ViCTORIA project: The LOFAR view of environmental effects in Virgo cluster star-forming galaxies

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Table A.1.

LOFAR data.

Name	S₁₄₄	d	L₁₄₄
	[Jy]	[Mpc]	[W Hz⁻¹]
(1)	(2)	(3)	(4)	(5)
HRS 2	(1.5±0.3)e−2	18.44	(6.1±1.3)e+20	−0.47 ± 0.11^a
IC 610	(2.0±0.4)e−2	16.71	(6.5±1.3)e+20	−0.58 ± 0.11^a
NGC 3254	(3.4±0.5)e−2	19.37	(1.5±0.2)e+21	< − 1.25^a
NGC 3277	(1.8±0.3)e−2	20.21	(8.8±1.4)e+20	−0.58 ± 0.09^a
HRS 10	(8.2±1.3)e−3	21.66	(4.6±0.8)e+20	−0.56 ± 0.13^a
NGC 3287	(2.8±0.6)e−2	18.93	(1.2±0.2)e+21	−0.39 ± 0.10^a
HRS 12	(3.4±0.8)e−3	19.89	(1.6±0.4)e+20	< − 0.27^a
NGC 3294	(2.3±0.3)e−1	22.47	(1.4±0.2)e+22	−0.70 ± 0.08^a
NGC 3338	(7.1±1.4)e−2	18.57	(2.9±0.6)e+21	−0.40 ± 0.10^a
NGC 3346	(3.0±0.6)e−2	18.0	(1.2±0.2)e+21	−0.34 ± 0.10^a
NGC 3380	(1.1±0.2)e−2	22.91	(7.1±1.2)e+20	−0.68 ± 0.12^a
NGC 3381	(2.9±0.4)e−2	23.29	(1.9±0.3)e+21	−0.70 ± 0.09^a
NGC 3395	(3.9±0.6)e−1	23.1	(2.5±0.4)e+22	−0.64 ± 0.08^a
NGC 3424	(3.0±0.4)e−1	21.44	(1.6±0.2)e+22	−0.75 ± 0.08^a
NGC 3430	(1.4±0.2)e−1	22.64	(8.7±1.3)e+21	−0.68 ± 0.08^a
NGC 3437	(2.6±0.5)e−1	18.24	(1.0±0.2)e+22	−0.59 ± 0.10^a
HRS 26	(4.8±0.8)e−3	22.41	(2.9±0.5)e+20	< − 0.42^a
NGC 3442	(4.6±0.7)e−2	24.77	(3.4±0.5)e+21	−0.56 ± 0.08^a
NGC 3451	(3.0±0.6)e−2	19.03	(1.3±0.3)e+21	−0.43 ± 0.10^a
NGC 3448	(1.9±0.3)e−1	19.63	(8.6±1.3)e+21	−0.54 ± 0.08^a
NGC 3504	(8.8±1.3)e−1	21.94	(5.1±0.8)e+22	−0.51 ± 0.08^a
NGC 3512	(3.8±0.6)e−2	19.61	(1.7±0.3)e+21	−0.56 ± 0.08^a
NGC 3596	(5.8±1.2)e−2	17.04	(2.0±0.4)e+21	−0.51 ± 0.10^a
NGC 3629	(2.1±0.4)e−2	21.53	(1.2±0.2)e+21	−0.46 ± 0.10^a
NGC 3631	(4.3±0.6)e−1	16.5	(1.4±0.2)e+22	−0.72 ± 0.08^a
NGC 3655	(1.6±0.3)e−1	21.43	(8.6±1.7)e+21	−0.43 ± 0.10^a
NGC 3657	(9.1±1.4)e−3	17.2	(3.2±0.5)e+20	−0.39 ± 0.10^a
NGC 3666	(5.1±1.0)e−2	15.14	(1.4±0.3)e+21	−0.45 ± 0.10^a
NGC 3684	(6.4±1.6)e−2	16.54	(2.1±0.5)e+21	−0.64 ± 0.11^a
NGC 3683	(4.9±0.7)e−1	24.4	(3.5±0.5)e+22	−0.69 ± 0.08^a
NGC 3686	(8.7±1.8)e−2	16.51	(2.8±0.6)e+21	−0.74 ± 0.10^a
NGC 3729	(6.8±1.0)e−2	15.14	(1.9±0.3)e+21	−0.51 ± 0.08^a
HRS 61	(4.3±0.7)e−3	17.39	(1.6±0.3)e+20	< − 0.37^a
NGC 3755	(3.2±0.5)e−2	22.44	(2.0±0.3)e+21	−0.57 ± 0.08^a
