Table 1.

Parameters of the 11 open clusters proposed to host the white dwarf candidates. We add a tickmark to the last column if at least one new cluster member is identified (Section 4).

NameRADecbr1r2Da, bE(BV)a, b|$t_{\rm {oc}}^{a,b}$|[Fe/H]|$M_{\rm {oc}}^{c}$|New
(h:m:s)(°:′:″)(deg)(deg)(arcmin)(pc)(mag)(Myr)log (M)
NGC 252708:04:58−28:08:48246.091.859, 20601, 6420.04445, 800−0.10, 0.202.5|$\checkmark$|
BH 2308:14:24−36:23:00254.08−0.969, 20414, 4800.062501.7
Platais 909:13:47−43:44:24266.873.3860, 126174, 2000.00100
ASCC 5910:20:13−57:39:00283.78−0.5112, 20509, 5500.05290, 400
Loden 14310:28:54−58:47:00285.35−0.8610, 18600, 6160.10, 0.12281, 288|$\checkmark$|
NGC 353211:05:39−58:45:12289.571.3512, 25492d0.03, 0.04300d0.022.6|$\checkmark$|
Platais 1013:43:28−59:07:18309.573.0831, 602460.00100, 210
Johansson 115:46:20−52:22:54327.901.8011, 18570, 8690.17200, 500|$\checkmark$|
ASCC 8315:50:13−52:48:00328.101.1112, 20600, 6190.12, 0.15125, 250
Ruprecht 13117:49:15−29:15:000.14−0.845, 10600, 6140.1014801.1|$\checkmark$|
Ruprecht 13918:01:03−23:32:006.41−0.245, 10550, 5930.10, 0.151120
NameRADecbr1r2Da, bE(BV)a, b|$t_{\rm {oc}}^{a,b}$|[Fe/H]|$M_{\rm {oc}}^{c}$|New
(h:m:s)(°:′:″)(deg)(deg)(arcmin)(pc)(mag)(Myr)log (M)
NGC 252708:04:58−28:08:48246.091.859, 20601, 6420.04445, 800−0.10, 0.202.5|$\checkmark$|
BH 2308:14:24−36:23:00254.08−0.969, 20414, 4800.062501.7
Platais 909:13:47−43:44:24266.873.3860, 126174, 2000.00100
ASCC 5910:20:13−57:39:00283.78−0.5112, 20509, 5500.05290, 400
Loden 14310:28:54−58:47:00285.35−0.8610, 18600, 6160.10, 0.12281, 288|$\checkmark$|
NGC 353211:05:39−58:45:12289.571.3512, 25492d0.03, 0.04300d0.022.6|$\checkmark$|
Platais 1013:43:28−59:07:18309.573.0831, 602460.00100, 210
Johansson 115:46:20−52:22:54327.901.8011, 18570, 8690.17200, 500|$\checkmark$|
ASCC 8315:50:13−52:48:00328.101.1112, 20600, 6190.12, 0.15125, 250
Ruprecht 13117:49:15−29:15:000.14−0.845, 10600, 6140.1014801.1|$\checkmark$|
Ruprecht 13918:01:03−23:32:006.41−0.245, 10550, 5930.10, 0.151120

References: aDias et al. (2002); bKharchenko et al. (2013); cPiskunov et al. (2008); dClem et al. (2011).

Table 1.

Parameters of the 11 open clusters proposed to host the white dwarf candidates. We add a tickmark to the last column if at least one new cluster member is identified (Section 4).

NameRADecbr1r2Da, bE(BV)a, b|$t_{\rm {oc}}^{a,b}$|[Fe/H]|$M_{\rm {oc}}^{c}$|New
(h:m:s)(°:′:″)(deg)(deg)(arcmin)(pc)(mag)(Myr)log (M)
NGC 252708:04:58−28:08:48246.091.859, 20601, 6420.04445, 800−0.10, 0.202.5|$\checkmark$|
BH 2308:14:24−36:23:00254.08−0.969, 20414, 4800.062501.7
Platais 909:13:47−43:44:24266.873.3860, 126174, 2000.00100
ASCC 5910:20:13−57:39:00283.78−0.5112, 20509, 5500.05290, 400
Loden 14310:28:54−58:47:00285.35−0.8610, 18600, 6160.10, 0.12281, 288|$\checkmark$|
NGC 353211:05:39−58:45:12289.571.3512, 25492d0.03, 0.04300d0.022.6|$\checkmark$|
Platais 1013:43:28−59:07:18309.573.0831, 602460.00100, 210
Johansson 115:46:20−52:22:54327.901.8011, 18570, 8690.17200, 500|$\checkmark$|
ASCC 8315:50:13−52:48:00328.101.1112, 20600, 6190.12, 0.15125, 250
Ruprecht 13117:49:15−29:15:000.14−0.845, 10600, 6140.1014801.1|$\checkmark$|
Ruprecht 13918:01:03−23:32:006.41−0.245, 10550, 5930.10, 0.151120
NameRADecbr1r2Da, bE(BV)a, b|$t_{\rm {oc}}^{a,b}$|[Fe/H]|$M_{\rm {oc}}^{c}$|New
(h:m:s)(°:′:″)(deg)(deg)(arcmin)(pc)(mag)(Myr)log (M)
NGC 252708:04:58−28:08:48246.091.859, 20601, 6420.04445, 800−0.10, 0.202.5|$\checkmark$|
BH 2308:14:24−36:23:00254.08−0.969, 20414, 4800.062501.7
Platais 909:13:47−43:44:24266.873.3860, 126174, 2000.00100
ASCC 5910:20:13−57:39:00283.78−0.5112, 20509, 5500.05290, 400
Loden 14310:28:54−58:47:00285.35−0.8610, 18600, 6160.10, 0.12281, 288|$\checkmark$|
NGC 353211:05:39−58:45:12289.571.3512, 25492d0.03, 0.04300d0.022.6|$\checkmark$|
Platais 1013:43:28−59:07:18309.573.0831, 602460.00100, 210
Johansson 115:46:20−52:22:54327.901.8011, 18570, 8690.17200, 500|$\checkmark$|
ASCC 8315:50:13−52:48:00328.101.1112, 20600, 6190.12, 0.15125, 250
Ruprecht 13117:49:15−29:15:000.14−0.845, 10600, 6140.1014801.1|$\checkmark$|
Ruprecht 13918:01:03−23:32:006.41−0.245, 10550, 5930.10, 0.151120

References: aDias et al. (2002); bKharchenko et al. (2013); cPiskunov et al. (2008); dClem et al. (2011).

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