Galactic bars and active galactic nucleus fuelling in the second half of cosmic history

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Volume 707 (March 2026)

A&A, 707 (2026) A152

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Table C.1.

Best-fit parameters of Eq. C.1 for X-ray and MIR AGN, and of Eq. C.2 for SED AGN.

AGN type	α	c
X-ray	$16 . 2_{- 3.52}^{+ 4.87}$ $Mathematical equation: $ 16.2^{+4.87}_{-3.52} $$	$0 . 287_{- 0.009}^{+ 0.009}$ $Mathematical equation: $ 0.287^{+0.009}_{-0.009} $$
MIR	$35 . 0_{- 9.46}^{+ 43.1}$ $Mathematical equation: $ 35.0^{+43.1}_{-9.46} $$	$0 . 478_{- 0.023}^{+ 0.022}$ $Mathematical equation: $ 0.478^{+0.022}_{-0.023} $$

AGN type	α	β	γ

SED	$47 . 2_{- 14.0}^{+ 29.1}$ $Mathematical equation: $ 47.2^{+29.1}_{-14.0} $$	$0 . 432_{- 0.018}^{+ 0.019}$ $Mathematical equation: $ 0.432^{+0.019}_{-0.018} $$	$0 . 637_{- 0.030}^{+ 0.041}$ $Mathematical equation: $ 0.637^{+0.041}_{-0.030} $$

Notes. Each parameter is estimated using a resampling process. The values reported are the median values of the 10 000 best-fit parameters and their 25^th–75^th percentile ranges.

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