The coordinated radio and infrared survey for high-mass star formation - III. A catalogue of northern ultra-compact H II regions

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Volume 615 (July 2018)

A&A, 615 (2018) A103

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Table 1

Comparison of a few MAGPIS flux values in the published 6–20 cm catalogue table (5th and 8th columns) with the measured flux values presented in this work – as from the automated script (3rd and 6th columns) and individual measurements with CASA (4th and 6th columns).

CORNISH name	F_C	F_{M6 cm}	F_{M6 cm}	F_{M6 cm}	F_{M20 cm}	F_{M20 cm}	F_{M20 cm}
	(cat.)	(ap.)	(CASA)	(cat.)	(ap.)	(CASA)	(cat.)
G011.1104−00.3985	305.37 ± 28.55	303.63 ± 9.12	320.3	112.37	326.73 ± 3.86	370.91	187.21
G012.1988−00.0345	62.71 ± 5.92	102.95 ± 1.47	110.18	59.82	42.52 ± 1.34	48.00	62.05
G016.3913−00.1383^‡	124.27 ± 15.43	43.18 ± 3.61	42.89	20.34	57.52 ± 5.18	66.71	58.23
G018.7106+00.0002	107.46 ± 10.62	177.74 ± 1.71	188.78	102.96	36.60 ± 0.94	41.97	35.39
G021.8751+00.0075	566.73 ± 54.14	1064.73 ± 8.85	1073.00	264.32	685.90 ± 7.84	719.53	599.63
G037.8731−00.3996	2561.21 ± 234.04	5189.35 ±23.38	5219.50	1518.5	1769.56 ± 6.57	1800.10	1279.40

Notes. Only highly-reliable values (based on median sky values and no overlapping sources) are compared in the table. All values are in mJy. The second column includes the corresponding CORNISH fluxes. The source denoted by ‡ could be intrinsically variable at 6 cm.

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