Table 4.

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).

NameClusterS/NTypeTefflog gMgE(BV)dMWDτWDδτWD
(K)(cgs)(mag)(mag)(pc)(M)(Gyr)
VPHAS J0804−2809NGC 252720DA18 160 ± 2608.24 ± 0.05|$11.27_{-0.07}^{+0.09}$|0.05 ± 0.07630 ± 77|$0.77_{-0.03}^{+0.03}$||$0.185_{-0.016}^{+0.016}$|0.12
VPHAS J0815−3625BH 2328DA31 870 ± 2108.04 ± 0.04|$9.79_{-0.06}^{+0.06}$|0.12 ± 0.03734 ± 40|$0.68_{-0.02}^{+0.02}$||$0.011_{-0.002}^{+0.002}$|0.10
VPHAS J0900−4556Platais 923DB19 040 ± 4508.13 ± 0.10|$10.94_{-0.14}^{+0.14}$|0.01 ± 0.05615 ± 59|$0.70_{-0.06}^{+0.06}$||$0.130_{-0.029}^{+0.029}$|0.11
VPHAS J1018−5752ASCC 5910DA17 430 ± 3907.79 ± 0.08|$10.66_{-0.12}^{+0.13}$|0.00 ± 0.041066 ± 86|$0.52_{-0.04}^{+0.04}$||$0.095_{-0.010}^{+0.010}$|0.00
VPHAS J1021−5732ASCC 5927DA30 110 ± 1608.56 ± 0.03|$10.79_{-0.05}^{+0.05}$|0.28 ± 0.04382 ± 27|$0.98_{-0.02}^{+0.02}$||$0.059_{-0.006}^{+0.006}$|0.10
VPHAS J1025−5841Loden 14321DA13 280 ± 2408.44 ± 0.04|$12.23_{-0.07}^{+0.07}$|0.12 ± 0.04263 ± 19|$0.89_{-0.03}^{+0.03}$||$0.580_{-0.028}^{+0.028}$|0.04
VPHAS J1029−5855Loden 14314DAHa35 000 ± 50008.00 ± 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 J1030−5900Loden 14322DA19 780 ± 2508.04 ± 0.04|$10.81_{-0.06}^{+0.06}$|0.07 ± 0.04565 ± 41|$0.65_{-0.02}^{+0.02}$||$0.084_{-0.011}^{+0.011}$|0.00
VPHAS J1103−5837NGC 353219DA23 910 ± 3608.87 ± 0.05|$11.89_{-0.11}^{+0.11}$|0.13 ± 0.07433 ± 54|$1.13_{-0.03}^{+0.03}$||$^{b}0.270_{-0.025}^{+0.034}$|
VPHAS J1104−5830NGC 35328DCa29 500 ± 3008.00 ± 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 J1105−5842NGC 353215DA14 230 ± 11608.16 ± 0.10|$11.64_{-0.16}^{+0.17}$|0.06 ± 0.04363 ± 36|$0.71_{-0.06}^{+0.06}$||$0.323_{-0.066}^{+0.086}$|0.11
VPHAS J1337−6121Platais 1014DA24 100 ± 5308.01 ± 0.08|$10.37_{-0.13}^{+0.13}$|0.20 ± 0.05709 ± 67|$0.64_{-0.04}^{+0.05}$||$0.032_{-0.005}^{+0.013}$|0.00
VPHAS J1344−6134Platais 1010DA49 670 ± 25207.92 ± 0.19|$8.87_{-0.37}^{+0.37}$|0.39 ± 0.061202 ± 169|$0.66_{-0.08}^{+0.09}$|0.002−0.81
VPHAS J1546−5233Johansson 112DA20 440 ± 5507.98 ± 0.09|$10.65_{-0.15}^{+0.15}$|0.12 ± 0.111052 ± 204|$0.62_{-0.04}^{+0.05}$||$0.063_{-0.006}^{+0.019}$|−0.01
VPHAS J1549−5251ASCC 8314DA20 320 ± 3908.05 ± 0.07|$10.77_{-0.11}^{+0.11}$|0.07 ± 0.10951 ± 165|$0.66_{-0.04}^{+0.04}$||$0.078_{-0.014}^{+0.017}$|0.01
VPHAS J1748−2914Ruprecht 13112DAHa8750 ± 12008.00 ± 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 J1800−2332Ruprecht 13921DA24 030 ± 3608.60 ± 0.05|$11.36_{-0.09}^{+0.09}$|0.24 ± 0.02165 ± 7|$0.99_{-0.03}^{+0.03}$||$0.153_{-0.019}^{+0.019}$|0.21
