Extended Data Fig. 5: uv profile of the original and continuum subtracted data.
From: Sunyaev–Zeldovich detection of hot intracluster gas at redshift 4.3
The real part of the averaged amplitude measured from the continuum-subtracted measurement sets as a function of uv-distance with uv bins of 3kλ. The errorbars are derived from visibility weightings. The negative signal becomes stronger at a shorter uv distance, suggesting that the tSZ decrement can be limited by the uv-coverage of the ACA and ALMA observations.
