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Table A.2

Results of the spectroscopic analysis of our program stars

Star Teff, K log g Vt , km s−1 [Fe/H] [O/H] [S/H] RG , kpc
ASAS J052610+1151.3 5810±70 1.75 3.5 –0.16±0.15 –0.24±0.15 –0.30±0.15 11.46±0.22
ASAS J061022+1438.6 6160±75 1.60 4.2 –0.09±0.15 –0.10±0.12 –0.12±0.15 11.09±0.14
ASAS J062840+0738.9 6270±110 2.00 2.7 –0.51±0.17 –0.42±0.12 –0.52±0.20 11.58±0.23
ASAS J063011+0751.2 6190±90 2.10 4.0 –0.25±0.18 –0.31±0.15 –0.36±0.20 12.05±0.23
ASAS J063519+2117.8 6230±200 2.00 3.9 –0.42±0.17 –0.27±0.15 –0.48±0.20 10.98±0.21
ASAS J064220-0318.9 6160±120 2.10 3.0 –0.23±0.17 –0.13±0.15 –0.24±0.25 12.17±0.42
ASAS J064220-0318.9 6100±120 1.90 3.4 –0.29±0.20 –0.26±0.18 –0.32±0.25
ASAS J065759-0159.7 5930±80 1.70 3.3 –0.42±0.17 –0.31±0.12 –0.35±0.15 12.51±0.36
ASAS J065759-0159.7 6080±80 1.90 3.3 –0.34±0.17 –0.27±0.12 –0.30±0.15
ASASSN-V J074310.73-113457.7 6300±150 2.00 3.3 –0.55±0.20 –0.22±0.20 –0.45±0.25 11.82±0.29
AU Cas 5790±80 1.60 4.7 –0.16±0.13 –0.05±0.13 –0.12±0.15 11.57±0.25
DP Mon 5720±90 1.85 3.8 –0.48±0.13 –0.34±0.12 –0.55±0.25 12.81±0.48
DP Mon 5800±90 2.00 3.8 –0.48±0.15 –0.34±0.12 –0.55±0.25
DT Cas 5600±70 1.70 4.2 –0.14±0.22 –0.21±0.13 –0.24±0.17 10.44±0.15
DT Gem 6300±100 2.50 3.5 –0.30±0.15 –0.19±0.12 –0.41±0.17 11.97±0.31
FL CMa 5650±100 1.75 3.3 –0.50±0.15 –0.40±0.12 –0.45±0.20 15.16±1.14
FL CMa 5835±100 2.00 3.2 –0.32±0.13 –0.43±0.12 –0.45±0.20
GI CMa 5850±60 1.70 2.9 –0.29±0.13 –0.34±0.10 –0.35±0.12 12.26±0.38
KO Cep 5900±130 1.65 4.0 –0.19±0.16 +0.09±0.20 –0.06±0.15 10.41±0.23
KO Cep 6100±110 1.50 4.2 –0.12±0.30 –0.07±0.15 –0.12±0.15
OR Cam 6140±90 2.00 4.0 –0.02±0.17 –0.12±0.13 –0.16±0.15 9.39 ±0.04
UCAC4 738-091921 5925±60 1.60 3.2 –0.16±0.17 –0.21±0.13 –0.22±0.15 11.14±0.27
V1016 Cas 5760±50 1.60 3.6 –0.22±0.12 –0.39±0.13 –0.29±0.12 12.12±0.28
V1543 Cyg 6085±70 2.00 3.0 –0.25±0.15 –0.21±0.12 –0.22±0.15 8.56 ±0.03
V2340 Cyg 5470±60 1.50 4.4 –0.04±0.20 –0.19±0.15 –0.09±0.15 8.96 ±0.06
V371 Gem 6350±80 1.65 3.4 –0.31±0.17 –0.14±0.12 –0.26±0.17 11.22±0.16
V394 Cep 5850±150 1.50 2.8 –0.40±0.23 –0.39±0.18 –0.32±0.17 16.13±1.68
V394 Cep 5800±150 1.70 2.8 –0.30±0.20 –0.18±0.25 –0.24±0.17
V432 Ori 6200±70 1.75 3.7 –0.30±0.14 –0.27±0.12 –0.29±0.15 12.24±0.44
