Comparison of total and imaged power for IRS 1 and IRS 3 together. Bottom: Total power spectrum for a roughly ±1^{﹩\arcmin﹩} field around NGC 2071IR (solid line) and a channel‐by‐channel sum of the peak flux density for each detected and fitted maser feature (dashed line) for 1996 March 24. Top: Ratio of the imaged and total power, which cannot exceed unity.