The SEDA method matches MeerKLASS radio sources to optical and infrared galaxies using measured offsets, stellar mass, and redshift, yielding about 82,000 counterpart identifications at roughly 95% expected purity.
N., Kauffmann, G., Heckman, T
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Optical Counterparts of MeerKLASS L-band and UHF-band surveys
The SEDA method matches MeerKLASS radio sources to optical and infrared galaxies using measured offsets, stellar mass, and redshift, yielding about 82,000 counterpart identifications at roughly 95% expected purity.