\begin{table}
%\centering
\par
\caption{\label{tab:data}Supernovae used in this work, including their CMB-frame redshift $z_{{\rm CMB}}$, SALT2 fit parameters~$x_1$ and $c$, Hubble residuals $\Delta\mu_B$, and flux ratios $\mathcal{R}^{(c)}_{642/443}$.}
\small \begin{tabular}{llrrrrrl}
\hline\hline
Name& \multicolumn{1}{c}{$z_{{\rm CMB}}$} & \multicolumn{1}{c}{$x_1$}
& \multicolumn{1}{c}{$c$} & \multicolumn{1}{c}{$\Delta\mu_B$}
 & \multicolumn{1}{c}{$\mathcal{R}_{642/443}$} & \multicolumn{1}{c}{$\mathcal{R}^c_{642/443}$}
& Discovery \\
\hline
\em{Training SNe} \\
SN2005hc & 0.0449 & $1.21 \pm 0.66$ & $0.016 \pm 0.029$ & $0.113 \pm 0.058$ & $0.393 \pm 0.012$ & $0.385 \pm 0.012$ & SDSS-II; CBET 259 \\
SN2006dm & 0.0208$^{a}$ & $-2.79 \pm 0.38$ & $0.037 \pm 0.032$ & $0.522 \pm 0.111$ & $0.533 \pm 0.007$ & $0.511 \pm 0.007$ & LOSS; CBET 568 \\
SN2007bd & 0.0320$^{b}$ & $-2.90 \pm 0.46$ & $-0.066 \pm 0.026$ & $0.066 \pm 0.073$ & $0.487 \pm 0.010$ & $0.526 \pm 0.011$ & LOSS; CBET 914 \\
SN2007kk & 0.0406$^{c}$ & $-0.20 \pm 0.29$ & $0.058 \pm 0.021$ & $-0.046 \pm 0.060$ & $0.396 \pm 0.007$ & $0.370 \pm 0.006$ & LOSS; CBET 1096 \\
SNF20060908-004 & 0.0490 & $0.60 \pm 0.28$ & $0.047 \pm 0.022$ & $-0.121 \pm 0.229$ & $0.422 \pm 0.010$ & $0.400 \pm 0.010$ \\
SNF20061021-003 & 0.0615 & $-0.34 \pm 0.20$ & $0.088 \pm 0.017$ & $0.198 \pm 0.042$ & $0.489 \pm 0.024$ & $0.441 \pm 0.022$ \\
SNF20061111-002 & 0.0681 & $0.81 \pm 0.36$ & $0.121 \pm 0.020$ & $0.216 \pm 0.039$ & $0.479 \pm 0.023$ & $0.416 \pm 0.020$ \\
SNF20070424-003 & 0.0678 & $0.44 \pm 0.18$ & $0.045 \pm 0.018$ & $0.374 \pm 0.039$ & $0.465 \pm 0.040$ & $0.442 \pm 0.038$ \\
SNF20070531-011 & 0.0365 & $-2.77 \pm 0.39$ & $-0.047 \pm 0.025$ & $0.207 \pm 0.068$ & $0.495 \pm 0.016$ & $0.523 \pm 0.017$ \\
SNF20070630-006 & 0.0708 & $-0.13 \pm 0.17$ & $0.002 \pm 0.018$ & $0.057 \pm 0.039$ & $0.425 \pm 0.036$ & $0.424 \pm 0.036$ \\
SNF20070712-003 & 0.0770 & $0.16 \pm 0.27$ & $-0.050 \pm 0.018$ & $-0.125 \pm 0.146$ & $0.457 \pm 0.027$ & $0.485 \pm 0.029$ \\
SNF20070717-003 & 0.0858 & $-1.09 \pm 0.30$ & $0.060 \pm 0.022$ & $0.373 \pm 0.038$ & $0.586 \pm 0.056$ & $0.546 \pm 0.052$ \\
SNF20070727-016 & 0.0662 & $0.13 \pm 0.22$ & $-0.066 \pm 0.019$ & $-0.376 \pm 0.048$ & $0.349 \pm 0.015$ & $0.377 \pm 0.016$ \\
SNF20070803-005 & 0.0302 & $0.75 \pm 0.28$ & $0.060 \pm 0.027$ & $-0.221 \pm 0.080$ & $0.354 \pm 0.006$ & $0.330 \pm 0.006$ \\
