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

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Table B.2.

Dependence of T_int on data constraints used (fixed sources).

ν^o	log₁₀T_int [K], ⟨log₁₀T_int [K]⟩

	t_i + 1 − t_i
[GHz]	< 30 days	< 50 days	< 100 days	< 500 days	< ∞ days
15	$10 . 73_{- 1.00}^{+ 0.83}$ $10.73^{+0.83}_{-1.00}$ , $10 . 63_{- 0.07}^{+ 0.07}$ $10.63^{+0.07}_{-0.07}$	$10 . 84_{- 0.97}^{+ 0.85}$ $10.84^{+0.85}_{-0.97}$ , $10 . 77_{- 0.07}^{+ 0.07}$ $10.77^{+0.07}_{-0.07}$	$11 . 05_{- 0.95}^{+ 0.85}$ $11.05^{+0.85}_{-0.95}$ , $11 . 00_{- 0.08}^{+ 0.08}$ $11.00^{+0.08}_{-0.08}$	$11 . 32_{- 0.88}^{+ 0.77}$ $11.32^{+0.77}_{-0.88}$ , $11 . 27_{- 0.08}^{+ 0.08}$ $11.27^{+0.08}_{-0.08}$	$11 . 37_{- 0.86}^{+ 0.78}$ $11.37^{+0.78}_{-0.86}$ , $11 . 33_{- 0.08}^{+ 0.08}$ $11.33^{+0.08}_{-0.08}$
43	$10 . 74_{- 1.13}^{+ 0.91}$ $10.74^{+0.91}_{-1.13}$ , $10 . 68_{- 0.14}^{+ 0.14}$ $10.68^{+0.14}_{-0.14}$	$10 . 86_{- 1.01}^{+ 0.93}$ $10.86^{+0.93}_{-1.01}$ , $10 . 84_{- 0.12}^{+ 0.13}$ $10.84^{+0.13}_{-0.12}$	$10 . 93_{- 1.00}^{+ 0.95}$ $10.93^{+0.95}_{-1.00}$ , $10 . 91_{- 0.13}^{+ 0.13}$ $10.91^{+0.13}_{-0.13}$	$10 . 93_{- 1.00}^{+ 0.94}$ $10.93^{+0.94}_{-1.00}$ , $10 . 91_{- 0.13}^{+ 0.14}$ $10.91^{+0.14}_{-0.13}$	$10 . 94_{- 0.99}^{+ 0.93}$ $10.94^{+0.93}_{-0.99}$ , $10 . 92_{- 0.13}^{+ 0.13}$ $10.92^{+0.13}_{-0.13}$

Notes. The same as Table B.1, but with the source sample fixed to the 75 sources at 15 GHz and 37 sources at 43 GHz that are common in all constraint sets. The number of sources used in each constraint has been omitted as it is fixed throughout for each frequency.

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