Search for radio halos in starburst galaxies | Astronomy & Astrophysics (A&A)

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Volume 685 (May 2024)

A&A, 685 (2024) A157

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Table 3.

Parameters obtained from fitting a single-component function to the z profile of the sample galaxies without halos.

Name	rms	d_r	$z_{0}^{d}$ $z_{0}^{\mathrm{d}}$
	(μJy beam⁻¹)	(′)	(″)
		(kpc)	(kpc)
(1)	(2)	(3)	(4)
ESO 428-G028	24	2.54	4.28 ± 0.08
		22.98	0.64 ± 0.01
IC 4595	18	3.16	5.95 ± 0.06
		42.06	1.32 ± 0.01
NGC 134	24	6.53	26.2 ± 0.2
		30.20	2.02 ± 0.01
NGC 1448	24	5.44	12.7 ± 0.4
		18.15	0.71 ± 0.02
NGC 2613	20	5.43	25.7 ± 0.7
		31.86	2.52 ± 0.07
NGC 2706	20	1.92	5.2 ± 0.1
		13.60	0.62 ± 0.01
NGC 3175	20	3.01	8.9 ± 0.1
		11.76	0.57 ± 0.01
NGC 3263	19	3.47	5.4 ± 0.1
		39.13	1.02 ± 0.02
NGC 3717	19	3.56	4.4 ± 0.1
		22.15	0.45 ± 0.01
NGC 4835	19	4.32	11.2 ± 0.1
		30.11	1.30 ± 0.02
NGC 5073	21	2.59	1.02 ± 0.07
		27.90	0.18 ± 0.01
UGCA 150	18	4.20	11.1 ± 0.2
		32.82	1.44 ± 0.02
UGCA 394	26	3.18	5.8 ± 0.4
		27.77	0.85 ± 0.05
UGCA 402	26	3.49	8.0 ± 0.2
		31.41	1.19 ± 0.03

Notes. (1) Galaxy common name. (2) Value of the rms noise estimated with the method described in Sect. 3.1. (3) Diameter of the radio emission calculated from the 3-σ contour in arc-minutes and in kpc, using the distances from Table 1. (4) Scale height of the disk in arc-seconds and kpc.

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