Fig. 2.

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Coverage of ViCTORIA project surveys. In green are the pointings at mid-frequency FWHM of the MeerKAT Virgo Survey designed to fill the orange region covered by NGVS in optical and VESTIGE in H α. In light and dark blue are the coverages of LOFAR LBA and HBA, respectively (mid-frequency FWHM). The red dashed line is the estimated r200. The contours trace the X-ray emission from ROSAT (Böhringer et al. 1994), grey dots are VCC galaxies with recessional velocity ≤ 3000 km s−1, and red dots mark cluster galaxies that we expect to detect based on their H α-brightness.
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