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tab_lg_sample_prop.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{cllllllr}
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\tablewidth{0pt}
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%\tabletypesize{\footnotesize}
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\tabletypesize{\small}
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%\tabletypesize{\scriptsize}
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%\tabletypesize{\tiny}
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%\rotate
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\tablewidth{0pt}
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\tablecolumns{7}
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\tablecaption{Properties of the Low-Gravity Optical-NIR Template Sample\label{tab:lg_sample_prop}}
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\tablehead{
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\colhead{} & \multicolumn{6}{c}{$J-K_S$} & \colhead{} \\
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\cline{2-7} \\
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\colhead{Optical} & \colhead{} & \colhead{1st/2nd} & \colhead{} & \colhead{} & \colhead{3rd/4th} & \colhead{} & \colhead{No. of}\\
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\colhead{Spectral Type} & \colhead{Min} & \colhead{Quartile} & \colhead{Median} & \colhead{Mean} & \colhead{Quartile} & \colhead{Max} & \colhead{Objects}
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}
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\startdata
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\cutinhead{$\gamma$-type objects}
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L0$\gamma$ & 1.44 & 1.55 & 1.64 & 1.64 & 1.74 & 1.80 & 8 \\
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L1$\gamma$ & 1.65 & 1.67 & 1.69 & 1.68 & 1.69 & 1.69 & 3 \\
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L2$\gamma$ & 1.91 & 1.94 & 1.96 & 1.96 & 1.98 & 2.00 & 2 \\
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L3$\gamma$ & 1.65 & 1.83 & 2.01 & 1.89 & 2.01 & 2.01 & 3 \\
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L4$\gamma$ & 1.93 & 1.95 & 2.02 & 2.12 & 2.23 & 2.48 & 5 \\
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\cutinhead{$\beta$-type objects}
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L0$\beta$ & 1.34 & 1.40 & 1.46 & 1.42 & 1.46 & 1.46 & 3 \\
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L1$\beta$ & 1.34 & 1.36 & 1.38 & 1.38 & 1.41 & 1.43 & 2 \\
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\cutinhead{Combined $\beta$- and $\gamma$-type objects}
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L1$\gamma$ \& L1$\beta$ & 1.34 & 1.43 & 1.65 & 1.56 & 1.69 & 1.69 & 5 \\
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L0$\gamma$ \& L0$\beta$ & 1.34 & 1.46 & 1.57 & 1.58 & 1.71 & 1.80 & 11 \\
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\enddata
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\tablecomments{Values describing the $J-K_S$ color distribution of the objects included in the low gravity spectral templates. The minimum, maximum, median, mean, and boundaries of the quartiles are listed in addition to the number of objects included in each template. These values are plotted in Figure~\ref{fig:JK_colors}. For L0 and L1, where we have both $\beta$ and $\gamma$ low-gravity objects, the statistics are listed for the subgroups individually (8 and 3 objects for L0, 3 and 2 objects for L1) and combined (11 total for L0 and 5 total for L1). The combined low-gravity stats are shown in Figure~\ref{fig:JK_colors}.}
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\end{deluxetable}

tab_lowg_excluded.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{lllllllll}
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\tabletypesize{\tiny}
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%\rotate
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\tablewidth{0pt}
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\tablecolumns{8}
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\tablecaption{Low-Gravity L Dwarfs Excluded from the Low-Gravity Template Sample\label{tab:lowg_excluded}}
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\tablehead{ \colhead{} & \colhead{} & \multicolumn{2}{c}{2MASS} \\
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\cline{3-4} \\
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\colhead{} & \colhead{Other} & \colhead{} & \colhead{} & \colhead{Optical} & \colhead{Sp. Type} & \colhead{SpeX Prism} & \colhead{Other} & \colhead{Reject}\\
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\colhead{Object} & \colhead{Name} & \colhead{$J$} & \colhead{$J-K_S$} & \colhead{Sp. Type} & \colhead{Ref.} & \colhead{Ref.} & \colhead{Refs.\tablenotemark{a}} & \colhead{Reason}
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}
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\startdata
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03483060+2244500 & Roque 25 & 17.79 $\pm$ 0.25 & 1.44 $\pm$ 0.354 & L0$\beta$ & \cite{Kirkpatrick08} & This Paper & \cite{Martin98} & noisy NIR \\
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04062677-3812102 & & 16.768 $\pm$ 0.126 & 1.655 $\pm$ 0.172 & L0$\gamma$ & \cite{Kirkpatrick10} & \cite{Kirkpatrick10} & \cite{Kirkpatrick10} & noisy NIR \\
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\enddata
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\tablecomments{Low gravity L dwarfs not included in templates and are shown in Figure~\ref{fig:lowg_excluded}.}
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\tablenotetext{a}{References listed are not exhaustive and pertain to discovery and spectral data.}
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\end{deluxetable}

tab_lowg_standards.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{llllll}
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%\tablewidth{0pt}
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%\tabletypesize{\footnotesize}
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%\tabletypesize{\small}
