The Close AGN Reference Survey (CARS) - IFU survey data and the BH mass dependence of long-term AGN variability

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Volume 659 (March 2022)

A&A, 659 (2022) A124

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Table 5.

ENLR size measurements.

Object	R_ENLR, max^(a)	R_{ENLR, 10⁻¹⁶}^(b)	R_{ENLR, 10⁻¹⁵}^(c)
	[″]	[″]	[″]
HE0021−1819	5.3 ± 0.6	2.2 ± 0.6	1.0 ± 0.6
HE0040−1105	11.1 ± 0.6	5.1 ± 0.6	2.3 ± 0.6
HE0108−4743	2.1 ± 1.3	2.1 ± 1.3	2.1 ± 1.3
HE0114−0015	7.4 ± 0.5	< 0.8	< 0.8
HE0119−0118	5.8 ± 0.7	4.7 ± 0.7	< 0.8
HE0203−0031	20.7 ± 1.1	8.2 ± 1.1	3.2 ± 1.1
HE0212−0059	29.4 ± 0.6	0.9 ± 0.6	0.9 ± 0.6
HE0224−2834	24.9 ± 1.5	23.1 ± 1.5	4.6 ± 1.5
HE0227−0913	21.2 ± 1.0	9.3 ± 1.0	< 0.8
HE0232−0900	12.1 ± 1.0	8.0 ± 1.0	5.1 ± 1.0
HE0253−1641	4.6 ± 0.8	3.4 ± 0.8	3.1 ± 0.8
HE0345+0056	< 0.8	< 0.8	< 0.8
HE0351+0240	14.4 ± 0.7	13.7 ± 0.7	10.5 ± 0.7
HE0412−0803	28.0 ± 0.7	19.0 ± 0.7	7.4 ± 0.7
HE0429−0247	9.6 ± 0.8	6.7 ± 0.8	2.2 ± 0.8
HE0433−1028	11.1 ± 0.5	5.2 ± 0.5	1.8 ± 0.5
HE0853+0102	3.4 ± 0.6	2.0 ± 0.6	0.6 ± 0.6
HE0853−0126	< 1.0	< 1.0	< 1.0
HE0934+0119	7.6 ± 0.7	1.0 ± 0.7	1.0 ± 0.7
HE0949−0122	8.1 ± 1.7	8.1 ± 1.7	4.0 ± 1.7
HE1011−0403	4.5 ± 0.7	1.4 ± 0.7	< 0.8
HE1017−0305	7.0 ± 0.6	3.5 ± 0.6	< 0.8
HE1029−1831	9.1 ± 0.6	3.3 ± 0.6	< 0.8
HE1107−0813	25.0 ± 0.6	15.7 ± 0.6	1.6 ± 0.6
HE1108−2813	4.9 ± 0.4	2.3 ± 0.4	1.6 ± 0.4
HE1126−0407	9.2 ± 0.7	3.7 ± 0.7	2.3 ± 0.7
HE1237−0504	12.7 ± 0.5	12.3 ± 0.5	1.7 ± 0.5
HE1248−1356	12.3 ± 0.5	7.7 ± 0.5	3.2 ± 0.5
HE1310−1051	< 0.7	< 0.7	< 0.7
HE1330−1013	6.8 ± 0.7	2.4 ± 0.7	0.6 ± 0.7
HE1338−1423	10.0 ± 1.4	8.7 ± 1.4	5.1 ± 1.4
HE1353−1917	35.0 ± 0.7	35.0 ± 0.7	5.3 ± 0.7
HE1417−0909	6.6 ± 0.7	4.7 ± 0.7	0.6 ± 0.7
HE2128−0221	1.3 ± 0.7	1.3 ± 0.7	1.0 ± 0.7
HE2211−3903	6.7 ± 0.4	3.4 ± 0.4	1.0 ± 0.4
HE2222−0026	3.9 ± 0.6	< 0.8	< 0.8
HE2233+0124	22.2 ± 0.8	2.2 ± 0.8	< 0.8
HE2302−0857	30.0 ± 0.6	8.3 ± 0.6	6.1 ± 0.6

Notes.

^(a)

Maximum projected distance of all robust AGN-ionized regions with respect to the AGN location as seen in each IFU observation.

^(b)

Maximum projected distance of robust AGN-ionized regions with respect to the AGN location down to an intrinsic [O III] surface brightness limit of Σ₁₆ = 10⁻¹⁶ erg s⁻¹ cm⁻² arcsec⁻²(1 + z)⁻⁴.

^(c)

Maximum projected distance of robust AGN-ionized regions with respect to the AGN location down to an intrinsic [O III] surface brightness limit of Σ₁₅ = 10⁻¹⁵ erg s⁻¹ cm⁻² arcsec⁻²(1 + z)⁻⁴.

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