NameClusterS/NTypeTefflog gMgE(BV)dMWDτWDδτWD
(K)(cgs)(mag)(mag)(pc)(M)(Gyr)
VPHAS J0804−2809NGC 252720DA18 160 ± 2608.24 ± 0.05|$11.27_{-0.07}^{+0.09}$|0.05 ± 0.07630 ± 77|$0.77_{-0.03}^{+0.03}$||$0.185_{-0.016}^{+0.016}$|0.12
VPHAS J0815−3625BH 2328DA31 870 ± 2108.04 ± 0.04|$9.79_{-0.06}^{+0.06}$|0.12 ± 0.03734 ± 40|$0.68_{-0.02}^{+0.02}$||$0.011_{-0.002}^{+0.002}$|0.10
VPHAS J0900−4556Platais 923DB19 040 ± 4508.13 ± 0.10|$10.94_{-0.14}^{+0.14}$|0.01 ± 0.05615 ± 59|$0.70_{-0.06}^{+0.06}$||$0.130_{-0.029}^{+0.029}$|0.11
VPHAS J1018−5752ASCC 5910DA17 430 ± 3907.79 ± 0.08|$10.66_{-0.12}^{+0.13}$|0.00 ± 0.041066 ± 86|$0.52_{-0.04}^{+0.04}$||$0.095_{-0.010}^{+0.010}$|0.00
VPHAS J1021−5732ASCC 5927DA30 110 ± 1608.56 ± 0.03|$10.79_{-0.05}^{+0.05}$|0.28 ± 0.04382 ± 27|$0.98_{-0.02}^{+0.02}$||$0.059_{-0.006}^{+0.006}$|0.10
VPHAS J1025−5841Loden 14321DA13 280 ± 2408.44 ± 0.04|$12.23_{-0.07}^{+0.07}$|0.12 ± 0.04263 ± 19|$0.89_{-0.03}^{+0.03}$||$0.580_{-0.028}^{+0.028}$|0.04
VPHAS J1029−5855Loden 14314DAHa35 000 ± 50008.00 ± 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 J1030−5900Loden 14322DA19 780 ± 2508.04 ± 0.04|$10.81_{-0.06}^{+0.06}$|0.07 ± 0.04565 ± 41|$0.65_{-0.02}^{+0.02}$||$0.084_{-0.011}^{+0.011}$|0.00
VPHAS J1103−5837NGC 353219DA23 910 ± 3608.87 ± 0.05|$11.89_{-0.11}^{+0.11}$|0.13 ± 0.07433 ± 54|$1.13_{-0.03}^{+0.03}$||$^{b}0.270_{-0.025}^{+0.034}$|
VPHAS J1104−5830NGC 35328DCa29 500 ± 3008.00 ± 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 J1105−5842NGC 353215DA14 230 ± 11608.16 ± 0.10|$11.64_{-0.16}^{+0.17}$|0.06 ± 0.04363 ± 36|$0.71_{-0.06}^{+0.06}$||$0.323_{-0.066}^{+0.086}$|0.11
VPHAS J1337−6121Platais 1014DA24 100 ± 5308.01 ± 0.08|$10.37_{-0.13}^{+0.13}$|0.20 ± 0.05709 ± 67|$0.64_{-0.04}^{+0.05}$||$0.032_{-0.005}^{+0.013}$|0.00
VPHAS J1344−6134Platais 1010DA49 670 ± 25207.92 ± 0.19|$8.87_{-0.37}^{+0.37}$|0.39 ± 0.061202 ± 169|$0.66_{-0.08}^{+0.09}$|0.002−0.81
VPHAS J1546−5233Johansson 112DA20 440 ± 5507.98 ± 0.09|$10.65_{-0.15}^{+0.15}$|0.12 ± 0.111052 ± 204|$0.62_{-0.04}^{+0.05}$||$0.063_{-0.006}^{+0.019}$|−0.01
VPHAS J1549−5251ASCC 8314DA20 320 ± 3908.05 ± 0.07|$10.77_{-0.11}^{+0.11}$|0.07 ± 0.10951 ± 165|$0.66_{-0.04}^{+0.04}$||$0.078_{-0.014}^{+0.017}$|0.01
VPHAS J1748−2914Ruprecht 13112DAHa8750 ± 12008.00 ± 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 J1800−2332Ruprecht 13921DA24 030 ± 3608.60 ± 0.05|$11.36_{-0.09}^{+0.09}$|0.24 ± 0.02165 ± 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(BV) estimates.

