Physical parameters of the 17 white dwarfs confirmed via spectroscopic follow-up. The S/N is measured at H β. δτWD is the fractional difference in cooling ages, between Montreal and BaSTI models (see Section 4.1 for details).
Name . | Cluster . | S/N . | Type . | Teff . | log g . | Mg . | E(B − V) . | d . | MWD . | τWD . | δτWD . |
---|---|---|---|---|---|---|---|---|---|---|---|
. | . | . | . | (K) . | (cgs) . | (mag) . | (mag) . | (pc) . | (M⊙) . | (Gyr) . | . |
VPHAS J0804−2809 | NGC 2527 | 20 | DA | 18 160 ± 260 | 8.24 ± 0.05 | |$11.27_{-0.07}^{+0.09}$| | 0.05 ± 0.07 | 630 ± 77 | |$0.77_{-0.03}^{+0.03}$| | |$0.185_{-0.016}^{+0.016}$| | 0.12 |
VPHAS J0815−3625 | BH 23 | 28 | DA | 31 870 ± 210 | 8.04 ± 0.04 | |$9.79_{-0.06}^{+0.06}$| | 0.12 ± 0.03 | 734 ± 40 | |$0.68_{-0.02}^{+0.02}$| | |$0.011_{-0.002}^{+0.002}$| | 0.10 |
VPHAS J0900−4556 | Platais 9 | 23 | DB | 19 040 ± 450 | 8.13 ± 0.10 | |$10.94_{-0.14}^{+0.14}$| | 0.01 ± 0.05 | 615 ± 59 | |$0.70_{-0.06}^{+0.06}$| | |$0.130_{-0.029}^{+0.029}$| | 0.11 |
VPHAS J1018−5752 | ASCC 59 | 10 | DA | 17 430 ± 390 | 7.79 ± 0.08 | |$10.66_{-0.12}^{+0.13}$| | 0.00 ± 0.04 | 1066 ± 86 | |$0.52_{-0.04}^{+0.04}$| | |$0.095_{-0.010}^{+0.010}$| | 0.00 |
VPHAS J1021−5732 | ASCC 59 | 27 | DA | 30 110 ± 160 | 8.56 ± 0.03 | |$10.79_{-0.05}^{+0.05}$| | 0.28 ± 0.04 | 382 ± 27 | |$0.98_{-0.02}^{+0.02}$| | |$0.059_{-0.006}^{+0.006}$| | 0.10 |
VPHAS J1025−5841 | Loden 143 | 21 | DA | 13 280 ± 240 | 8.44 ± 0.04 | |$12.23_{-0.07}^{+0.07}$| | 0.12 ± 0.04 | 263 ± 19 | |$0.89_{-0.03}^{+0.03}$| | |$0.580_{-0.028}^{+0.028}$| | 0.04 |
VPHAS J1029−5855 | Loden 143 | 14 | DAH | a35 000 ± 5000 | 8.00 ± 0.25 | |$9.52_{-0.46}^{+0.46}$| | 1326 ± 214 | |$0.66_{-0.11}^{+0.15}$| | |$0.006_{-0.002}^{+0.009}$| | −0.12 | |
VPHAS J1030−5900 | Loden 143 | 22 | DA | 19 780 ± 250 | 8.04 ± 0.04 | |$10.81_{-0.06}^{+0.06}$| | 0.07 ± 0.04 | 565 ± 41 | |$0.65_{-0.02}^{+0.02}$| | |$0.084_{-0.011}^{+0.011}$| | 0.00 |
VPHAS J1103−5837 | NGC 3532 | 19 | DA | 23 910 ± 360 | 8.87 ± 0.05 | |$11.89_{-0.11}^{+0.11}$| | 0.13 ± 0.07 | 433 ± 54 | |$1.13_{-0.03}^{+0.03}$| | |$^{b}0.270_{-0.025}^{+0.034}$| | |
VPHAS J1104−5830 | NGC 3532 | 8 | DC | a29 500 ± 300 | 8.00 ± 0.25 | |$9.90_{-0.44}^{+0.44}$| | 1174 ± 174 | |$0.64_{-0.11}^{+0.15}$| | |$0.011_{-0.003}^{+0.021}$| | −0.19 | |