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\tabletypesize{\scriptsize}
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%\tabletypesize{\tiny}
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%\rotate
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\tablewidth{0pt}
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\tablecolumns{5}
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\tablecaption{Proposed Revised Set of L Dwarf NIR Spectral Standards\label{tab:standards}}
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\tablehead{ \multicolumn{3}{c}{2MASS} \\
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\cline{1-3} & \colhead{} & \colhead{} & \colhead{Sp.} & \colhead{} \\
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\colhead{Designation} & \colhead{$J$} & \colhead{$J-K_S$} & \colhead{Type} &
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\colhead{Refs.}
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}
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\startdata
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\multicolumn{5}{c}{Field Gravity} \\
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\hline \\
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03454316+2540233 & 13.997$\pm$0.027 & 1.325$\pm$0.036 & L0 & \cite{K99} \\
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21304464$-$0845205 & 14.137$\pm$0.032 & 1.322$\pm$0.046 & L1 & \cite{Kirkpatrick08,Reid08} \\
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04082905$-$1450334\tablenotemark{a} & 14.222$\pm$0.030 & 1.405$\pm$0.038 & L2 & \cite{Wilson01_thesis,Cruz03}\\
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15065441+1321060 & 13.365$\pm$0.023 & 1.624$\pm$0.030 & L3 & \cite{NN} \\
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21580457$-$1550098 & 15.040$\pm$0.040 & 1.855$\pm$0.054 & L4 & \cite{Cruz07, Kirkpatrick08} \\
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08350622+1953050 & 16.094$\pm$0.075 & 1.775$\pm$0.090 & L5 & \cite{Chiu06,Kirkpatrick10} \\
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21373742+0808463\tablenotemark{b} & 14.774$\pm$0.032 & 1.755$\pm$0.042 & L5 & \cite{Reid08} \\
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10101480$-$0406499 & 15.508$\pm$0.059 & 1.889$\pm$0.075 & L6 & \cite{Cruz03,Cruz07} \\
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08251968+2115521\tablenotemark{c} & 15.100$\pm$0.034 & 2.072$\pm$0.043 & L7.5 & \cite{K00} \\
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16322911+1904407 & 15.867$\pm$0.070 & 1.864$\pm$0.085 & L8 & \cite{K99} \\
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\cutinhead{Low Gravity $\beta$} \\
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15525906+2948485\tablenotemark{d} & 13.478$\pm$0.026 & 1.456$\pm$0.038 & L0$\beta$ & \cite{Reid08,Wilson03} \\
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02271036$-$1624479 & 13.573$\pm$0.023 & 1.430$\pm$0.038 & L1$\beta$ & \cite{Reid08,Deacon05} \\
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\cutinhead{Low Gravity $\gamma$} \\
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01415823$-$4633574 & 14.832$\pm$0.043 & 1.735$\pm$0.054 & L0$\gamma$ & \cite{Cruz09_lowg, Kirkpatrick06} \\
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17111353+2326333 & 14.499$\pm$0.026 & 1.443$\pm$0.037 & L0$\gamma$ & \cite{Cruz07} \\
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05184616$-$2756457\tablenotemark{d} & 15.262$\pm$0.043 & 1.647$\pm$0.059 & L1$\gamma$ & \cite{Cruz07} \\
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05361998$-$1920396\tablenotemark{d} & 15.768$\pm$0.074 & 1.914$\pm$0.097 & L2$\gamma$ & \cite{Cruz07} \\
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22081363+2921215\tablenotemark{d} & 15.797$\pm$0.085 & 1.649$\pm$0.112 & L3$\gamma$ & \cite{K00,Cruz09_lowg} \\
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05012406$-$0010452 & 14.982$\pm$0.038 & 2.019$\pm$0.052 & L4$\gamma$ & \cite{Reid08,Cruz09_lowg} \\
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\enddata
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%\tablecomments{}
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\tablenotetext{a}{Proposed replacement for Kelu-1 originally proposed as L2 NIR standard by K10.}
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\tablenotetext{b}{Proposed secondary L5 standard.}
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\tablenotetext{c}{Proposed replacement for 2M~0103+1935 originally proposed as L6 NIR standard by K10.}
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\tablenotetext{d}{Also proposed as a low-gravity NIR spectral standard by \citet{Allers:2013hk}.}
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\end{deluxetable}

tab_lowg_template.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{llllllll}
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\floattable
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\rotate
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\tabletypesize{\tiny}
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\tablewidth{0pt}
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\tablecolumns{8}
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\tablecaption{Low-Gravity L Dwarfs Included in the Low-Gravity Template Sample\label{tab:lowg_template}}
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\tablehead{ \colhead{} & \colhead{} & \multicolumn{2}{c}{2MASS} \\
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\cline{3-4} \\
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\colhead{2MASS} & \colhead{Other} & \colhead{} & \colhead{} & \colhead{Optical} & \colhead{Sp. Type} & \colhead{SpeX Prism} & \colhead{Other} \\
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\colhead{Designation} & \colhead{Name} & \colhead{$J$} & \colhead{$J-K_S$} & \colhead{Sp. Type} &
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\colhead{Ref.} & \colhead{Ref.} & \colhead{Refs.\tablenotemark{a}}
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}
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\startdata
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00325584$-$4405058 & EROS-MP J0032$-$4405 & 14.776$\pm$0.035 & 1.507$\pm$0.05 & L0$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{EROSCollaboration:1999uj} \\