NGC 3756	(2.8±0.4)e−2	18.41	(1.1±0.2)e+21	−0.81 ± 0.09^a
NGC 3795	(3.7±0.6)e−3	17.33	(1.3±0.2)e+20	< − 0.31^a
NGC 3794	(1.0±0.2)e−2	19.76	(4.8±0.8)e+20	< − 0.74^a
NGC 3813	(3.4±0.5)e−1	20.97	(1.8±0.3)e+22	−0.57 ± 0.08^a
HRS 67	(6.2±1.0)e−3	20.51	(3.1±0.5)e+20	−0.34 ± 0.11^a
HRS 68	(1.1±0.2)e−2	20.17	(5.6±0.8)e+20	−0.49 ± 0.10^a
NGC 3898	(3.9±0.6)e−2	16.73	(1.3±0.2)e+21	−0.78 ± 0.08^a
NGC 3953	(2.4±0.4)e−1	15.0	(6.4±1.0)e+21	−0.75 ± 0.08^a
NGC 3982	(2.5±0.4)e−1	15.83	(7.6±1.1)e+21	−0.61 ± 0.08^a
HRS 76	(4.7±0.8)e−3	15.27	(1.3±0.2)e+20	−0.18 ± 0.11^a
NGC 4100	(2.1±0.3)e−1	15.31	(6.0±0.9)e+21	−0.60 ± 0.08^a
NGC 4178	(5.6±1.2)e−2	16.5	(1.8±0.4)e+21	−0.38 ± 0.10^a
IC 3061	(1.2±0.3)e−2	16.5	(3.8±0.9)e+20	< − 0.80^a
NGC 4207	(3.4±0.7)e−2	16.5	(1.1±0.2)e+21	−0.25 ± 0.10^a
NGC 4212	(1.3±0.3)e−1	16.5	(4.1±0.8)e+21	−0.72 ± 0.10^a
NGC 4216	(6.4±1.3)e−2	16.5	(2.1±0.4)e+21	−0.72 ± 0.10^b
NGC 4222	(1.3±0.3)e−2	16.5	(4.4±1.0)e+20	−0.58 ± 0.12^a
NGC 4237	(2.3±0.5)e−2	16.5	(7.5±1.7)e+20	−0.58 ± 0.11^a
IC 3105^†	(4.0±1.1)e−3	16.5	(1.3±0.4)e+20	< − 0.36^c
NGC 4254^†	(2.5±0.5)e+0	16.5	(8.3±1.7)e+22	−0.77 ± 0.10^a
NGC 4289	(1.5±0.4)e−2	16.5	(4.8±1.2)e+20	−0.53 ± 0.12^b
NGC 4294	(8.6±1.7)e−2	16.5	(2.8±0.6)e+21	−0.51 ± 0.10^b
NGC 4298	(1.3±0.3)e−1	16.5	(4.2±0.8)e+21	−0.88 ± 0.10^d
NGC 4302^†	(2.5±0.5)e−1	16.5	(8.0±1.6)e+21	−0.77 ± 0.10^a
NGC 4303	(2.0±0.4)e+0	16.5	(6.5±1.3)e+22	−0.67 ± 0.10^a
NGC 4307	(9.5±2.1)e−3	23.0	(6.0±1.4)e+20	−0.57 ± 0.14^a
NGC 4312	(3.6±0.7)e−2	16.5	(1.2±0.2)e+21	−0.50 ± 0.10^a
NGC 4316	(2.1±0.4)e−2	23.0	(1.3±0.3)e+21	−0.54 ± 0.10^c
NGC 4321	(1.5±0.3)e+0	16.5	(4.9±1.0)e+22	−0.74 ± 0.10^d
NGC 4330^†	(5.6±1.1)e−2	16.5	(1.8±0.4)e+21	−0.63 ± 0.11^a
NGC 4343	(4.2±0.9)e−2	23.0	(2.7±0.5)e+21	−1.01 ± 0.11^b
IC 3258^†	(9.8±2.1)e−3	16.5	(3.2±0.7)e+20	< − 0.74^a
NGC 4351	(2.0±0.4)e−2	16.5	(6.5±1.3)e+20	< − 1.03^a
IC 3268	(8.0±1.9)e−3	23.0	(5.1±1.2)e+20	−0.26 ± 0.12^a
NGC 4359	(1.1±0.2)e−2	17.9	(4.2±0.7)e+20	< − 0.77^a
NGC 4370	(1.1±0.2)e−2	23.0	(6.8±1.5)e+20	< − 0.77^a
NGC 4376	(5.0±1.4)e−3	23.0	(3.1±0.9)e+20	< − 0.43^b
NGC 4380	(2.0±0.4)e−2	23.0	(1.2±0.3)e+21	< − 0.68^a