VPHAS J1105−5842 | NGC 3532 | 15 | DA | 14 230 ± 1160 | 8.16 ± 0.10 | |$11.64_{-0.16}^{+0.17}$| | 0.06 ± 0.04 | 363 ± 36 | |$0.71_{-0.06}^{+0.06}$| | |$0.323_{-0.066}^{+0.086}$| | 0.11 |
VPHAS J1337−6121 | Platais 10 | 14 | DA | 24 100 ± 530 | 8.01 ± 0.08 | |$10.37_{-0.13}^{+0.13}$| | 0.20 ± 0.05 | 709 ± 67 | |$0.64_{-0.04}^{+0.05}$| | |$0.032_{-0.005}^{+0.013}$| | 0.00 |
VPHAS J1344−6134 | Platais 10 | 10 | DA | 49 670 ± 2520 | 7.92 ± 0.19 | |$8.87_{-0.37}^{+0.37}$| | 0.39 ± 0.06 | 1202 ± 169 | |$0.66_{-0.08}^{+0.09}$| | 0.002 | −0.81 |
VPHAS J1546−5233 | Johansson 1 | 12 | DA | 20 440 ± 550 | 7.98 ± 0.09 | |$10.65_{-0.15}^{+0.15}$| | 0.12 ± 0.11 | 1052 ± 204 | |$0.62_{-0.04}^{+0.05}$| | |$0.063_{-0.006}^{+0.019}$| | −0.01 |
VPHAS J1549−5251 | ASCC 83 | 14 | DA | 20 320 ± 390 | 8.05 ± 0.07 | |$10.77_{-0.11}^{+0.11}$| | 0.07 ± 0.10 | 951 ± 165 | |$0.66_{-0.04}^{+0.04}$| | |$0.078_{-0.014}^{+0.017}$| | 0.01 |
VPHAS J1748−2914 | Ruprecht 131 | 12 | DAH | a8750 ± 1200 | 8.00 ± 0.25 | |$12.84_{-0.52}^{+0.61}$| | 471 ± 102 | |$0.60_{-0.12}^{+0.16}$| | |$0.854_{-0.243}^{+0.672}$| | 0.05 | |
VPHAS J1800−2332 | Ruprecht 139 | 21 | DA | 24 030 ± 360 | 8.60 ± 0.05 | |$11.36_{-0.09}^{+0.09}$| | 0.24 ± 0.02 | 165 ± 7 | |$0.99_{-0.03}^{+0.03}$| | |$0.153_{-0.019}^{+0.019}$| | 0.21 |
Name . | Cluster . | S/N . | Type . | Teff . | log g . | Mg . | E(B − V) . | d . | MWD . | τWD . | δτWD . |
---|---|---|---|---|---|---|---|---|---|---|---|
. | . | . | . | (K) . | (cgs) . | (mag) . | (mag) . | (pc) . | (M⊙) . | (Gyr) . | . |
VPHAS J0804−2809 | NGC 2527 | 20 | DA | 18 160 ± 260 | 8.24 ± 0.05 | |$11.27_{-0.07}^{+0.09}$| | 0.05 ± 0.07 | 630 ± 77 | |$0.77_{-0.03}^{+0.03}$| | |$0.185_{-0.016}^{+0.016}$| | 0.12 |
VPHAS J0815−3625 | BH 23 | 28 | DA | 31 870 ± 210 | 8.04 ± 0.04 | |$9.79_{-0.06}^{+0.06}$| | 0.12 ± 0.03 | 734 ± 40 | |$0.68_{-0.02}^{+0.02}$| | |$0.011_{-0.002}^{+0.002}$| | 0.10 |
VPHAS J0900−4556 | Platais 9 | 23 | DB | 19 040 ± 450 | 8.13 ± 0.10 | |$10.94_{-0.14}^{+0.14}$| | 0.01 ± 0.05 | 615 ± 59 | |$0.70_{-0.06}^{+0.06}$| | |$0.130_{-0.029}^{+0.029}$| | 0.11 |
VPHAS J1018−5752 | ASCC 59 | 10 | DA | 17 430 ± 390 | 7.79 ± 0.08 | |$10.66_{-0.12}^{+0.13}$| | 0.00 ± 0.04 | 1066 ± 86 | |$0.52_{-0.04}^{+0.04}$| | |$0.095_{-0.010}^{+0.010}$| | 0.00 |
VPHAS J1021−5732 | ASCC 59 | 27 | DA | 30 110 ± 160 | 8.56 ± 0.03 | |$10.79_{-0.05}^{+0.05}$| | 0.28 ± 0.04 | 382 ± 27 | |$0.98_{-0.02}^{+0.02}$| | |$0.059_{-0.006}^{+0.006}$| | 0.10 |