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01415823$-$4633574 & & 14.832$\pm$0.043 & 1.735$\pm$0.054 & L0$\gamma$ & \cite{Cruz09_lowg} & \cite{Kirkpatrick06} & \cite{Kirkpatrick06} \\
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02103857$-$3015313 & & 15.066$\pm$0.048 & 1.566$\pm$0.064 & L0$\gamma$ & This Paper & This Paper & \\
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0241115$-$032658 & & 15.799$\pm$0.065 & 1.764$\pm$0.082 & L0$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{Cruz07} \\
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03231002$-$4631237 & & 15.389$\pm$0.07 & 1.687$\pm$0.086 & L0$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{Reid08} \\
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1711135+232633 & & 14.499$\pm$0.026 & 1.443$\pm$0.037 & L0$\gamma$ & This Paper & This Paper & \cite{Cruz07} \\
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2213449$-$213607 & & 15.376$\pm$0.035 & 1.620$\pm$0.052 & L0$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{Cruz07} \\
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23153135+0617146 & & 15.861$\pm$0.083 & 1.796$\pm$0.105 & L0$\gamma$ & This Paper & This Paper & This Paper \\
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\hline
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03572695$-$4417305 & DENIS J0357$-$4417 & 14.367$\pm$0.032 & 1.46 $\pm$0.042 & L0$\beta$ & \cite{Kirkpatrick08} & This Paper & \cite{Bouy03} \\
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11544223$-$3400390 & DENIS-P J115442.2$-$340039 & 14.195$\pm$0.033 & 1.344$\pm$0.047 & L0$\beta$ & \cite{Kirkpatrick08} & This Paper & \cite{Bouy03} \\
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15525906+2948485 & & 13.478$\pm$0.026 & 1.456$\pm$0.038 & L0$\beta$ & \cite{Reid08} & This Paper & \cite{Wilson03} \\
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\hline
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00452143+1634446 & & 13.059$\pm$0.022 & 1.693$\pm$0.03 & L1.5$\gamma$ & \cite{Reid08} & This Paper & \cite{Wilson03} \\
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0117474-340325 & & 15.178$\pm$0.036 & 1.689$\pm$0.052 & L1$\gamma$ & This Paper & This Paper & \cite{Cruz03} \\
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0518461-275645 & & 15.262$\pm$0.043 & 1.647$\pm$0.059 & L1$\gamma$ & This Paper & This Paper & \cite{Cruz07} \\
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\hline
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02271036-1624479 & SIPS J0227-1624 & 13.573 $\pm$ 0.023 & 1.43 $\pm$ 0.038 & L1$\beta$ & \cite{Reid08} & This Paper & \cite{Deacon05} \\
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10224821+5825453 & & 13.499$\pm$0.026 & 1.339$\pm$0.036 & L1$\beta$ & \cite{Cruz09_lowg} & This Paper & \cite{Reid08} \\
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\hline
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00550564+0134365 & & 16.436$\pm$0.114 & 1.998$\pm$0.133 & L2$\gamma$ & This Paper & This Paper & \\
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0536199-192039 & & 15.768$\pm$0.074 & 1.914$\pm$0.097 & L2$\gamma$ & This Paper & This Paper & \cite{Cruz07} \\
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\hline
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%1004207+502300 G 196-3B & 14.831$\pm$0.047 & 2.053$\pm$0.058 & L3$\beta$ & Cruz09 & This Paper & \\
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15515237+0941148 & & 16.319$\pm$0.111 & 2.009$\pm$0.125 & L3.5$\gamma$ & This Paper & This Paper & \cite{Reid08} \\
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1726000+153819 & & 15.669$\pm$0.065 & 2.01 $\pm$0.082 & L3.5$\gamma$ & This Paper & This Paper & \cite{K00} \\
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22081363+2921215 & & 15.797$\pm$0.085 & 1.649$\pm$0.112 & L3$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{K00} \\
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\hline
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05012406-0010452 & & 14.982$\pm$0.038 & 2.019$\pm$0.052 & L4$\gamma$ & \cite{Cruz09_lowg} & This Paper & \cite{Reid08} \\
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15382417-1953116 & & 15.934$\pm$0.064 & 1.93 $\pm$0.081 & L4$\gamma$ & This Paper & This Paper & \\
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1615425+495321 & & 16.789$\pm$0.138 & 2.483$\pm$0.155 & L4$\gamma$ & This Paper & This Paper & \cite{Cruz07} \\
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2206449-421720 & & 15.555$\pm$0.066 & 1.946$\pm$0.086 & L4$\gamma$ & \cite{K00} & This Paper & \cite{K00} \\
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SDSS 2249+0044 & & 16.587$\pm$0.125 & 2.229$\pm$0.143 & L4$\gamma$ & This Paper & \cite{Allers:2010cg} & \cite{Geballe02,Kirkpatrick08} \\
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\enddata
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\tablecomments{Templates generated using spectra of these objects are shown in Figures~\ref{fig:beta_templates} and \ref{fig:gamma_templates}.}
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\tablenotetext{a}{References listed pertain to discovery and spectral data and are not exhaustive.}
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\end{deluxetable}

tab_newnir.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{ll}
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%\tabletypesize{\scriptsize}
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%\tabletypesize{\tiny}
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\tablecolumns{2}
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\tablecaption{New Near-Infrared IRTF SpeX Prism Observations\label{tab:newnir}}
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\tablehead{
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\colhead{2MASS} & \colhead{Obs Date (UT)} \\
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\colhead{Designation} & \colhead{yyyy/mm/dd}
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}
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\startdata
