The LOFAR – eFEDS survey: The incidence of radio and X-ray AGN and the disk–jet connection

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Volume 686 (June 2024)

A&A, 686 (2024) A43

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Table 3.

Fit results for the power law and power law plus Gaussian trends fit to the incidence of radio AGN in different stellar mass and redshift bins (z1 and z2 for the low and high redshift bins, respectively).

	Compact-only (pow)				Compact and complex (pow+Gauss)
	Pow norm.		Pow slope		Pow norm.		Gauss norm.
log(M_*/M_⊙)	z1	z2	z1	z2	z1	z2	z1	z2
10.6 − 11.0	$1 . 5_{- 0.6}^{+ 0.5}$ $1.5^{+0.5}_{-0.6}$	−	$- 1 . 29_{- 0.6}^{+ 0.88}$ $-1.29^{+0.88}_{-0.6}$	−	$2 . 0_{- 0.6}^{+ 0.5}$ $2.0^{+0.5}_{-0.6}$	−	$1 . 0_{- 0.7}^{+ 0.6}$ $1.0^{+0.6}_{-0.7}$	−
11.0 − 11.2	$3 . 0_{- 0.9}^{+ 0.9}$ $3.0^{+0.9}_{-0.9}$	$5 . 4_{- 2.2}^{+ 1.5}$ $5.4^{+1.5}_{-2.2}$	$- 1 . 38_{- 0.4}^{+ 0.52}$ $-1.38^{+0.52}_{-0.4}$	$- 1 . 69_{- 0.62}^{+ 0.74}$ $-1.69^{+0.74}_{-0.62}$	$4 . 2_{- 0.9}^{+ 1.1}$ $4.2^{+1.1}_{-0.9}$	$8 . 1_{- 2.4}^{+ 2.3}$ $8.1^{+2.3}_{-2.4}$	$0 . 8_{- 1.5}^{+ 1.2}$ $0.8^{+1.2}_{-1.5}$	$2 . 0_{- 2.0}^{+ 1.7}$ $2.0^{+1.7}_{-2.0}$
11.2 − 11.4	$6 . 2_{- 2.1}^{+ 1.7}$ $6.2^{+1.7}_{-2.1}$	$10 . 3_{- 4.0}^{+ 2.8}$ $10.3^{+2.8}_{-4.0}$	$- 1 . 61_{- 0.39}^{+ 0.51}$ $-1.61^{+0.51}_{-0.39}$	$- 1 . 59_{- 0.54}^{+ 0.7}$ $-1.59^{+0.7}_{-0.54}$	$9 . 8_{- 3.2}^{+ 2.9}$ $9.8^{+2.9}_{-3.2}$	$15 . 4_{- 5.4}^{+ 4.3}$ $15.4^{+4.3}_{-5.4}$	$5 . 6_{- 4.0}^{+ 3.3}$ $5.6^{+3.3}_{-4.0}$	$8 . 2_{- 5.0}^{+ 4.2}$ $8.2^{+4.2}_{-5.0}$
11.4 − 12.0	$11 . 7_{- 4.0}^{+ 3.4}$ $11.7^{+3.4}_{-4.0}$	$14 . 1_{- 3.6}^{+ 3.4}$ $14.1^{+3.4}_{-3.6}$	$- 1 . 45_{- 0.38}^{+ 0.51}$ $-1.45^{+0.51}_{-0.38}$	$- 1 . 46_{- 0.38}^{+ 0.49}$ $-1.46^{+0.49}_{-0.38}$	$21 . 7_{- 6.0}^{+ 5.8}$ $21.7^{+5.8}_{-6.0}$	$21 . 1_{- 4.5}^{+ 5.2}$ $21.1^{+5.2}_{-4.5}$	$30 . 5_{- 19.6}^{+ 10.9}$ $30.5^{+10.9}_{-19.6}$	$23 . 2_{- 16.4}^{+ 10.7}$ $23.2^{+10.7}_{-16.4}$

Notes. The power law norm (pow norm.) is the value of the intercept ×10³ at log λ_Jet = −3.25. Gauss norm. represents the normalisation of the Gaussian function, with an additional multiplicative factor of 1000. These values are used to plot the trends in Figs. 19 and 22.

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