NGC 4383	(1.2±0.2)e−1	16.5	(3.9±0.8)e+21	−0.45 ± 0.10^a
VCC 827	(5.1±1.1)e−2	23.0	(3.2±0.7)e+21	−0.59 ± 0.10^a
NGC 4390	(1.8±0.4)e−2	23.0	(1.1±0.2)e+21	< − 0.98^d
IC 3322	(1.9±0.4)e−2	23.0	(1.2±0.3)e+21	−0.79 ± 0.12^d
NGC 4396^†	(9.6±1.9)e−2	16.5	(3.1±0.6)e+21	−0.79 ± 0.10^a
NGC 4402^†	(4.3±0.9)e−1	16.5	(1.4±0.3)e+22	−0.81 ± 0.10^a
NGC 4413	(8.8±1.9)e−3	16.5	(2.9±0.6)e+20	< − 0.68^a
NGC 4412	(4.0±0.9)e−2	16.5	(1.3±0.3)e+21	−0.44 ± 0.11^d
NGC 4416	(1.8±0.4)e−2	16.5	(6.0±1.3)e+20	−0.57 ± 0.11^a
NGC 4424^†	(3.0±0.6)e−2	23.0	(1.9±0.4)e+21	−0.67 ± 0.11^a
NGC 4430	(2.5±0.5)e−2	23.0	(1.6±0.3)e+21	−0.57 ± 0.10^b
VCC 1091	(6.1±1.4)e−3	23.0	(3.9±0.9)e+20	−0.25 ± 0.12^a
NGC 4450	(4.3±0.9)e−2	16.5	(1.4±0.3)e+21	−0.71 ± 0.10^a
NGC 4451	(2.1±0.4)e−2	23.0	(1.3±0.3)e+21	−0.52 ± 0.10^b
IC 3392	(8.2±1.8)e−3	16.5	(2.7±0.6)e+20	−0.44 ± 0.13^a
NGC 4457	(8.0±1.7)e−2	16.5	(2.6±0.5)e+21	−0.45 ± 0.10^a
NGC 4470	(2.1±0.4)e−2	16.5	(7.0±1.4)e+20	−0.14 ± 0.10^a
NGC 4480	(2.2±0.5)e−2	16.5	(7.1±1.6)e+20	−0.86 ± 0.13^a
NGC 4491	(7.5±2.0)e−3	16.5	(2.4±0.7)e+20	< − 0.61^a
NGC 4505	(2.7±0.6)e−2	16.5	(8.7±2.0)e+20	< − 1.15^d
IC 797	(1.1±0.2)e−2	16.5	(3.6±0.8)e+20	< − 0.78^a
NGC 4501^†	(1.8±0.4)e+0	16.5	(6.0±1.2)e+22	−0.75 ± 0.10^a
IC 3476^†	(5.0±1.0)e−2	16.5	(1.6±0.3)e+21	−0.81 ± 0.10^c
NGC 4519	(6.4±1.3)e−2	16.5	(2.1±0.4)e+21	−0.83 ± 0.10^a
NGC 4522^†	(8.1±1.6)e−2	16.5	(2.6±0.5)e+21	−0.48 ± 0.10^a
NGC 4525	(2.1±0.4)e−3	16.77	(7.2±1.4)e+19	< − 0.07^d
IC 800^†	(1.1±0.2)e−2	16.5	(3.5±0.8)e+20	< − 0.76^b
NGC 4532	(5.0±1.0)e−1	16.5	(1.6±0.3)e+22	−0.63 ± 0.10^a
NGC 4535	(6.4±1.3)e−1	16.5	(2.1±0.4)e+22	−0.96 ± 0.10^a
IC 3521	(2.6±0.5)e−2	16.5	(8.3±1.7)e+20	−0.84 ± 0.12^b
NGC 4540	(1.4±0.3)e−2	16.5	(4.5±1.0)e+20	−0.64 ± 0.12^a
NGC 4548^†	(1.1±0.2)e−1	16.5	(3.7±0.8)e+21	−1.32 ± 0.10^b
NGC 4565	(8.6±1.7)e−1	17.61	(3.2±0.6)e+22	−0.80 ± 0.10^b
NGC 4567	(7.1±1.4)e−2	16.5	(2.3±0.5)e+21	−0.76 ± 0.10^c
NGC 4568	(5.8±1.2)e−1	16.5	(1.9±0.4)e+22	−0.60 ± 0.10^c
NGC 4569^†	(5.5±1.1)e−1	16.5	(1.8±0.4)e+22	−0.55 ± 0.10^c
NGC 4579	(6.5±1.3)e−1	16.5	(2.1±0.4)e+22	−0.59 ± 0.10^a
NGC 4580	(1.2±0.3)e−2	16.5	(3.8±0.9)e+20	< − 0.79^b
NGC 4595	(9.6±2.2)e−3	16.5	(3.1±0.7)e+20	−0.31 ± 0.12^b
