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Table A.1

Summary of strong correlations found for the stars analysed in clusters IC4651, IC4756, NGC2345, NGC2423, NGC3114, NGC3532, NGC3680, NGC4349 and NGC5822.

Star ρw(RV,BIS) ρw(RV,FWHM) ρw(RV,Teff) ρw(RV,Hα1.6Å) ρw(RV,Hα0.6Å) A(Li) [dex] Mass (M) υsin(i) (km s–1) n
IC4651No10393 –0.500 1.801 1.870 23
IC4651No11453 –0.007 2.699 1.750 33
IC4651No12935 × 0.315 1.800 0.000 5
IC4651No14527 –0.500 1.867 1.810 31
IC4651No6333 × × 1.209 1.779 2.130 5
IC4651No7646 –0.500 2.438 0.000 31
IC4651No8540 0.715 1.797 0.000 27
IC4651No9025 0.621 1.815 0.000 30
IC4651No9122 –0.500 1.795 0.680 74
IC4651No9791 1.277 1.750 1.850 33

IC4756No14 × × –0 016 1.973 2.030 5
IC4756No38 × 0.783 2.005 0.000 7
IC4756No44 × × 0.823 2.016 2.830 6
IC4756No52 × 1.447 2.272 2.870 16

NGC2345No50 × ×★ ×★ 0.977 5.843 5.270 26

NGC2423No3 ×★ 1.377 2.035 2.190 60
NGC2423No56 × 1 035 1.991 0.000 7

NGC3114No150 × 1.340 4.490 16.190 11
NGC3114No170 × × × × 1.503 3.981 11.320 6
NGC3114No181 × × 0.309 4.022 3.950 11
NGC3114No223 × –0.500 2.508 0.330 8
NGC3114No238 0.533 3.807 4.090 10
NGC3114No262 × 1.190 3.884 9.220 31
NGC3114No283 × 1.415 4.663 12.470 30
NGC3114No6 × 1.092 4.612 7.480 44

NGC3532No100 0.952 3.379 4 870 19
NGC3532No122 × 1.344 2.873 9.570 20
NGC3532No160 × × × × 1.125 3.149 4.780 8
NGC3532No19 1.443 3.218 5.050 46
NGC3532No221 × × × 0.186 4.818 5.890 22
NGC3532No522 × × × 1.202 4.412 12.480 6
NGC3532No596 × 1.153 3.126 7.210 31
NGC3532No670 × 1.475 3.047 4.640 29

NGC3680No13 × × × 1.252 1.659 0.280 7
NGC3680No26 1 192 1.704 0.960 18
NGC3680No34 0.246 1.752 3.010 12
NGC3680No41 0.633 1.641 0.000 18
NGC3680No44 × × × –0.500 1.690 2.550 6
NGC3680No53 1.211 1.652 0.120 18

NGC4349No127 1.375 3.007 4.810 56
NGC4349No168 1 000 3.358 5.510 35
NGC4349No174 × × 0.843 3.003 3.190 22
NGC4349No203 × 1.105 3.296 5.310 10
NGC4349No5 –0.500 3.134 7.270 35
NGC4349No9 × × 1.262 3.005 9.580 24

NGC5822No102 × × × × 1.348 2.020 5.830 5
NGC5822No1 0 126 2.274 3.120 8
NGC5822No201 1.009 2.422 1.600 23
NGC5822No240 1.401 2.071 2.830 7
NGC5822No316 × × × × 0.636 2.205 0.000 7
NGC5822No375 –0.076 2.142 2.190 19
NGC5822No443 × –0.138 2.111 1.830 8
NGC5822No8 0.431 2.262 0.360 36

Notes. Each cross represents a correlation with BIS, FWHM, Teff or Hα > 0.4. Highlighted in blue are every star in this part of the sample that can be considered Li-rich, and highlighted in purple are all stars with considerable rotation, that is, υ sin(i) > 5 km/s. ★ indicates that a significant peak was found for the GLSP of the respective quantity which also appeared in RV. Also in this table are the values of the mass for each star (M) as well as the number of points (n) used to calculate the correlations.

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