Fig. 2.
Continuum emission of the combined ALMA data on the EP Aqr system. Contours are drawn at 3, 6, 12, 24, 48 and 96 times the continuum rms noise value (σrms = 2.83 × 10−5 Jy beam−1). The offset position of the target with respect to the telescope pointing (ICRS 21:46:31.8475, −02:12:45.930) is due to transverse motion over the field of view. The ALMA beam is shown in the bottom right corner.
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