NGC 4606	(8.9±2.1)e−3	16.5	(2.9±0.7)e+20	< − 0.68^a
NGC 4607^†	(9.8±2.0)e−2	16.5	(3.2±0.6)e+21	−0.70 ± 0.10^a
NGC 4630	(2.4±0.5)e−2	16.5	(7.9±1.7)e+20	−0.28 ± 0.10^a
NGC 4634^†	(1.5±0.3)e−1	16.5	(5.0±1.0)e+21	−0.66 ± 0.10^a
NGC 4639	(3.7±0.8)e−2	16.5	(1.2±0.3)e+21	−0.68 ± 0.10^b
NGC 4647	(3.0±0.6)e−1	16.5	(9.8±2.0)e+21	−0.92 ± 0.10^a
NGC 4654^†	(8.5±1.7)e−1	16.5	(2.8±0.6)e+22	−0.87 ± 0.10^a
NGC 4689	(1.4±0.3)e−1	16.5	(4.6±0.9)e+21	−1.15 ± 0.10^a
NGC 4725	(1.8±0.3)e−1	17.27	(6.4±1.0)e+21	−0.79 ± 0.08^a
NGC 4747	(1.6±0.3)e−2	16.84	(5.4±0.9)e+20	−0.33 ± 0.08^a
NGC 4746	(1.8±0.4)e−1	16.5	(5.9±1.2)e+21	−0.52 ± 0.10^a
NGC 4758	(6.7±1.5)e−3	16.5	(2.2±0.5)e+20	−0.34 ± 0.13^a
NGC 4779	(2.6±0.5)e−2	16.5	(8.4±1.8)e+20	−0.49 ± 0.10^a
NGC 5014	(3.2±0.5)e−2	16.23	(10.0±1.5)e+20	−0.44 ± 0.08^a
NGC 5145	(1.3±0.2)e−1	17.5	(4.7±0.7)e+21	−0.58 ± 0.08^a
IC 902	(2.1±0.3)e−2	22.97	(1.3±0.2)e+21	−0.46 ± 0.08^a
NGC 5248	(5.4±1.1)e−1	16.46	(1.8±0.4)e+22	−0.58 ± 0.10^a
NGC 5301	(7.2±1.1)e−2	21.54	(4.0±0.6)e+21	−0.63 ± 0.08^a
NGC 5303	(7.4±1.1)e−2	20.27	(3.6±0.5)e+21	−0.46 ± 0.08^a
HRS 300	(3.0±0.6)e−3	19.34	(1.4±0.3)e+20	< − 0.22^a
NGC 5372	(5.2±0.8)e−2	24.53	(3.7±0.6)e+21	−0.51 ± 0.08^a
NGC 5486	(9.5±1.5)e−3	19.76	(4.4±0.7)e+20	< − 0.71^a
HRS 315	(3.2±0.7)e−3	20.57	(1.6±0.4)e+20	< − 0.24^a
NGC 5645	(4.1±0.9)e−2	19.57	(1.9±0.4)e+21	−0.44 ± 0.10^a
NGC 5669	(2.6±0.5)e−2	19.54	(1.2±0.2)e+21	−0.38 ± 0.10^a
NGC 5692	(3.0±0.6)e−2	22.59	(1.8±0.4)e+21	−0.68 ± 0.10^a

Notes. Column (1) lists the galaxy names, objects that are marked with a dagger symbol are in the RPS sample. Column (2) shows the LOFAR flux density measured at 20″ resolution, column (3) the distance (taken form Boselli et al. 2010 for objects outside the Virgo cluster, otherwise assumed to be 16.5 Mpc), column (4) the 144 MHz luminosity and column (5) the spectral index between 144 MHz and 1.4 GHz. The 1.4 GHz flux densities (or upper limits) are taken from ^aBoselli et al. (2015); ^b measured from the maps of Chung et al. (2009); ^cMurphy et al. (2009) and ^dVollmer et al. (2010).

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