satellites from Javanmardi & Kroupa (2020) has been reduced to the SAGA limit for direct comparison.

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