VPHAS J1025−5841 | Loden 143 | 21 | DA | 13 280 ± 240 | 8.44 ± 0.04 | |$12.23_{-0.07}^{+0.07}$| | 0.12 ± 0.04 | 263 ± 19 | |$0.89_{-0.03}^{+0.03}$| | |$0.580_{-0.028}^{+0.028}$| | 0.04 |
VPHAS J1029−5855 | Loden 143 | 14 | DAH | a35 000 ± 5000 | 8.00 ± 0.25 | |$9.52_{-0.46}^{+0.46}$| | 1326 ± 214 | |$0.66_{-0.11}^{+0.15}$| | |$0.006_{-0.002}^{+0.009}$| | −0.12 | |
VPHAS J1030−5900 | Loden 143 | 22 | DA | 19 780 ± 250 | 8.04 ± 0.04 | |$10.81_{-0.06}^{+0.06}$| | 0.07 ± 0.04 | 565 ± 41 | |$0.65_{-0.02}^{+0.02}$| | |$0.084_{-0.011}^{+0.011}$| | 0.00 |
VPHAS J1103−5837 | NGC 3532 | 19 | DA | 23 910 ± 360 | 8.87 ± 0.05 | |$11.89_{-0.11}^{+0.11}$| | 0.13 ± 0.07 | 433 ± 54 | |$1.13_{-0.03}^{+0.03}$| | |$^{b}0.270_{-0.025}^{+0.034}$| | |
VPHAS J1104−5830 | NGC 3532 | 8 | DC | a29 500 ± 300 | 8.00 ± 0.25 | |$9.90_{-0.44}^{+0.44}$| | 1174 ± 174 | |$0.64_{-0.11}^{+0.15}$| | |$0.011_{-0.003}^{+0.021}$| | −0.19 | |
VPHAS J1105−5842 | NGC 3532 | 15 | DA | 14 230 ± 1160 | 8.16 ± 0.10 | |$11.64_{-0.16}^{+0.17}$| | 0.06 ± 0.04 | 363 ± 36 | |$0.71_{-0.06}^{+0.06}$| | |$0.323_{-0.066}^{+0.086}$| | 0.11 |
VPHAS J1337−6121 | Platais 10 | 14 | DA | 24 100 ± 530 | 8.01 ± 0.08 | |$10.37_{-0.13}^{+0.13}$| | 0.20 ± 0.05 | 709 ± 67 | |$0.64_{-0.04}^{+0.05}$| | |$0.032_{-0.005}^{+0.013}$| | 0.00 |
VPHAS J1344−6134 | Platais 10 | 10 | DA | 49 670 ± 2520 | 7.92 ± 0.19 | |$8.87_{-0.37}^{+0.37}$| | 0.39 ± 0.06 | 1202 ± 169 | |$0.66_{-0.08}^{+0.09}$| | 0.002 | −0.81 |
VPHAS J1546−5233 | Johansson 1 | 12 | DA | 20 440 ± 550 | 7.98 ± 0.09 | |$10.65_{-0.15}^{+0.15}$| | 0.12 ± 0.11 | 1052 ± 204 | |$0.62_{-0.04}^{+0.05}$| | |$0.063_{-0.006}^{+0.019}$| | −0.01 |
VPHAS J1549−5251 | ASCC 83 | 14 | DA | 20 320 ± 390 | 8.05 ± 0.07 | |$10.77_{-0.11}^{+0.11}$| | 0.07 ± 0.10 | 951 ± 165 | |$0.66_{-0.04}^{+0.04}$| | |$0.078_{-0.014}^{+0.017}$| | 0.01 |
VPHAS J1748−2914 | Ruprecht 131 | 12 | DAH | a8750 ± 1200 | 8.00 ± 0.25 | |$12.84_{-0.52}^{+0.61}$| | 471 ± 102 | |$0.60_{-0.12}^{+0.16}$| | |$0.854_{-0.243}^{+0.672}$| | 0.05 | |
VPHAS J1800−2332 | Ruprecht 139 | 21 | DA | 24 030 ± 360 | 8.60 ± 0.05 | |$11.36_{-0.09}^{+0.09}$| | 0.24 ± 0.02 | 165 ± 7 | |$0.99_{-0.03}^{+0.03}$| | |$0.153_{-0.019}^{+0.019}$| | 0.21 |
Notes. aEffective temperatures of DAH and DC white dwarfs are estimated from photometric fitting; no E(B−V) estimates.
bCooling age determined from Althaus et al. (2007) oxygen–neon core models.
