CHANG-ES - IX. Radio scale heights and scale lengths of a consistent sample of 13 spiral galaxies seen edge-on and their correlations

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Volume 611 (March 2018)

A&A, 611 (2018) A72

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Table 3

Fit results.

Source	C-band D-array		L-band C-array
		h		h
	[′′]	[′′]	[′′]	[′′]
N2820	2.0 ± 1.6	9.1 ± 0.6	1.8 ± 0.5	11.6 ± 1.5
N3003	0.2 ± 3.1	0.4 ± 2.0	2.5 ± 2.5	29.7 ± 10.0
N3044	1.2 ± 1.8	10.5 ± 1.7	0.5 ± 0.7	13.6 ± 1.6
N3079	0.2 ± 0.1	15.4 ± 4.0	1.0 ± 1.4^b	11.8 ± 1.9^b
N3432	0.9 ± 0.9	15.1 ± 4.6	0.9 ± 0.9	20.3 ± 5.4
N3735	0.9 ± 1.2	7.0 ± 1.1	3.0 ± 0.4	8.1 ± 2.2
N3877	–	10.0 ± 1.8	–	12.5 ± 2.0
N4013	0.4 ± 0.3	8.2 ± 0.6	2.5 ± 1.1	13.2 ± 1.8
N4157	0.5 ± 0.6	13.0 ± 1.3	1.0 ± 1.4	14.4 ± 0.9
N4217	0.2 ± 0.1	10.8 ± 0.5	1.1 ± 0.7	10.6 ± 0.9
N4302	0.6 ± 0.6	11.9 ± 5.0	1.4 ± 1.3	10.7 ± 2.7
N5775	1.3 ± 1.3	10.4 ± 0.9	2.8 ± 1.2	14.2 ± 2.5
U10288	–	4.4 ± 0.1	–	5.1 ± 0.5

Notes. ^(a) We note the limitations on the thin disk scale height as discussed in Sect. 4.1. They are not considered further. ^(b) The L-band values for NGC 3079 may be underestimated because of the poor quality of the map (see Table 1).

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