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 2.

Percentage of total (compact and complex) radio AGN that have FRII-like morphologies.

	0 < z ≤ 0.285		0.285 < z ≤ 0.4
log(M_*/M_⊙)	♦	♢	♦	♢
10.6 − 11.0	$11 . 7_{- 6.6}^{+ 10.0}$ $11.7^{+10.0}_{-6.6}$	$21 . 9_{- 8.0}^{+ 9.7}$ $21.9^{+9.7}_{-8.0}$	−	−
11.0 − 11.2	$31 . 4_{- 16.7}^{+ 21.0}$ $31.4^{+21.0}_{-16.7}$	$16 . 2_{- 9.0}^{+ 13.2}$ $16.2^{+13.2}_{-9.0}$	$23 . 6_{- 10.7}^{+ 13.7}$ $23.6^{+13.7}_{-10.7}$	$21 . 2_{- 8.5}^{+ 10.7}$ $21.2^{+10.7}_{-8.5}$
11.2 − 11.4	$32 . 1_{- 14.2}^{+ 16.9}$ $32.1^{+16.9}_{-14.2}$	$32 . 6_{- 11.3}^{+ 12.9}$ $32.6^{+12.9}_{-11.3}$	$13 . 1_{- 6.2}^{+ 8.5}$ $13.1^{+8.5}_{-6.2}$	$22 . 7_{- 7.0}^{+ 8.3}$ $22.7^{+8.3}_{-7.0}$
11.4 − 12.0	$25 . 6_{- 10.2}^{+ 12.4}$ $25.6^{+12.4}_{-10.2}$	$30 . 9_{- 9.9}^{+ 11.3}$ $30.9^{+11.3}_{-9.9}$	$25 . 5_{- 9.1}^{+ 10.9}$ $25.5^{+10.9}_{-9.1}$	$26 . 1_{- 7.5}^{+ 8.6}$ $26.1^{+8.6}_{-7.5}$

Notes. The statistics are only shown for the incidence of the filled diamond λ_Jet sources (♦ on Fig. 22 where the boosted incidence is present) and for the range −3 < log λ_Jet ≤ −1.5 (unfilled diamond, ♢) in each stellar mass and redshift bin.

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