Physical parameters of the 17 white dwarfs confirmed via spectroscopic follow-up. The S/N is measured at H β. δτWD is the fractional difference in cooling ages, between Montreal and BaSTI models (see Section 4.1 for details).
Name . | Cluster . | S/N . | Type . | Teff . | log g . | Mg . | E(B − V) . | d . | MWD . | τWD . | δτWD . |
---|---|---|---|---|---|---|---|---|---|---|---|
. | . | . | . | (K) . | (cgs) . | (mag) . | (mag) . | (pc) . | (M⊙) . | (Gyr) . | . |
VPHAS J0804−2809 | NGC 2527 | 20 | DA | 18 160 ± 260 | 8.24 ± 0.05 | |$11.27_{-0.07}^{+0.09}$| | 0.05 ± 0.07 | 630 ± 77 | |$0.77_{-0.03}^{+0.03}$| | |$0.185_{-0.016}^{+0.016}$| | 0.12 |
VPHAS J0815−3625 | BH 23 | 28 | DA | 31 870 ± 210 | 8.04 ± 0.04 | |$9.79_{-0.06}^{+0.06}$| | 0.12 ± 0.03 | 734 ± 40 | |$0.68_{-0.02}^{+0.02}$| | |$0.011_{-0.002}^{+0.002}$| | 0.10 |
VPHAS J0900−4556 | Platais 9 | 23 | DB | 19 040 ± 450 | 8.13 ± 0.10 | |$10.94_{-0.14}^{+0.14}$| | 0.01 ± 0.05 | 615 ± 59 | |$0.70_{-0.06}^{+0.06}$| | |$0.130_{-0.029}^{+0.029}$| | 0.11 |
VPHAS J1018−5752 | ASCC 59 | 10 | DA | 17 430 ± 390 | 7.79 ± 0.08 | |$10.66_{-0.12}^{+0.13}$| | 0.00 ± 0.04 | 1066 ± 86 | |$0.52_{-0.04}^{+0.04}$| | |$0.095_{-0.010}^{+0.010}$| | 0.00 |
VPHAS J1021−5732 | ASCC 59 | 27 | DA | 30 110 ± 160 | 8.56 ± 0.03 | |$10.79_{-0.05}^{+0.05}$| | 0.28 ± 0.04 | 382 ± 27 | |$0.98_{-0.02}^{+0.02}$| | |$0.059_{-0.006}^{+0.006}$| | 0.10 |
VPHAS J1025−5841 | Loden 143 | 21 | DA | 13 280 ± 240 | 8.44 ± 0.04 | |$12.23_{-0.07}^{+0.07}$| | 0.12 ± 0.04 | 263 ± 19 | |$0.89_{-0.03}^{+0.03}$| | |$0.580_{-0.028}^{+0.028}$| | 0.04 |
VPHAS J1029−5855 | Loden 143 | 14 | DAH | a35 000 ± 5000 | 8.00 ± 0.25 | |$9.52_{-0.46}^{+0.46}$| | 1326 ± 214 | |$0.66_{-0.11}^{+0.15}$| | |$0.006_{-0.002}^{+0.009}$| | −0.12 | |
VPHAS J1030−5900 | Loden 143 | 22 | DA | 19 780 ± 250 | 8.04 ± 0.04 | |$10.81_{-0.06}^{+0.06}$| | 0.07 ± 0.04 | 565 ± 41 | |$0.65_{-0.02}^{+0.02}$| | |$0.084_{-0.011}^{+0.011}$| | 0.00 |
VPHAS J1103−5837 | NGC 3532 | 19 | DA | 23 910 ± 360 | 8.87 ± 0.05 | |$11.89_{-0.11}^{+0.11}$| | 0.13 ± 0.07 | 433 ± 54 | |$1.13_{-0.03}^{+0.03}$| | |$^{b}0.270_{-0.025}^{+0.034}$| | |
VPHAS J1104−5830 | NGC 3532 | 8 | DC | a29 500 ± 300 | 8.00 ± 0.25 | |$9.90_{-0.44}^{+0.44}$| | 1174 ± 174 | |$0.64_{-0.11}^{+0.15}$| | |$0.011_{-0.003}^{+0.021}$| | −0.19 | |
VPHAS J1105−5842 | NGC 3532 | 15 | DA | 14 230 ± 1160 | 8.16 ± 0.10 | |$11.64_{-0.16}^{+0.17}$| | 0.06 ± 0.04 | 363 ± 36 | |$0.71_{-0.06}^{+0.06}$| | |$0.323_{-0.066}^{+0.086}$| | 0.11 |
