Table 1: The characteristics of our thirteen DB + dM and two DC + dM binaries are given in this table. The uncertainties are about one subtype for the dM star and about 4000 Kelvin in WD temperature for a fixed dM spectral type. The temperatures are shown as given in Kleinman et al. (2004) for the best fit template WD. a See Sect. 3. b These objects are DC + dM binaries.
Name g u-g g-r r-i i-z $T_{\rm WD}$ dM D (pc) $\chi^2$
SDSS J075235.79+401339.0 20.01 0.05 0.01 0.58 0.39 30 252 M3V 1544 1.64
SDSS J080636.85+251912.1 19.61 0.07 0.21 0.79 0.60 24 266 M3V 1045 1.68
SDSS J093645.14+420625.6a 20.37 -0.09 -0.14 0.42 0.07 15 919 M5V 860 2.01
SDSS J100636.39+563346.8 19.42 0.10 0.28 0.72 0.49 14 575 M4V 531 3.70
SDSS J102131.55+511622.9 18.27 -0.25 -0.37 0.14 0.35 30 252 M4V 700 1.56
SDSS J113609.59+484318.9a 16.80 -0.38 -0.54 -0.16 0.14 38 211 M6V 354 4.00
SDSS J134135.23+612128.7 19.14 -0.10 0.12 0.50 0.48 30 694 M3V 1054 2.20
SDSS J143222.06+611231.1 18.53 0.02 -0.08 0.49 0.60 36 815 M3V 879 3.56
SDSS J144258.47+001031.5a 18.35 0.04 0.08 0.80 0.72 30 694 M3V 674 11.22
SDSS J150118.40+042232.3a 19.57 0.02 -0.01 0.49 0.48 26 020 M3V 1220 2.42
SDSS J162329.50+355427.2 18.77 0.02 0.22 0.65 0.53 24 266 M3V 695 3.46
SDSS J220313.29+113236.0 19.34 -0.08 -0.10 0.22 0.45 30 694 M4V 1085 2.04
SDSS J232438.31-093106.5 18.64 -0.08 -0.16 0.41 0.66 36 815 M3V 911 3.45
SDSS J074425.42+353040.8a,b 18.91 0.23 0.03 0.70 0.68 15 700 M4V 481 7.14
SDSS J113457.72+655408.7a,b 18.15 0.10 0.02 0.70 0.75 12 500 M4V 278 9.59


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