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Fig. 10.

image

Normalization A of the LXT relation (top) and statistical significance of the deviation of every sky region compared to the rest of the sky (bottom) as functions of the position in the extragalactic sky for θ = 75° when only the 246 clusters with T >  2.5 keV and z >  0.03 are used, as well as CMB frame redshifts.

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