The variability angular diameter distance and the intrinsic brightness temperature of active galactic nuclei

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Table B.1.

Dependence of T_int on data constraints used.

ν^o	log₁₀T_int [K], ⟨log₁₀T_int [K]⟩

	t_i + 1 − t_i
[GHz]	< 30 days	< 50 days	< 100 days	< 500 days	< ∞ days
15	$10 . 73_{- 0.99}^{+ 0.83}$ $10.73^{+0.83}_{-0.99}$ , $10 . 63_{- 0.07}^{+ 0.07}$ $10.63^{+0.07}_{-0.07}$	$10 . 73_{- 1.01}^{+ 0.86}$ $10.73^{+0.86}_{-1.01}$ , $10 . 66_{- 0.05}^{+ 0.05}$ $10.66^{+0.05}_{-0.05}$	$10 . 88_{- 0.87}^{+ 0.78}$ $10.88^{+0.78}_{-0.87}$ , $10 . 84_{- 0.04}^{+ 0.04}$ $10.84^{+0.04}_{-0.04}$	$11 . 13_{- 0.81}^{+ 0.73}$ $11.13^{+0.73}_{-0.81}$ , $11 . 09_{- 0.03}^{+ 0.03}$ $11.09^{+0.03}_{-0.03}$	$11 . 19_{- 0.80}^{+ 0.75}$ $11.19^{+0.75}_{-0.80}$ , $11 . 15_{- 0.03}^{+ 0.03}$ $11.15^{+0.03}_{-0.03}$
15	(75)	(130)	(234)	(350)	(356)

43	$10 . 74_{- 1.12}^{+ 0.91}$ $10.74^{+0.91}_{-1.12}$ , $10 . 68_{- 0.13}^{+ 0.13}$ $10.68^{+0.13}_{-0.13}$	$10 . 85_{- 1.00}^{+ 0.94}$ $10.85^{+0.94}_{-1.00}$ , $10 . 84_{- 0.13}^{+ 0.14}$ $10.84^{+0.14}_{-0.13}$	$10 . 91_{- 0.96}^{+ 0.95}$ $10.91^{+0.95}_{-0.96}$ , $10 . 91_{- 0.13}^{+ 0.13}$ $10.91^{+0.13}_{-0.13}$	$10 . 92_{- 0.96}^{+ 0.94}$ $10.92^{+0.94}_{-0.96}$ , $10 . 91_{- 0.13}^{+ 0.13}$ $10.91^{+0.13}_{-0.13}$	$10 . 92_{- 0.96}^{+ 0.94}$ $10.92^{+0.94}_{-0.96}$ , $10 . 91_{- 0.13}^{+ 0.13}$ $10.91^{+0.13}_{-0.13}$
43	(37)	(37)	(38)	(38)	(38)

Notes. Values of log₁₀T_int [K] and ⟨log₁₀T_int [K]⟩ for a uniform disk geometry obtained for each of the different constraints on t_i + 1 − t_i. The first column corresponds observation frequency in units of GHz. Columns 2 to 6 correspond to the constraint on the t_i + 1 − t_i. The number of sources used in each constraint is given in parentheses under each value.

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