Table D1

Candidates for thick disc RR Lyrae and BHB stars with distances (D) within 2 kpc.

D < 1 kpc star[Fe/H]SEcc.zmaxLLz1 < D < 2 kpc star[Fe/H]SEcc.zmaxLLz
RR LYRAE:RR LYRAE:
FW LUP−0.20(1)0.060.130681607CN LYR−0.58(1)0.160.32661846
KX LYR−0.46(2)0.310.410691561CG PEG−0.50(1)0.030.39871736
DX DEL−0.50(1)0.220.230731594HH PUP−0.50(1)0.120.351221815
SW DRA−1.12(1)0.420.711071176ST OPH−1.30(2)0.100.561291514
AV PEG−0.36(1)0.270.391291287TW HER−0.88(1)0.130.611391796
v494 SCO−1.01(2)0.120.211381548SS CNC−0.56(1)0.180.831592009
RS BOO−0.62(1)0.170.941911971TW LYN−0.66(1)0.212.131702276
SW AND−0.41(1)0.130.471931692TZ AQR−1.24(1)0.201.391931200
DH PEG−1.24(2)0.270.522071338Z MIC−1.10(1)0.391.252101196
AR PER−0.57(1)0.060.402261987UW OCT−0.49(2)0.471.582101170
UY CYG−0.95(1)0.110.232401630EZ LYR−1.29(1)0.420.651761309
AN SER−0.39(1)0.100.842451440RR LEO−1.51(1)0.381.042181256
v690 SCO−1.16(2)0.190.482481405RR GEM−0.55(1)0.180.732252152
DM CYG−0.57(1)0.130.482051890AA CMI−0.15(1)0.090.432251978
XZ DRA−0.89(1)0.100.682991746AV SER−1.20(3)0.110.862301605
v445 OPH−0.19(2)0.110.813881419RW ARI−1.16(2)0.261.442381639
T SEX−1.33(1)0.301.184311255U PIC−0.72(1)0.091.012421885
UU VIR−0.87(2)0.521.714391142BS APS−1.33(2)0.301.122641852
RX ERI−1.33(1)0.001.676281654CP AQR−0.77(1)0.311.072781308
W CVN−1.22(1)0.292.476431132RW DRA−1.55(2)0.601.112801100
RW TRA−0.13(1)0.140.783211605
BHB:AT SER−2.03(1)0.161.473801137
HD 4850−1.18(4)3571311BR AQR−0.74(1)0.111.654261473
HD 8376−2.82(4)5011173VV PEG−1.88(2)0.262.554951575
BD +01 0548−2.23(4)2991794RV SEX−1.10(2)0.402.145511226
BO AQR−1.80(2)0.461.822571159
D < 1 kpc star[Fe/H]SEcc.zmaxLLz1 < D < 2 kpc star[Fe/H]SEcc.zmaxLLz
RR LYRAE:RR LYRAE:
FW LUP−0.20(1)0.060.130681607CN LYR−0.58(1)0.160.32661846
KX LYR−0.46(2)0.310.410691561CG PEG−0.50(1)0.030.39871736
DX DEL−0.50(1)0.220.230731594HH PUP−0.50(1)0.120.351221815
SW DRA−1.12(1)0.420.711071176ST OPH−1.30(2)0.100.561291514
AV PEG−0.36(1)0.270.391291287TW HER−0.88(1)0.130.611391796
v494 SCO−1.01(2)0.120.211381548SS CNC−0.56(1)0.180.831592009
RS BOO−0.62(1)0.170.941911971TW LYN−0.66(1)0.212.131702276
SW AND−0.41(1)0.130.471931692TZ AQR−1.24(1)0.201.391931200
DH PEG−1.24(2)0.270.522071338Z MIC−1.10(1)0.391.252101196
AR PER−0.57(1)0.060.402261987UW OCT−0.49(2)0.471.582101170
UY CYG−0.95(1)0.110.232401630EZ LYR−1.29(1)0.420.651761309
AN SER−0.39(1)0.100.842451440RR LEO−1.51(1)0.381.042181256
v690 SCO−1.16(2)0.190.482481405RR GEM−0.55(1)0.180.732252152
DM CYG−0.57(1)0.130.482051890AA CMI−0.15(1)0.090.432251978
XZ DRA−0.89(1)0.100.682991746AV SER−1.20(3)0.110.862301605
v445 OPH−0.19(2)0.110.813881419RW ARI−1.16(2)0.261.442381639
T SEX−1.33(1)0.301.184311255U PIC−0.72(1)0.091.012421885
UU VIR−0.87(2)0.521.714391142BS APS−1.33(2)0.301.122641852
RX ERI−1.33(1)0.001.676281654CP AQR−0.77(1)0.311.072781308
W CVN−1.22(1)0.292.476431132RW DRA−1.55(2)0.601.112801100
RW TRA−0.13(1)0.140.783211605
BHB:AT SER−2.03(1)0.161.473801137
HD 4850−1.18(4)3571311BR AQR−0.74(1)0.111.654261473
HD 8376−2.82(4)5011173VV PEG−1.88(2)0.262.554951575
BD +01 0548−2.23(4)2991794RV SEX−1.10(2)0.402.145511226
BO AQR−1.80(2)0.461.822571159

†Sources of [Fe/H]: (1) Feast et al. (2008); (2) Beers et al. (2000); (3) Layden (1994); (4) Kinman et al. (2009).

The orbital eccentricity (Ecc.) and the maximum height in kpc above the Galactic plane (zmax) are taken from Maintz & de Boer (2005). L and Lz are in units of kpc km s−1.

