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 1

VLA observations.

Epoch	Starting time	Initial API rms	Projected baseline
	(UTC)	(°)	(m)	(Jy)
1	2016-12-02 21:31	11	310–34 300	1.4
2	2016-12-05 21:18	6.0	460–34 300	1.3
3	2017-01-06 18:05	13	325–32 800	1.4
4	2017-01-14 18:40	13	310–34 300	1.3
5	2017-01-22 17:12	4.4	665–33 100	1.3

Notes. API refers to Atmospheric Phase Interferometer, which observes an 11.7 GHz beacon from a geostationary satellite with a 300 meters baseline. is the measured flux of the gain calibrator J1625-2527.

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