bCooling age determined from Althaus et al. (2007) oxygen–neon core models.

Table 4.

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).

NameClusterS/NTypeTefflog gMgE(BV)dMWDτWDδτWD
(K)(cgs)(mag)(mag)(pc)(M)(Gyr)
VPHAS J0804−2809NGC 252720DA18 160 ± 2608.24 ± 0.05|$11.27_{-0.07}^{+0.09}$|0.05 ± 0.07630 ± 77|$0.77_{-0.03}^{+0.03}$||$0.185_{-0.016}^{+0.016}$|0.12
VPHAS J0815−3625BH 2328DA31 870 ± 2108.04 ± 0.04|$9.79_{-0.06}^{+0.06}$|0.12 ± 0.03734 ± 40|$0.68_{-0.02}^{+0.02}$||$0.011_{-0.002}^{+0.002}$|0.10
VPHAS J0900−4556Platais 923DB19 040 ± 4508.13 ± 0.10|$10.94_{-0.14}^{+0.14}$|0.01 ± 0.05615 ± 59|$0.70_{-0.06}^{+0.06}$||$0.130_{-0.029}^{+0.029}$|0.11
VPHAS J1018−5752ASCC 5910DA17 430 ± 3907.79 ± 0.08|$10.66_{-0.12}^{+0.13}$|0.00 ± 0.041066 ± 86|$0.52_{-0.04}^{+0.04}$||$0.095_{-0.010}^{+0.010}$|0.00
VPHAS J1021−5732ASCC 5927DA30 110 ± 1608.56 ± 0.03|$10.79_{-0.05}^{+0.05}$|0.28 ± 0.04382 ± 27|$0.98_{-0.02}^{+0.02}$||$0.059_{-0.006}^{+0.006}$|0.10
VPHAS J1025−5841Loden 14321DA13 280 ± 2408.44 ± 0.04|$12.23_{-0.07}^{+0.07}$|0.12 ± 0.04263 ± 19|$0.89_{-0.03}^{+0.03}$||$0.580_{-0.028}^{+0.028}$|0.04
VPHAS J1029−5855Loden 14314DAHa35 000 ± 50008.00 ± 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 J1030−5900Loden 14322DA19 780 ± 2508.04 ± 0.04|$10.81_{-0.06}^{+0.06}$|0.07 ± 0.04565 ± 41|$0.65_{-0.02}^{+0.02}$||$0.084_{-0.011}^{+0.011}$|0.00
VPHAS J1103−5837NGC 353219DA23 910 ± 3608.87 ± 0.05|$11.89_{-0.11}^{+0.11}$|0.13 ± 0.07433 ± 54|$1.13_{-0.03}^{+0.03}$||$^{b}0.270_{-0.025}^{+0.034}$|
VPHAS J1104−5830NGC 35328DCa29 500 ± 3008.00 ± 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 J1105−5842NGC 353215DA14 230 ± 11608.16 ± 0.10|$11.64_{-0.16}^{+0.17}$|0.06 ± 0.04363 ± 36|$0.71_{-0.06}^{+0.06}$||$0.323_{-0.066}^{+0.086}$|0.11
VPHAS J1337−6121Platais 1014DA24 100 ± 5308.01 ± 0.08|$10.37_{-0.13}^{+0.13}$|0.20 ± 0.05709 ± 67|$0.64_{-0.04}^{+0.05}$||$0.032_{-0.005}^{+0.013}$|0.00
VPHAS J1344−6134Platais 1010DA49 670 ± 25207.92 ± 0.19|$8.87_{-0.37}^{+0.37}$|0.39 ± 0.061202 ± 169|$0.66_{-0.08}^{+0.09}$|0.002−0.81
VPHAS J1546−5233Johansson 112DA20 440 ± 5507.98 ± 0.09|$10.65_{-0.15}^{+0.15}$|0.12 ± 0.111052 ± 204|$0.62_{-0.04}^{+0.05}$||$0.063_{-0.006}^{+0.019}$|−0.01
VPHAS J1549−5251ASCC 8314DA20 320 ± 3908.05 ± 0.07|$10.77_{-0.11}^{+0.11}$|0.07 ± 0.10951 ± 165|$0.66_{-0.04}^{+0.04}$||$0.078_{-0.014}^{+0.017}$|0.01
VPHAS J1748−2914Ruprecht 13112DAHa8750 ± 12008.00 ± 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 J1800−2332Ruprecht 13921DA24 030 ± 3608.60 ± 0.05|$11.36_{-0.09}^{+0.09}$|0.24 ± 0.02165 ± 7|$0.99_{-0.03}^{+0.03}$||$0.153_{-0.019}^{+0.019}$|0.21
