Table 2.
Parameters of the galaxy models.
| Subset | Model |
 |
 |
 |
 |
 |
re |
|---|---|---|---|---|---|---|---|
| [arcsec] | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| #1 | mii001 | 0.25 | 0.20 | 0.67 | 0.11 | 0.10 | 9.6 |
| mii002 | 0.50 | 0.33 | 0.67 | 0.22 | 0.18 | 9.3 | |
| mii003 | 0.75 | 0.43 | 0.67 | 0.33 | 0.25 | 9.0 | |
| mii004 | 1.00 | 0.50 | 0.67 | 0.44 | 0.31 | 8.8 | |
| mii005 | 1.25 | 0.56 | 0.67 | 0.54 | 0.35 | 8.6 | |
| mii006 | 1.50 | 0.60 | 0.67 | 0.65 | 0.39 | 8.5 | |
| mii007 | 1.75 | 0.64 | 0.67 | 0.76 | 0.43 | 8.4 | |
| mii008 | 2.00 | 0.67 | 0.67 | 0.87 | 0.47 | 8.2 | |
| #2 | mii009 | 0.25 | 0.20 | 1.00 | 0.25 | 0.20 | 10.0 |
| mii010 | 0.50 | 0.33 | 1.00 | 0.50 | 0.33 | 10.0 | |
| mii011 | 0.75 | 0.43 | 1.00 | 0.75 | 0.43 | 10.0 | |
| mii012 | 1.00 | 0.50 | 1.00 | 1.00 | 0.50 | 10.0 | |
| mii013 | 1.25 | 0.56 | 1.00 | 1.25 | 0.56 | 10.0 | |
| mii014 | 1.50 | 0.60 | 1.00 | 1.50 | 0.60 | 10.0 | |
| mii015 | 1.75 | 0.64 | 1.00 | 1.75 | 0.64 | 10.0 | |
| mii016 | 2.00 | 0.67 | 1.00 | 2.00 | 0.67 | 10.0 | |
| #3 | mii017 | 0.25 | 0.20 | 1.33 | 0.44 | 0.31 | 11.0 |
| mii018 | 0.50 | 0.33 | 1.33 | 0.88 | 0.47 | 11.5 | |
| mii019 | 0.75 | 0.43 | 1.33 | 1.33 | 0.57 | 11.8 | |
| mii020 | 1.00 | 0.50 | 1.33 | 1.77 | 0.64 | 12.0 | |
| mii021 | 1.25 | 0.56 | 1.33 | 2.21 | 0.69 | 12.2 | |
| mii022 | 1.50 | 0.60 | 1.33 | 2.65 | 0.73 | 12.4 | |
| mii023 | 1.75 | 0.64 | 1.33 | 3.10 | 0.76 | 12.5 | |
| mii024 | 2.00 | 0.67 | 1.33 | 3.54 | 0.78 | 12.6 | |
Notes. Column (1): Subset number. Column (2): Name of the galaxy model, where ii = {40, 50, 70} is the model inclination in degree. Column (3)−(4): Ratio of the central surface brightness of the counter-rotating disk to that of the prograde disk and to that of the model. Column (5): Ratio of the scale length of the counter-rotating disk to that of the prograde disk. Column (6)−(7): Ratio of the total luminosity of the counter-rotating disk to that of the prograde disk and to that of the model. Column (8): Effective radius of the model.
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