SNF20070806-026 & 0.0439 & $-2.48 \pm 0.22$ & $-0.053 \pm 0.018$ & $0.272 \pm 0.057$ & $0.531 \pm 0.014$ & $0.565 \pm 0.015$ \\
SNF20070810-004 & 0.0823 & $-0.50 \pm 0.20$ & $0.005 \pm 0.017$ & $0.125 \pm 0.034$ & $0.460 \pm 0.023$ & $0.457 \pm 0.023$ \\
SNF20070818-001 & 0.0742 & $-0.68 \pm 0.58$ & $0.096 \pm 0.027$ & $0.201 \pm 0.044$ & $0.499 \pm 0.031$ & $0.445 \pm 0.028$ \\
SNF20071015-000 & 0.0373 & $0.76 \pm 0.31$ & $0.521 \pm 0.025$ & $1.470 \pm 0.067$ & $0.804 \pm 0.035$ & $0.437 \pm 0.019$ \\
SNF20071021-000 & 0.0262 & $-0.90 \pm 0.22$ & $0.126 \pm 0.026$ & $0.471 \pm 0.088$ & $0.572 \pm 0.011$ & $0.494 \pm 0.009$ \\
SNF20080510-001 & 0.0726 & $-0.44 \pm 0.26$ & $-0.032 \pm 0.019$ & $0.043 \pm 0.154$ & $0.481 \pm 0.035$ & $0.499 \pm 0.037$ \\
SNF20080512-010 & 0.0635 & $-3.53 \pm 0.42$ & $-0.036 \pm 0.023$ & $0.221 \pm 0.043$ & $0.490 \pm 0.029$ & $0.512 \pm 0.030$ \\
SNF20080514-002 & 0.0231$^{d}$ & $-2.04 \pm 0.16$ & $-0.079 \pm 0.018$ & $0.234 \pm 0.096$ & $0.478 \pm 0.007$ & $0.524 \pm 0.007$ \\
SNF20080516-022 & 0.0747$^{d}$ & $-0.26 \pm 0.16$ & $-0.058 \pm 0.015$ & $-0.008 \pm 0.035$ & $0.443 \pm 0.048$ & $0.474 \pm 0.051$ \\
SNF20080522-011 & 0.0385 & $1.54 \pm 0.27$ & $0.045 \pm 0.019$ & $-0.152 \pm 0.061$ & $0.456 \pm 0.010$ & $0.433 \pm 0.010$ \\
SNF20080626-002 & 0.0232 & $0.61 \pm 0.31$ & $-0.012 \pm 0.025$ & $-0.048 \pm 0.099$ & $0.426 \pm 0.005$ & $0.432 \pm 0.005$ \\
SNF20080714-008 & 0.0767 & $-0.43 \pm 0.23$ & $0.186 \pm 0.021$ & $0.833 \pm 0.147$ & $0.634 \pm 0.063$ & $0.510 \pm 0.050$ \\
SNF20080803-000 & 0.0568 & $0.28 \pm 0.36$ & $0.147 \pm 0.028$ & $0.520 \pm 0.053$ & $0.573 \pm 0.035$ & $0.482 \pm 0.030$ \\
SNF20080822-005 & 0.0704 & $0.58 \pm 1.07$ & $0.003 \pm 0.029$ & $-0.093 \pm 0.058$ & $0.368 \pm 0.016$ & $0.367 \pm 0.016$ \\
\hline
\em{Validation SNe} \\
SN2004ef & 0.0298$^{e}$ & $-2.40 \pm 0.24$ & $0.152 \pm 0.021$ & $0.594 \pm 0.078$ & $0.645 \pm 0.016$ & $0.540 \pm 0.013$ & Boles, Armstrong; IAUC 8399 \\
SN2005M & 0.0230$^{f}$ & $0.74 \pm 0.34$ & $0.124 \pm 0.026$ & $0.260 \pm 0.101$ & $0.470 \pm 0.008$ & $0.407 \pm 0.007$ & Puckett \& George; IAUC 8470 \\
SN2005di & 0.0242$^{g}$ & $-1.01 \pm 0.25$ & $0.503 \pm 0.037$ & $1.703 \pm 0.102$ & $0.918 \pm 0.041$ & $0.509 \pm 0.023$ & LOSS; CBET 0198 \\
SN2007cq & 0.0245 & $-0.89 \pm 0.25$ & $-0.021 \pm 0.027$ & $-0.135 \pm 0.095$ & $0.406 \pm 0.006$ & $0.416 \pm 0.006$ & Orff \& Newton; CBET 983 \\
