Table 5.
Open in new tab

Metallicity, reddening, averaged surface gravity, effective temperature, angular radius of the stars and the standard deviation of the averaged quantities.

|$[M/\text{H}]$|E(B − V)|$\overline{\log g_{\rm e}}$||$\overline{T_{\rm e}}$||$\overline{\vartheta \times 10^{11}}$|
(dex)(mag)(cm s−2)(K)(rad)
SW And, HJD-2444720 = 0, 1, 2, 3, 4
0.022.60 ± 0.356676 ± 42117.52 ± 0.68
HJD-2454350 = 0, 1, 3
0.100.022.85 ± 0.636610 ± 42817.31 ± 0.68
HJD-2454830 = −8, −1, 0, 1, 2
2.75 ± 0.446637 ± 39317.53 ± 0.65
SU Draa
−1.600.0152.72 ± 0.596743 ± 51216.68 ± 0.91
DH Peg
−0.350.08b2.86 ± 0.437413 ± 31216.90 ± 0.04
DY Peg
−0.050.03.41 ± 0.167157 ± 24610.60 ± 0.19
CU Com
−2.200.023.09 ± 0.516925 ± 3093.21 ± 0.12
V372 Serc
−0.530.0033.24 ± 0.366713 ± 3248.13 ± 0.16
V500 Hyac
−1.050.0083.69 ± 0.506902 ± 26110.17 ± 0.37
|$[M/\text{H}]$|E(B − V)|$\overline{\log g_{\rm e}}$||$\overline{T_{\rm e}}$||$\overline{\vartheta \times 10^{11}}$|
(dex)(mag)(cm s−2)(K)(rad)
SW And, HJD-2444720 = 0, 1, 2, 3, 4
0.022.60 ± 0.356676 ± 42117.52 ± 0.68
HJD-2454350 = 0, 1, 3
0.100.022.85 ± 0.636610 ± 42817.31 ± 0.68
HJD-2454830 = −8, −1, 0, 1, 2
2.75 ± 0.446637 ± 39317.53 ± 0.65
SU Draa
−1.600.0152.72 ± 0.596743 ± 51216.68 ± 0.91
DH Peg
−0.350.08b2.86 ± 0.437413 ± 31216.90 ± 0.04
DY Peg
−0.050.03.41 ± 0.167157 ± 24610.60 ± 0.19
CU Com
−2.200.023.09 ± 0.516925 ± 3093.21 ± 0.12
V372 Serc
−0.530.0033.24 ± 0.366713 ± 3248.13 ± 0.16
V500 Hyac
−1.050.0083.69 ± 0.506902 ± 26110.17 ± 0.37

The following phase intervals were used in the folded colour curves to derive |$[M/\text{H}]$| and E(B − V).

SW And: 0.4 < φ < 0.8 (HJD − 2454300 = 50, 51, 53);

DH Peg: 0.1 < φ < 0.4 (HJD = 2454349);

DY Peg: 0.3 < φ < 0.8 (HJD = 2454300 = 45, 46, 47);

CU Com: 39 epochs were taken from the shock-free

intervals on HJD − 2454800 = 71, 73, 74.

The errors are |$\pm 0.10\:\mbox{dex}\text{ and}\:\pm 0.01\:\mbox{mag}$| (except for CU Com where it is ±0.20 dex), respectively.

aPaper I.

b Jones et al. (1988).

cPaper II.

Table 5.
Open in new tab

Metallicity, reddening, averaged surface gravity, effective temperature, angular radius of the stars and the standard deviation of the averaged quantities.

|$[M/\text{H}]$|E(B − V)|$\overline{\log g_{\rm e}}$||$\overline{T_{\rm e}}$||$\overline{\vartheta \times 10^{11}}$|
(dex)(mag)(cm s−2)(K)(rad)
SW And, HJD-2444720 = 0, 1, 2, 3, 4
0.022.60 ± 0.356676 ± 42117.52 ± 0.68
HJD-2454350 = 0, 1, 3
0.100.022.85 ± 0.636610 ± 42817.31 ± 0.68
HJD-2454830 = −8, −1, 0, 1, 2
2.75 ± 0.446637 ± 39317.53 ± 0.65
SU Draa
−1.600.0152.72 ± 0.596743 ± 51216.68 ± 0.91
DH Peg
−0.350.08b2.86 ± 0.437413 ± 31216.90 ± 0.04
DY Peg
−0.050.03.41 ± 0.167157 ± 24610.60 ± 0.19
CU Com
−2.200.023.09 ± 0.516925 ± 3093.21 ± 0.12
V372 Serc
−0.530.0033.24 ± 0.366713 ± 3248.13 ± 0.16
V500 Hyac
−1.050.0083.69 ± 0.506902 ± 26110.17 ± 0.37
|$[M/\text{H}]$|E(B − V)|$\overline{\log g_{\rm e}}$||$\overline{T_{\rm e}}$||$\overline{\vartheta \times 10^{11}}$|
(dex)(mag)(cm s−2)(K)(rad)
SW And, HJD-2444720 = 0, 1, 2, 3, 4
0.022.60 ± 0.356676 ± 42117.52 ± 0.68
HJD-2454350 = 0, 1, 3
0.100.022.85 ± 0.636610 ± 42817.31 ± 0.68
HJD-2454830 = −8, −1, 0, 1, 2
2.75 ± 0.446637 ± 39317.53 ± 0.65
SU Draa
−1.600.0152.72 ± 0.596743 ± 51216.68 ± 0.91
DH Peg
−0.350.08b2.86 ± 0.437413 ± 31216.90 ± 0.04
DY Peg
−0.050.03.41 ± 0.167157 ± 24610.60 ± 0.19
CU Com
−2.200.023.09 ± 0.516925 ± 3093.21 ± 0.12
V372 Serc
−0.530.0033.24 ± 0.366713 ± 3248.13 ± 0.16
V500 Hyac
−1.050.0083.69 ± 0.506902 ± 26110.17 ± 0.37

The following phase intervals were used in the folded colour curves to derive |$[M/\text{H}]$| and E(B − V).

SW And: 0.4 < φ < 0.8 (HJD − 2454300 = 50, 51, 53);

DH Peg: 0.1 < φ < 0.4 (HJD = 2454349);

DY Peg: 0.3 < φ < 0.8 (HJD = 2454300 = 45, 46, 47);

CU Com: 39 epochs were taken from the shock-free

intervals on HJD − 2454800 = 71, 73, 74.

The errors are |$\pm 0.10\:\mbox{dex}\text{ and}\:\pm 0.01\:\mbox{mag}$| (except for CU Com where it is ±0.20 dex), respectively.

aPaper I.

b Jones et al. (1988).

cPaper II.

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