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Table 5:

Distribution of the red-clump parameters.

Freq.
$\char93 $ of $R/R_\odot$ $M/ M_\odot$ $L / L_\odot$ $T_{{\rm eff}}$
($\mu $Hz) stars       (K)
28-32 146 $10.0_{\rm -1.3}^{+1.1}$ $1.00_{\rm -0.18}^{+0.19}$ $38.5_{\rm -10.0}^{+9.7} $ $4510_{\rm -180}^{+170} $
  LRc01 $10.1_{\rm -0.7}^{+0.7}$ $1.01_{\rm -0.15}^{+0.17}$ $39.0_{\rm -7.0 }^{+9.5} $ $4530_{\rm -150}^{+140} $
  LRa01 $9.8_{\rm -0.6}^{+0.7}$ $0.98_{\rm -0.12}^{+0.20}$ $38.1_{\rm -7.0 }^{+8.5} $ $4480_{\rm -100}^{+120} $
           
37-43 137 $10.3_{\rm -0.7}^{+1.1}$ $1.34_{\rm -0.18}^{+0.25}$ $42.4_{\rm - 8.3}^{+11.2}$ $4580_{\rm -170}^{+140} $
  LRc01 $10.3_{\rm -0.7}^{+0.8}$ $1.33_{\rm -0.15}^{+0.22}$ $42.1_{\rm - 7.8}^{+9.4}$ $4580_{\rm -140}^{+130} $
  LRa01 $10.4_{\rm -0.6}^{+1.2}$ $1.36_{\rm -0.19}^{+0.28}$ $42.7_{\rm - 7.3}^{+8.3}$ $4590_{\rm -150}^{+120} $

Notes. The 2nd column gives first the total number of targets considered in each region of the clump, then indicates which field is considered.
The following columns present the main values of the stellar parameters and the dispersion in their distribution in each region.


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