SN2007qe & 0.0227 & $-0.36 \pm 0.28$ & $0.119 \pm 0.029$ & $0.302 \pm 0.102$ & $0.462 \pm 0.008$ & $0.402 \pm 0.007$ & ROTSE; CBET 1138 \\
SN2008ec & 0.0151$^{h}$ & $-1.34 \pm 0.22$ & $0.216 \pm 0.028$ & $0.708 \pm 0.149$ & $0.636 \pm 0.006$ & $0.494 \pm 0.005$ & LOSS; CBET 1437 \\
SNF20060511-014 & 0.0467 & $-1.48 \pm 0.23$ & $-0.002 \pm 0.029$ & $0.055 \pm 0.068$ & $0.496 \pm 0.023$ & $0.497 \pm 0.023$ \\
SNF20060526-003 & 0.0787 & $-0.19 \pm 0.56$ & $0.031 \pm 0.029$ & $0.139 \pm 0.042$ & $0.461 \pm 0.025$ & $0.445 \pm 0.024$ \\
SNF20060621-015 & 0.0543 & $0.07 \pm 0.34$ & $-0.065 \pm 0.021$ & $-0.187 \pm 0.047$ & $0.422 \pm 0.012$ & $0.455 \pm 0.013$ \\
SNF20060912-000 & 0.0722 & $-0.13 \pm 0.91$ & $0.141 \pm 0.027$ & $0.191 \pm 0.053$ & $0.498 \pm 0.023$ & $0.423 \pm 0.020$ \\
SNF20060919-007 & 0.0694$^{i}$ & $-0.38 \pm 0.29$ & $-0.008 \pm 0.020$ & $0.015 \pm 0.038$ & $0.459 \pm 0.021$ & $0.463 \pm 0.022$ \\
SNF20061020-000 & 0.0379 & $-2.28 \pm 0.23$ & $0.056 \pm 0.024$ & $0.385 \pm 0.064$ & $0.556 \pm 0.017$ & $0.520 \pm 0.016$ \\
SNF20070403-001 & 0.0815$^{d}$ & $-1.90 \pm 0.30$ & $0.035 \pm 0.016$ & $0.191 \pm 0.034$ & $0.496 \pm 0.042$ & $0.476 \pm 0.041$ \\
\hline
SNF20070427-001 & 0.0778$^{d}$ & $0.46 \pm 0.31$ & $-0.115 \pm 0.021$ & $-0.088 \pm 0.036$ & $0.421 \pm 0.025$ & $0.482 \pm 0.029$ \\
SNF20070506-006 & 0.0355 & $0.49 \pm 0.15$ & $-0.017 \pm 0.018$ & $-0.329 \pm 0.065$ & $0.413 \pm 0.011$ & $0.421 \pm 0.011$ \\
SNF20070701-005 & 0.0682 & $-0.88 \pm 0.41$ & $0.039 \pm 0.030$ & $-0.069 \pm 0.050$ & $0.405 \pm 0.024$ & $0.387 \pm 0.023$ \\
SNF20070725-001 & 0.0668 & $0.45 \pm 0.21$ & $-0.105 \pm 0.022$ & $-0.266 \pm 0.050$ & $0.461 \pm 0.021$ & $0.521 \pm 0.024$ \\
SNF20070802-000 & 0.0646 & $0.16 \pm 0.23$ & $0.125 \pm 0.017$ & $0.366 \pm 0.040$ & $0.575 \pm 0.043$ & $0.496 \pm 0.037$ \\
SNF20070817-003 & 0.0630 & $-1.20 \pm 0.24$ & $-0.009 \pm 0.018$ & $0.321 \pm 0.177$ & $0.547 \pm 0.030$ & $0.553 \pm 0.030$ \\
SNF20080323-009 & 0.0834$^{d}$ & $-0.73 \pm 0.23$ & $-0.028 \pm 0.024$ & $0.033 \pm 0.037$ & $0.429 \pm 0.031$ & $0.443 \pm 0.032$ \\
SNF20080510-005 & 0.0850 & $2.29 \pm 0.41$ & $0.123 \pm 0.021$ & $0.191 \pm 0.133$ & $0.455 \pm 0.028$ & $0.395 \pm 0.025$ \\
SNF20080516-000 & 0.0726 & $0.88 \pm 0.24$ & $-0.007 \pm 0.019$ & $-0.076 \pm 0.155$ & $0.415 \pm 0.025$ & $0.419 \pm 0.025$ \\
SNF20080522-000 & 0.0460 & $0.96 \pm 0.20$ & $0.076 \pm 0.019$ & $-0.225 \pm 0.242$ & $0.363 \pm 0.012$ & $0.332 \pm 0.011$ \\
