VLA cm-wave survey of young stellar objects in the Oph A cluster: constraining extreme UV- and X-ray-driven disk photoevaporation - A pathfinder for Square Kilometre Array studies

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Table 3

Comparison of fluxes (mJy) measured towards 3 YSOs with VLBA and VLA.

#	Source	VLBA⁽¹⁾	VLA⁽²⁾	VLBA⁽¹⁾	VLA⁽²⁾
		5 GHz	5 GHz	8 GHz	8 GHz
10	J162625.63-242 429.4	0.66	0.22	<0.12	0.20
13	J162616.85-242 223.5	0.15–0.47^(a)	0.34	…	0.36
18	J162622.39-242 253.4	0.30–0.38^(a)	2.02	<0.09	1.42

Notes. ^(a) The flux of these sources is known to vary.

References. ⁽¹⁾From Ortiz-Leónet al. (2017). ⁽²⁾From Dzib et al. (2013).

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