VPHAS J1337−6121 | Platais 10 | 14 | DA | 24 100 ± 530 | 8.01 ± 0.08 | |$10.37_{-0.13}^{+0.13}$| | 0.20 ± 0.05 | 709 ± 67 | |$0.64_{-0.04}^{+0.05}$| | |$0.032_{-0.005}^{+0.013}$| | 0.00 |
VPHAS J1344−6134 | Platais 10 | 10 | DA | 49 670 ± 2520 | 7.92 ± 0.19 | |$8.87_{-0.37}^{+0.37}$| | 0.39 ± 0.06 | 1202 ± 169 | |$0.66_{-0.08}^{+0.09}$| | 0.002 | −0.81 |
VPHAS J1546−5233 | Johansson 1 | 12 | DA | 20 440 ± 550 | 7.98 ± 0.09 | |$10.65_{-0.15}^{+0.15}$| | 0.12 ± 0.11 | 1052 ± 204 | |$0.62_{-0.04}^{+0.05}$| | |$0.063_{-0.006}^{+0.019}$| | −0.01 |
VPHAS J1549−5251 | ASCC 83 | 14 | DA | 20 320 ± 390 | 8.05 ± 0.07 | |$10.77_{-0.11}^{+0.11}$| | 0.07 ± 0.10 | 951 ± 165 | |$0.66_{-0.04}^{+0.04}$| | |$0.078_{-0.014}^{+0.017}$| | 0.01 |
VPHAS J1748−2914 | Ruprecht 131 | 12 | DAH | a8750 ± 1200 | 8.00 ± 0.25 | |$12.84_{-0.52}^{+0.61}$| | 471 ± 102 | |$0.60_{-0.12}^{+0.16}$| | |$0.854_{-0.243}^{+0.672}$| | 0.05 | |
VPHAS J1800−2332 | Ruprecht 139 | 21 | DA | 24 030 ± 360 | 8.60 ± 0.05 | |$11.36_{-0.09}^{+0.09}$| | 0.24 ± 0.02 | 165 ± 7 | |$0.99_{-0.03}^{+0.03}$| | |$0.153_{-0.019}^{+0.019}$| | 0.21 |
Name . | Cluster . | S/N . | Type . | Teff . | log g . | Mg . | E(B − V) . | d . | MWD . | τWD . | δτWD . |
---|---|---|---|---|---|---|---|---|---|---|---|
. | . | . | . | (K) . | (cgs) . | (mag) . | (mag) . | (pc) . | (M⊙) . | (Gyr) . | . |
VPHAS J0804−2809 | NGC 2527 | 20 | DA | 18 160 ± 260 | 8.24 ± 0.05 | |$11.27_{-0.07}^{+0.09}$| | 0.05 ± 0.07 | 630 ± 77 | |$0.77_{-0.03}^{+0.03}$| | |$0.185_{-0.016}^{+0.016}$| | 0.12 |
VPHAS J0815−3625 | BH 23 | 28 | DA | 31 870 ± 210 | 8.04 ± 0.04 | |$9.79_{-0.06}^{+0.06}$| | 0.12 ± 0.03 | 734 ± 40 | |$0.68_{-0.02}^{+0.02}$| | |$0.011_{-0.002}^{+0.002}$| | 0.10 |
VPHAS J0900−4556 | Platais 9 | 23 | DB | 19 040 ± 450 | 8.13 ± 0.10 | |$10.94_{-0.14}^{+0.14}$| | 0.01 ± 0.05 | 615 ± 59 | |$0.70_{-0.06}^{+0.06}$| | |$0.130_{-0.029}^{+0.029}$| | 0.11 |
VPHAS J1018−5752 | ASCC 59 | 10 | DA | 17 430 ± 390 | 7.79 ± 0.08 | |$10.66_{-0.12}^{+0.13}$| | 0.00 ± 0.04 | 1066 ± 86 | |$0.52_{-0.04}^{+0.04}$| | |$0.095_{-0.010}^{+0.010}$| | 0.00 |
VPHAS J1021−5732 | ASCC 59 | 27 | DA | 30 110 ± 160 | 8.56 ± 0.03 | |$10.79_{-0.05}^{+0.05}$| | 0.28 ± 0.04 | 382 ± 27 | |$0.98_{-0.02}^{+0.02}$| | |$0.059_{-0.006}^{+0.006}$| | 0.10 |