SNF20080531-000 & 0.0369 & $-0.08 \pm 0.33$ & $0.037 \pm 0.022$ & $0.282 \pm 0.064$ & $0.504 \pm 0.014$ & $0.482 \pm 0.014$ \\
SNF20080610-000 & 0.0789$^{d}$ & $-0.48 \pm 0.23$ & $-0.005 \pm 0.019$ & $0.150 \pm 0.038$ & $0.477 \pm 0.029$ & $0.480 \pm 0.030$ \\
SNF20080612-003 & 0.0329 & $0.15 \pm 0.20$ & $-0.011 \pm 0.022$ & $-0.284 \pm 0.072$ & $0.450 \pm 0.011$ & $0.456 \pm 0.011$ \\
SNF20080614-010 & 0.0752$^{d}$ & $-2.89 \pm 0.18$ & $-0.002 \pm 0.018$ & $0.340 \pm 0.036$ & $0.488 \pm 0.037$ & $0.489 \pm 0.037$ \\
SNF20080623-001 & 0.0427 & $-0.70 \pm 0.18$ & $-0.050 \pm 0.017$ & $0.262 \pm 0.260$ & $0.483 \pm 0.013$ & $0.512 \pm 0.014$ \\
SNF20080720-001 & 0.0200 & $0.30 \pm 0.26$ & $0.650 \pm 0.025$ & $1.436 \pm 0.156$ & $0.861 \pm 0.015$ & $0.402 \pm 0.007$ \\
SNF20080810-001 & 0.0426 & $-1.37 \pm 0.26$ & $0.038 \pm 0.026$ & $0.274 \pm 0.060$ & $0.529 \pm 0.016$ & $0.506 \pm 0.015$ \\
\hline
\em{Literature SNe} \\
SN1998V & $0.0172$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.412 \pm 0.167$  & $0.423 \pm 0.017$  & \multicolumn{1}{c}{...}  & Armstrong; IAUC 6841 \\
SN1998aq & $0.0045$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.002 \pm 0.558$  & $0.404 \pm 0.013$  & \multicolumn{1}{c}{...}  & Armstrong; IAUC 6875 \\
SN1998bp & $0.0102$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $1.210 \pm 0.217$  & $0.723 \pm 0.106$  & \multicolumn{1}{c}{...}  & Armstrong; IAUC 6890 \\
SN1998de & $0.0156$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $2.303 \pm 0.141$  & $0.992 \pm 0.239$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 6977 \\
SN1998dh & $0.0077$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.515 \pm 0.270$  & $0.553 \pm 0.190$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 6978 \\
SN1998ec & $0.0201$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.628 \pm 0.156$  & $0.667 \pm 0.024$  & \multicolumn{1}{c}{...}  & BAO SN Survey; IAUC 7022 \\
SN1998eg & $0.0235$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.467 \pm 0.141$  & $0.550 \pm 0.190$  & \multicolumn{1}{c}{...}  & Boles; IAUC 7033 \\
SN1998es & $0.0096$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $-0.108 \pm 0.212$  & $0.452 \pm 0.012$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7050 \\
SN1999aa & $0.0153$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $-0.231 \pm 0.155$  & $0.356 \pm 0.023$  & \multicolumn{1}{c}{...}  & Arbour; IAUC 7108 \\
