Open Access
Table B.1
Our WD sample and observations used in the spectral analysis.
WD Name(a) | Other Name | Program ID (FUSE) | Proposal ID (HST) | Optical(b) |
---|---|---|---|---|
DAO | ||||
Longmore 1 | P133 | − | UVES | |
0439+466 | LS V +46 21 | M107 | 8638 | G10 |
0500–156 | Abell 7 | B052 | − | G10 |
0615+556 | PuWe 1 | B052 | − | G10 |
0823+316 | Ton 320 | B053 | − | G10 |
0834+500 | PG 0834+501 | B053 | − | G10 |
0851+090 | Abell 31 | B052 | − | UVES |
1111+552 | NGC 3587 | B052 | − | - |
1214+267 | LB 2 | B053 | − | G10 |
1253+378 | HZ 34 | B053 | − | G10 |
1957+225 | NGC 6853 | M107 | 8638 | G10 |
2226–210 | NGC 7293 | C177 | 8638 | G10 |
2342+806 | GD 561 | B052 | 8329 | G10 |
DA | ||||
0027–636 | RE J0029–632 | Z903 | − | G11 |
0229–481 | LB 1628 | M105 | − | G11 |
0232+035 | Feige 24 | P104 | 7755 | G11 |
0311+480 | KPD 0311+4801 | Z904 | − | G10 |
0343–007 | KUV03439–0048 | E568 | − | G11 |
0455–282 | RE J0457–280 | P104 | 14791 | G10 |
0615+655 | HS 0615+6535 | E568 | 8636 | G10 |
0621–376 | RE J0623–374 | P104 | 14791 | G10, UVES |
0939+262 | Ton 21 | − | 8179 | G11 |
1056+516 | LB 1919 | D003 | − | G11, SDSS |
1342+443 | PG 1342+444 | A034 | − | G11, SDSS |
1738+669 | RE J1738+665 | M105 | 8179 | G10 |
1827+778 | HS 1827+7753 | E568 | − | G11, SDSS |
2046+396 | KPD 2046+3940 | E568 | − | G11 |
2146–433 | MCT2146–4320 | Z903 | − | G10 |
2211–495 | RE J2214–491 | M103 | 14791 | G10, UVES |
2218+706 | DeHt 5 | A034 | 8179 | G10 |
2350–706 | HD 223816 | B120, A054 | − | − |
2353+026 | PG 2353+027 | E568 | − | G11 |
Notes. (a) WD names from McCook & Sion (1999). (b) G10 and G11 refer to MWDD spectra used in Gianninas et al. (2010, 2011), respectively.
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