Table D1

Candidates for thick disc RR Lyrae and BHB stars with distances (D) within 2 kpc.

D < 1 kpc star[Fe/H]SEcc.zmaxLLz1 < D < 2 kpc star[Fe/H]SEcc.zmaxLLz
RR LYRAE:RR LYRAE:
FW LUP−0.20(1)0.060.130681607CN LYR−0.58(1)0.160.32661846
KX LYR−0.46(2)0.310.410691561CG PEG−0.50(1)0.030.39871736
DX DEL−0.50(1)0.220.230731594HH PUP−0.50(1)0.120.351221815
SW DRA−1.12(1)0.420.711071176ST OPH−1.30(2)0.100.561291514
AV PEG−0.36(1)0.270.391291287TW HER−0.88(1)0.130.611391796
v494 SCO−1.01(2)0.120.211381548SS CNC−0.56(1)0.180.831592009
RS BOO−0.62(1)0.170.941911971TW LYN−0.66(1)0.212.131702276
SW AND−0.41(1)0.130.471931692TZ AQR−1.24(1)0.201.391931200
DH PEG−1.24(2)0.270.522071338Z MIC−1.10(1)0.391.252101196
AR PER−0.57(1)0.060.402261987UW OCT−0.49(2)0.471.582101170
UY CYG−0.95(1)0.110.232401630EZ LYR−1.29(1)0.420.651761309
AN SER−0.39(1)0.100.842451440RR LEO−1.51(1)0.381.042181256
v690 SCO−1.16(2)0.190.482481405RR GEM−0.55(1)0.180.732252152
DM CYG−0.57(1)0.130.482051890AA CMI−0.15(1)0.090.432251978
XZ DRA−0.89(1)0.100.682991746AV SER−1.20(3)0.110.862301605
v445 OPH−0.19(2)0.110.813881419RW ARI−1.16(2)0.261.442381639
T SEX−1.33(1)0.301.184311255U PIC−0.72(1)0.091.012421885
UU VIR−0.87(2)0.521.714391142BS APS−1.33(2)0.301.122641852
RX ERI−1.33(1)0.001.676281654CP AQR−0.77(1)0.311.072781308
W CVN−1.22(1)0.292.476431132RW DRA−1.55(2)0.601.112801100
RW TRA−0.13(1)0.140.783211605
BHB:AT SER−2.03(1)0.161.473801137
HD 4850−1.18(4)3571311BR AQR−0.74(1)0.111.654261473
HD 8376−2.82(4)5011173VV PEG−1.88(2)0.262.554951575
BD +01 0548−2.23(4)2991794RV SEX−1.10(2)0.402.145511226
BO AQR−1.80(2)0.461.822571159
D < 1 kpc star[Fe/H]SEcc.zmaxLLz1 < D < 2 kpc star[Fe/H]SEcc.zmaxLLz
RR LYRAE:RR LYRAE:
FW LUP−0.20(1)0.060.130681607CN LYR−0.58(1)0.160.32661846
KX LYR−0.46(2)0.310.410691561CG PEG−0.50(1)0.030.39871736
DX DEL−0.50(1)0.220.230731594HH PUP−0.50(1)0.120.351221815
SW DRA−1.12(1)0.420.711071176ST OPH−1.30(2)0.100.561291514
AV PEG−0.36(1)0.270.391291287TW HER−0.88(1)0.130.611391796
v494 SCO−1.01(2)0.120.211381548SS CNC−0.56(1)0.180.831592009
RS BOO−0.62(1)0.170.941911971TW LYN−0.66(1)0.212.131702276
SW AND−0.41(1)0.130.471931692TZ AQR−1.24(1)0.201.391931200
DH PEG−1.24(2)0.270.522071338Z MIC−1.10(1)0.391.252101196
AR PER−0.57(1)0.060.402261987UW OCT−0.49(2)0.471.582101170
UY CYG−0.95(1)0.110.232401630EZ LYR−1.29(1)0.420.651761309
AN SER−0.39(1)0.100.842451440RR LEO−1.51(1)0.381.042181256
v690 SCO−1.16(2)0.190.482481405RR GEM−0.55(1)0.180.732252152
DM CYG−0.57(1)0.130.482051890AA CMI−0.15(1)0.090.432251978
XZ DRA−0.89(1)0.100.682991746AV SER−1.20(3)0.110.862301605
v445 OPH−0.19(2)0.110.813881419RW ARI−1.16(2)0.261.442381639
T SEX−1.33(1)0.301.184311255U PIC−0.72(1)0.091.012421885
UU VIR−0.87(2)0.521.714391142BS APS−1.33(2)0.301.122641852
RX ERI−1.33(1)0.001.676281654CP AQR−0.77(1)0.311.072781308
W CVN−1.22(1)0.292.476431132RW DRA−1.55(2)0.601.112801100
RW TRA−0.13(1)0.140.783211605
BHB:AT SER−2.03(1)0.161.473801137
HD 4850−1.18(4)3571311BR AQR−0.74(1)0.111.654261473
HD 8376−2.82(4)5011173VV PEG−1.88(2)0.262.554951575
BD +01 0548−2.23(4)2991794RV SEX−1.10(2)0.402.145511226
BO AQR−1.80(2)0.461.822571159

†Sources of [Fe/H]: (1) Feast et al. (2008); (2) Beers et al. (2000); (3) Layden (1994); (4) Kinman et al. (2009).

The orbital eccentricity (Ecc.) and the maximum height in kpc above the Galactic plane (zmax) are taken from Maintz & de Boer (2005). L and Lz are in units of kpc km s−1.

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