SN1999ac & $0.0098$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.096 \pm 0.235$  & $0.419 \pm 0.004$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7144 \\
SN1999cc & $0.0315$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.232 \pm 0.073$  & $0.519 \pm 0.033$  & \multicolumn{1}{c}{...}  & Schwartz; IAUC 7163 \\
SN1999cl & $0.0087$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $1.141 \pm 0.292$  & $1.890 \pm 0.245$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7185 \\
SN1999ej & $0.0128$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.823 \pm 0.195$  & $0.569 \pm 0.005$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7286 \\
SN1999gd & $0.0193$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $1.302 \pm 0.162$  & $0.946 \pm 0.190$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7319 \\
SN2000dk & $0.0164$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.225 \pm 0.136$  & $0.545 \pm 0.126$  & \multicolumn{1}{c}{...}  & LOSS; IAUC 7493 \\
SN2000fa & $0.0218$  & \multicolumn{1}{c}{...} & \multicolumn{1}{c}{...}  & $0.004 \pm 0.151$  & $0.433 \pm 0.093$  & \multicolumn{1}{c}{...}  & LOTOSS; IAUC 7533 \\
\hline
\end{tabular}
\medskip
{\it Notes}: The Hubble residuals are {\em before} any corrections for $c$, $x_1$, or $\mathcal{R}$. The peak magnitudes for the literature SNe Hubble diagram fits are from \cite{HickenLC} and \cite{Jha_LC}, which did not use SALT2. The $\mathcal{R}_{642/443}$ Hubble diagram fits were performed separately for the literature and SNfactory observations; the reported $\Delta\mu_B$ residuals are with respect to the individual fits. The full table available from CDS includes all flux ratios from Table~\ref{tab:results} for the SNe observed by the SNfactory.  Discoveries and redshifts are from SNfactory observations except as otherwise noted. Literature SNe redshifts are via \cite{HickenLC} and \cite{Jha_LC}. Other redshift citations via NED except for SDSS: \\
 $^{a}$ Theureau, G., et~al. 1998, \aaps, 130, 333;  $^{b}$~Falco, E.~E., et~al. 1999, \pasp, 111, 438;  $^{c}$~Huchra, J.~P., Vogeley, M.~S., \& Geller, M.~J. 1999, \apjs, 121, 287;  $^{d}$~SDSS;
 $^{e}$~O'Neil, K. 2004, \aj, 128, 2080;  $^{f}$~de Vaucouleurs, G., et~al. 1992, VizieR Online Data Calalog, 7137, 0;  $^{g}$~Mathewson, D.~S., \& Ford, V.~L. 1996, \apjs, 107, 97;  $^{h}$~Keel, W.~C. 1996, \apjs, 106, 27;  $^{i}$~Jones, D.~H., et~al. 2005, PASA, 22, 277. 
\end{table}