V470 Cas 6300±100 2.45 3.5 –0.38±0.17 –0.30±0.10 –0.34±0.17 10.51±0.15
V553 Cas 5685±80 1.40 4.5 –0.15±0.32 –0.35±0.15 –0.24±0.15 11.32±0.24
V553 Cas 5570±100 1.45 4.5 –0.21±0.17 –0.27±0.20 –0.26±0.15
V598 Per 5550±70 1.75 3.8 –0.12±0.17 –0.11±0.15 –0.18±0.15 10.04±0.09
V824 Cas 5905±60 1.50 3.4 –0.12±0.12 –0.25±0.15 –0.20±0.12 10.27±0.10
V824 Cas 6090±80 1.60 4.2 –0.14±0.19 –0.12±0.19 –0.26±0.18 10.27±0.10
V827 Cas 5975±60 1.80 2.9 –0.12±0.17 –0.26±0.12 –0.15±0.12 10.34±0.12
V827 Cas 6160±70 1.50 3.2 –0.12±0.17 –0.33±0.12 –0.20±0.15 10.34±0.12
V836 Cas 6245±80 2.00 3.2 –0.23±0.15 –0.21±0.15 –0.26±0.17 10.81±0.16
V892 Per 6070±70 1.80 3.7 –0.07±0.15 –0.25±0.15 –0.16±0.15 10.67±0.17
V892 Per 5910±70 1.70 3.7 –0.13±0.17 –0.17±0.15 –0.21±0.15
V908 Cep 6300±100 2.00 3.7 –0.19±0.11 –0.14±0.15 –0.20±0.15 9.71 ±0.09
V913 Mon 5860±90 1.70 2.2 –0.42±0.17 –0.46±0.12 –0.57±0.15 11.64±0.32
V913 Mon 5955±85 2.00 2.6 –0.33±0.15 –0.43±0.12 –0.48±0.17
XZ CMa 5815±60 1.90 3.2 –0.48±0.16 –0.41±0.12 –0.52±0.18 12.41±0.42
AI CMa 5740±60 1.85 3.7 –0.34±0.14 –0.45±0.17 18.17±2.19
AL CMa 6400±150 2.45 3.9 –0.54±0.10 –0.64±0.25 18.15±2.36
AL CMa 5880±80 2.35 4.2 –0.46±0.15 –0.56±0.18
AM CMa 5800±60 1.80 2.8 –0.40±0.12 –0.54±0.15 22.11±4.42
BY CMa 5780±70 1.90 3.5 –0.43±0.12 –0.47±0.20 13.90±0.90
CM Pup 6015±65 1.80 2.1 –0.29±0.12 –0.46±0.15 14.30±0.90
CP CMa 6175±80 1.50 3.0 –0.36±0.12 –0.48±0.18 14.38±0.87
CV Ori 6470±75 1.55 1.9 –0.07±0.12 –0.26±0.15 11.28±0.26
ET CMa 6100±80 1.50 1.8 –0.31±0.12 –0.52±0.12 12.56±0.62
FP CMa 6065±60 1.70 2.1 –0.54±0.12 –0.52±0.18 16.79±1.83
ASAS J071705-2849.4 6095±50 2.00 3.0 –0.44±0.12 –0.62±0.20 13.60±0.56
V1819 Ori 6300±150 2.00 3.7 –0.50±0.14 –0.70±0.20 14.02±0.72
V336 Ori 5760±50 1.95 4.0 –0.22±0.17 –0.35±0.20 14.68±0.78
V390 CMa 5550±70 1.40 3.2 –0.39±0.12 –0.36±0.18 13.35±0.66
V418 CMa 6105±65 2.00 2.5 –0.47±0.12 –0.47±0.20 15.02±0.93
V423 CMa 6215±55 2.25 2.3 –0.32±0.12 –0.56±0.18 12.85±0.61
V434 CMa 5855±70 1.30 2.5 –0.05±0.15 –0.26±0.15 12.24±0.34
VW Mon 5960±75 2.20 2.2 –0.20±0.12 –0.26±0.17 13.11±0.53
WY CMa 6255±60 2.00 2.0 –0.43±0.12 –0.50±0.17 13.80±0.64

Remark: errors in galactocentric distances were estimated taking into account the errors in heliocentric distances.

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