Correlates optical and X-ray selected galaxy clusters, highlighting their similarities and differences.
Context. This paper is the first in a series undertaking a comprehensive correlation analysis between optically selected and X-ray-selected cluster catalogues. The rationale of the project is to develop a holistic picture of galaxy clusters utilising optical and X-ray-cluster-selected catalogues with well-understood selection functions.
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Sadibekova et al. (2014) studied this question.
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