Best-fit normalization A of the LX–T relation for every sky region over Aall as a function of the Galactic longitude. The 1σ (68.3%) uncertainties are also shown. The results correspond to this work’s sample (top left), ACC (top right), this work’s sample excluding all the common clusters with ACC and XCS-DR1 (bottom left) and XCS-DR1 (bottom right).
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