Deciphering the radio–star formation correlation on kpc scales - II. The integrated infrared–radio continuum and star formation–radio continuum correlations

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Volume 667 (November 2022)

A&A, 667 (2022) A30

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Table B.4.

High-z star-forming disk galaxies.

Galaxy Name	v_max^(c)	l_flat^(b)^(d)	l_*	M_*	Ṁ_∗	log(L_TIR)^(e)	Ṁ^(a)	M_gas^(a)
	(km s⁻¹)	(kpc)	(kpc)	(10¹⁰ M_⊙)	(M_⊙ yr⁻¹)	(L_⊙)	(M_⊙ yr⁻¹)	(10⁹ M_⊙)
EGS12004280	230	0.10	4.7	4.1	100	11.59	30.5	47.5
EGS12004754	215	0.10	6.5	9.3	53	11.48	5.8	39.2
EGS12007881	232	0.10	5.7	5.2	94	11.74	23.5	53.8
EGS12015684	233	0.10	4.0	4.6	113	12.24	30.5	41.3
EGS12023832	215	0.10	4.7	5.9	115	11.78	36.8	47.4
EGS12024462	253	0.10	8.6	6.0	78	11.99	12.9	73.5
EGS12024866	221	0.10	4.6	2.5	31	11.42	4.0	24.5
EGS13003805	387	0.10	5.7	17.0	200	12.11	9.7	70.9
EGS13004661	171	0.10	5.0	3.0	60	11.91	36.3	39.4
EGS13004684	295	0.10	5.0	11.0	42	11.30	1.4	27.7
EGS13011148	260	0.10	5.2	11.0	52	11.57	2.9	31.3
EGS13011155	296	0.10	7.8	12.0	201	11.77	35.2	106.5
EGS13011166	363	0.10	6.5	12.0	373	12.36	69.0	133.0
EGS13017614	346	0.10	4.5	13.0	88	11.73	2.9	36.0
EGS13017707	324	0.10	3.6	7.4	351	12.25	93.0	72.2
EGS13017843	227	0.10	4.2	4.0	35	11.36	3.3	22.2
EGS13017973	155	0.10	7.2	4.4	55	11.44	36.6	52.0
EGS13018632	319	0.10	1.9	5.2	82	12.01	3.9	15.1
EGS13019114	327	0.10	7.2	6.6	47	11.77	1.9	45.9
EGS13019128	194	0.10	5.2	4.4	87	11.67	39.6	48.1
EGS13026117	436	0.10	3.2	13.0	113	12.27	2.3	29.9
EGS13033624	301	0.10	5.3	8.9	148	-	17.0	59.6
EGS13033731	350	0.10	5.5	2.8	28	11.42	0.8	29.2
EGS13034339	299	0.10	3.0	6.6	86	12.28	5.4	24.4
EGS13034541	330	0.10	8.0	9.3	183	11.97	24.2	107.8
EGS13034542	195	0.10	4.0	5.2	61	11.58	11.9	26.7
EGS13035123	219	0.10	11.2	15.0	87	12.04	14.8	89.3
EGS13042293	167	0.10	5.2	3.9	55	11.79	24.2	36.0
zC406690	224	0.10	6.3	4.0	480	-	304.8	158.1
Q1623BX599	376	0.10	1.7	5.7	131	-	5.6	17.5
Q1700BX691	260	0.10	3.9	7.6	50	-	2.9	23.3
Q2343BX610	402	0.10	4.6	10.0	212	-	12.7	63.2
Q2343BX442	309	0.10	4.3	12.0	145	-	10.5	44.1
Q2343MD59	371	0.10	2.8	7.6	26	-	0.3	13.2
Q2346BX482se	285	0.10	2.4	0.6	34	-	3.9	15.8
BzK4171	261	0.10	4.5	4.0	101	-	20.2	45.4
BzK210000	292	0.10	4.7	7.8	231	-	54.3	72.2
BzK16000	258	0.10	4.0	4.3	82	-	11.9	34.4
BzK17999	238	0.10	4.7	3.9	450	-	351.0	122.8
BzK12591	361	0.10	4.5	11.0	267	-	26.7	69.4
BzK25536	254	0.10	3.0	3.3	62	-	7.4	22.2
J2135-0102	381	0.10	1.5	1.7	230	-	46.0	27.8

Notes.

^(a)

calculated quantities; the mean CO(1-0)–H₂ conversion factor is α_CO = 2.6 ± 0.9 M_⊙(K km s⁻¹ pc²)⁻¹ (Vollmer et al. 2017).

^(b)

assumed quantities; all other columns are input quantities from Tabatabaei et al. (2013).

^(c)

if the assumed rotation velocity is .

^(d)

A rotation curve of the form v_rot = v_max(1 − exp(−R/l_flat)) was assumed.

^(e)

From Barro et al. (2011). The mean conversion factor is Ṁ_∗/L_TIR = 1.4 10⁻¹⁰ M_⊙ yr⁻¹.

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