Left: best-fit normalization A of the LX–T relation for every sky region over Aall as a function of the position in the extragalactic sky when the slope B is left completely free to vary. The cone size used is θ = 75°. Right: LX–T relation for the 136 clusters within 75° from (l, b) ∼ (26°, −13°) (red) and for the 124 clusters within 75° from (l, b) ∼ (272°, −21°) (black). Their best-fit models are displayed as solid lines.
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