2MASS wide field extinction maps - III. The Taurus, Perseus, and California cloud complexes

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Table 2:

The best-fit parameters and their 1- $\sigma$ errors for the log-normal distribution used to fit the column density probability shown in Fig. 11 (see Eq. (11) for the meaning of the various quantities).
Center A₀	Scale A₁	Dispersion $\sigma$	Normalization a
$-0.058 \pm 0.006$	$0.134 \pm 0.006$	$0.660 \pm 0.010$	$2314 \pm 81$

Source LaTeX | All tables | In the text

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