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Table 3
Parameter estimates of local comparison samples using the maximum-likelihood method with a Gaussian intrinsic distribution of the independent variable.
| Local TFR |
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| slope a | intercept b | scatter (σint) | ||
|
|
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| Sample T | B-band TFR | |||
| −7.93 ± 0.29 | −2.66 ± 0.64 | 0.43 ± 0.04 | ||
| −7.04 fixed | − 4.62 ± 0.04 | 0.40 ± 0.03 | ||
| Sample V | B-band TFR | |||
| −6.98 ± 0.52 | −4.65 ± 1.11 | 0.61 ± 0.10 | ||
| −7.04 fixed | − 4.52 ± 0.09 | 0.61 ± 0.09 | ||
| Sample P | stellar-mass TFR | |||
| 3.40 ± 0.11 | 2.89 ± 0.23 | 0.17 ± 0.02 | ||
| 3.04 fixed | 3.70 ± 0.02 | 0.15 ± 0.02 | ||
Notes.For each sample we carry out an inverse fit with a free and a fixed slope.
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