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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