VPHAS J1025−5841 | Loden 143 | 21 | DA | 13 280 ± 240 | 8.44 ± 0.04 | |$12.23_{-0.07}^{+0.07}$| | 0.12 ± 0.04 | 263 ± 19 | |$0.89_{-0.03}^{+0.03}$| | |$0.580_{-0.028}^{+0.028}$| | 0.04 |
VPHAS J1029−5855 | Loden 143 | 14 | DAH | a35 000 ± 5000 | 8.00 ± 0.25 | |$9.52_{-0.46}^{+0.46}$| | 1326 ± 214 | |$0.66_{-0.11}^{+0.15}$| | |$0.006_{-0.002}^{+0.009}$| | −0.12 | |
VPHAS J1030−5900 | Loden 143 | 22 | DA | 19 780 ± 250 | 8.04 ± 0.04 | |$10.81_{-0.06}^{+0.06}$| | 0.07 ± 0.04 | 565 ± 41 | |$0.65_{-0.02}^{+0.02}$| | |$0.084_{-0.011}^{+0.011}$| | 0.00 |
VPHAS J1103−5837 | NGC 3532 | 19 | DA | 23 910 ± 360 | 8.87 ± 0.05 | |$11.89_{-0.11}^{+0.11}$| | 0.13 ± 0.07 | 433 ± 54 | |$1.13_{-0.03}^{+0.03}$| | |$^{b}0.270_{-0.025}^{+0.034}$| | |
VPHAS J1104−5830 | NGC 3532 | 8 | DC | a29 500 ± 300 | 8.00 ± 0.25 | |$9.90_{-0.44}^{+0.44}$| | 1174 ± 174 | |$0.64_{-0.11}^{+0.15}$| | |$0.011_{-0.003}^{+0.021}$| | −0.19 | |
VPHAS J1105−5842 | NGC 3532 | 15 | DA | 14 230 ± 1160 | 8.16 ± 0.10 | |$11.64_{-0.16}^{+0.17}$| | 0.06 ± 0.04 | 363 ± 36 | |$0.71_{-0.06}^{+0.06}$| | |$0.323_{-0.066}^{+0.086}$| | 0.11 |
VPHAS J1337−6121 | Platais 10 | 14 | DA | 24 100 ± 530 | 8.01 ± 0.08 | |$10.37_{-0.13}^{+0.13}$| | 0.20 ± 0.05 | 709 ± 67 | |$0.64_{-0.04}^{+0.05}$| | |$0.032_{-0.005}^{+0.013}$| | 0.00 |
VPHAS J1344−6134 | Platais 10 | 10 | DA | 49 670 ± 2520 | 7.92 ± 0.19 | |$8.87_{-0.37}^{+0.37}$| | 0.39 ± 0.06 | 1202 ± 169 | |$0.66_{-0.08}^{+0.09}$| | 0.002 | −0.81 |
VPHAS J1546−5233 | Johansson 1 | 12 | DA | 20 440 ± 550 | 7.98 ± 0.09 | |$10.65_{-0.15}^{+0.15}$| | 0.12 ± 0.11 | 1052 ± 204 | |$0.62_{-0.04}^{+0.05}$| | |$0.063_{-0.006}^{+0.019}$| | −0.01 |
VPHAS J1549−5251 | ASCC 83 | 14 | DA | 20 320 ± 390 | 8.05 ± 0.07 | |$10.77_{-0.11}^{+0.11}$| | 0.07 ± 0.10 | 951 ± 165 | |$0.66_{-0.04}^{+0.04}$| | |$0.078_{-0.014}^{+0.017}$| | 0.01 |
VPHAS J1748−2914 | Ruprecht 131 | 12 | DAH | a8750 ± 1200 | 8.00 ± 0.25 | |$12.84_{-0.52}^{+0.61}$| | 471 ± 102 | |$0.60_{-0.12}^{+0.16}$| | |$0.854_{-0.243}^{+0.672}$| | 0.05 | |
VPHAS J1800−2332 | Ruprecht 139 | 21 | DA | 24 030 ± 360 | 8.60 ± 0.05 | |$11.36_{-0.09}^{+0.09}$| | 0.24 ± 0.02 | 165 ± 7 | |$0.99_{-0.03}^{+0.03}$| | |$0.153_{-0.019}^{+0.019}$| | 0.21 |
Notes. aEffective temperatures of DAH and DC white dwarfs are estimated from photometric fitting; no E(B−V) estimates.
bCooling age determined from Althaus et al. (2007) oxygen–neon core models.
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