NameClusterS/NTypeTefflog gMgE(BV)dMWDτWDδτWD
(K)(cgs)(mag)(mag)(pc)(M)(Gyr)
VPHAS J0804−2809NGC 252720DA18 160 ± 2608.24 ± 0.05|$11.27_{-0.07}^{+0.09}$|0.05 ± 0.07630 ± 77|$0.77_{-0.03}^{+0.03}$||$0.185_{-0.016}^{+0.016}$|0.12
VPHAS J0815−3625BH 2328DA31 870 ± 2108.04 ± 0.04|$9.79_{-0.06}^{+0.06}$|0.12 ± 0.03734 ± 40|$0.68_{-0.02}^{+0.02}$||$0.011_{-0.002}^{+0.002}$|0.10
VPHAS J0900−4556Platais 923DB19 040 ± 4508.13 ± 0.10|$10.94_{-0.14}^{+0.14}$|0.01 ± 0.05615 ± 59|$0.70_{-0.06}^{+0.06}$||$0.130_{-0.029}^{+0.029}$|0.11
VPHAS J1018−5752ASCC 5910DA17 430 ± 3907.79 ± 0.08|$10.66_{-0.12}^{+0.13}$|0.00 ± 0.041066 ± 86|$0.52_{-0.04}^{+0.04}$||$0.095_{-0.010}^{+0.010}$|0.00
VPHAS J1021−5732ASCC 5927DA30 110 ± 1608.56 ± 0.03|$10.79_{-0.05}^{+0.05}$|0.28 ± 0.04382 ± 27|$0.98_{-0.02}^{+0.02}$||$0.059_{-0.006}^{+0.006}$|0.10
VPHAS J1025−5841Loden 14321DA13 280 ± 2408.44 ± 0.04|$12.23_{-0.07}^{+0.07}$|0.12 ± 0.04263 ± 19|$0.89_{-0.03}^{+0.03}$||$0.580_{-0.028}^{+0.028}$|0.04
VPHAS J1029−5855Loden 14314DAHa35 000 ± 50008.00 ± 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 J1030−5900Loden 14322DA19 780 ± 2508.04 ± 0.04|$10.81_{-0.06}^{+0.06}$|0.07 ± 0.04565 ± 41|$0.65_{-0.02}^{+0.02}$||$0.084_{-0.011}^{+0.011}$|0.00
VPHAS J1103−5837NGC 353219DA23 910 ± 3608.87 ± 0.05|$11.89_{-0.11}^{+0.11}$|0.13 ± 0.07433 ± 54|$1.13_{-0.03}^{+0.03}$||$^{b}0.270_{-0.025}^{+0.034}$|
VPHAS J1104−5830NGC 35328DCa29 500 ± 3008.00 ± 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 J1105−5842NGC 353215DA14 230 ± 11608.16 ± 0.10|$11.64_{-0.16}^{+0.17}$|0.06 ± 0.04363 ± 36|$0.71_{-0.06}^{+0.06}$||$0.323_{-0.066}^{+0.086}$|0.11
VPHAS J1337−6121Platais 1014DA24 100 ± 5308.01 ± 0.08|$10.37_{-0.13}^{+0.13}$|0.20 ± 0.05709 ± 67|$0.64_{-0.04}^{+0.05}$||$0.032_{-0.005}^{+0.013}$|0.00
VPHAS J1344−6134Platais 1010DA49 670 ± 25207.92 ± 0.19|$8.87_{-0.37}^{+0.37}$|0.39 ± 0.061202 ± 169|$0.66_{-0.08}^{+0.09}$|0.002−0.81
VPHAS J1546−5233Johansson 112DA20 440 ± 5507.98 ± 0.09|$10.65_{-0.15}^{+0.15}$|0.12 ± 0.111052 ± 204|$0.62_{-0.04}^{+0.05}$||$0.063_{-0.006}^{+0.019}$|−0.01
VPHAS J1549−5251ASCC 8314DA20 320 ± 3908.05 ± 0.07|$10.77_{-0.11}^{+0.11}$|0.07 ± 0.10951 ± 165|$0.66_{-0.04}^{+0.04}$||$0.078_{-0.014}^{+0.017}$|0.01
VPHAS J1748−2914Ruprecht 13112DAHa8750 ± 12008.00 ± 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 J1800−2332Ruprecht 13921DA24 030 ± 3608.60 ± 0.05|$11.36_{-0.09}^{+0.09}$|0.24 ± 0.02165 ± 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(BV) estimates.

bCooling age determined from Althaus et al. (2007) oxygen–neon core models.

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