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Fig. 6.


Best-fit normalization A (top) and slope B (bottom) of the LXT relation for every sky region over the best-fit results for the full sample (Aall and Ball) as functions of the Galactic longitude. The 1σ (68.3%) uncertainties are also shown. Every region covers a sky area of Δl = 90° and Δb = 180°. The x-axis values represent the central l value for every bin.

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