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Table 7

SDSS-WDMS binaries in common with Farihi et al. (2010).

WD-Name SDSS-Name Type # spec Δt [d]
Not resolved by HST
WD0303 – 007 SDSS J030607.18 – 003114.4 pceb 4 2991
WD0908 + 226 SDSS J091143.09 + 222748.8 pceb 4 5
WD1051 + 516 SDSS J105421.97 + 512254.2 pceb 3 1089
WD1140 + 004 SDSS J114312.57 + 000926.51 pceb 3 2551
WD1339 + 606 SDSS J134100.03 + 602610.4 wide 3 0.03
WD1433 + 538 SDSS J143443.24 + 533521.2 pceb 3 1157
WD1458 + 171 SDSS J150019.33 + 165914.4 wide 2 0.01
WD1522 + 508 SDSS J152425.21 + 504009.72 pceb 3 1007
Resolved by HST
WD0257 – 005 SDSS J030024.57 – 002342.0 wide 2 10
WD1049 + 103 SDSS J105227.72 + 100337.6 wide 3 0.03
WD1106 + 316 SDSS J110843.03 + 312356.1 wide 3 0.03
WD1108 + 325 SDSS J111045.90 + 321447.2 - 0 0
WD1133 + 489 SDSS J113609.59 + 484318.9 - 0 0
WD1218 + 497 SDSS J122105.34 + 492720.5 wide 3 0.03
WD1236 – 004 SDSS J123836.34 – 004042.2 wide 4 3197
WD1419 + 576 SDSS J142105.31 + 572457.1 wide 4 0.05
WD1443 + 336 SDSS J144600.72 + 332849.9 wide 3 0.02
WD1622 + 323 SDSS J162449.00 + 321702.0 wide 5 1438
WD1833 + 644 SDSS J183329.18 + 643151.7 wide 9 43

Notes. “Type” is our classification based on the radial velocity information. We list the number of spectra used for the classification and the time span between them. Two of the systems unresolved by HST only have SDSS subspectra taken within  < 1 h.

(1)

Porb = 9.274 h.

(2)

Porb = 14.15 h.

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