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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Table 2

Ratio of CORNISH to MAGPIS 5 GHz fluxes for candidate variable UCHII regions (observed 15 years apart).

CORNISH name	F_C∕F_{M,6 cm}
G011.0328+00.0274	2.42 ± 0.61
G011.9786−00.0973	3.56 ± 1.83
G014.5988+00.0198	2.92 ± 0.80
G016.3913−00.1383	2.88 ± 0.15
G023.4553−00.2010	17.42 ± 1.28
G025.7157+00.0487	4.33 ± 0.49
G030.7579+00.2042	73.85 ± 4.49
G030.7661−00.0348	7.04 ± 0.56
G037.7347−00.1128	22.90 ± 1.09

Notes. We note that in some cases, the source was not detected in MAGPIS, so the upper flux limit was used instead for the comparison.

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