Field l = 9.6° ,b = 0°. Top: UKIDSS CMD. In green the red clump track corresponding to our results with its 1σ confidence interval, in blue the Marshall et al. (2006) results, in green the Lallement et al. (2019) ones. Middle: extinction, 1σ confidence interval in grey (see Fig. 8). Dotted line: FEDReD result using the isochrone HRD. Thin black line: isocontours of the spectroscopic sample results of Babusiaux et al. (2014). Bottom: stellar density. The bar distance determined by Babusiaux & Gilmore (2005) is indicated with a red line and the distance spread in light red.