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00100009$-$2031122 & 2008/07/14 \\
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00250365+4759191 & 2003/09/03 \\
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00325584$-$4405058 & 2007/11/13 \\
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00325584$-$4405058 & 2008/09/07 \\
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00332386$-$1521309 & 2003/09/04 \\
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\enddata
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\tablecomments{Data are publicly available from the SpeX Library. This table is published in its entirety in a machine readable format in the electronic edition of the journal. A portion is shown here for guidance regarding its form and content.}
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\end{deluxetable}

tab_newnir.txt

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Title: Meeting the Cool Neighbors XII: An Optically-Anchored Analysis of the Near-Infrared Spectra of L Dwarfs.
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Authors: Cruz et al.
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Table: New Near-Infrared IRTF SpeX Prism Observations
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================================================================================
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Byte-by-byte Description of file: tab_newnir.txt
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--------------------------------------------------------------------------------
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Bytes Format Units Label Explanations
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--------------------------------------------------------------------------------
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1- 16 A16 -- Name 2MASS Designation
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18- 27 A10 -- Date Observation date (YYYY/MM/DD)
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--------------------------------------------------------------------------------
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0010001-203112 2008/07/14
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0025036+475919 2003/09/03
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00325584-4405058 2007/11/13
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00325584-4405058 2008/09/07
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00361617+1821104 2003/08/12
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00452143+1634446 2007/09/16
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00550564+0134365 2003/09/04
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0103320+193536 2003/09/19
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0117474-340325 2006/08/21
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0141032+180450 2003/08/12
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0141032+180450 2008/09/07
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0144353-071614 2004/11/07
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0144353-071614 2004/11/08
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0144353-071614 2005/08/10
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0205034+125142 2006/08/20
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0205293-115930 2003/08/11
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02103857-3015313 2003/09/04
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0213288+444445 2004/11/08
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02271036-1624479 2011/12/08
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0230155+270406 2008/09/07
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0241115-032658 2006/08/21
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02572581-3105523 2003/09/05
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0310140-275645 2011/12/08
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03140344+1603056 2011/12/07
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0318540-342129 2003/09/03
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03231002-4631237 2007/11/13
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0325013+225303 2003/09/03
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0325013+225303 2011/12/08
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0337036-175807 2011/12/08
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03454316+2540233 2003/09/05
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03483060+2244500 2006/12/09
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03483060+2244500 2007/11/14
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03572695-4417305 2007/09/16
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03582255-4116060 2007/11/14
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03582255-4116060 2011/12/08
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0408290-145033 2011/12/07
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0439010-235308 2004/11/08
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0445538-304820 2004/11/08
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05012406-0010452 2007/10/12
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0518461-275645 2011/12/08
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0523382-140302 2004/11/07
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0536199-192039 2003/09/03
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05431887+6422528 2011/12/08
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06022216+6336391 2011/12/08
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06160532-4557080 2011/12/08
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06244595-4521548 2005/03/24
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06521977-2534505 2006/09/02
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06521977-2534505 2009/01/25
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06521977-2534505 2009/11/04
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0652307+471034 2004/11/07
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0700366+315726 2004/11/07
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07231462+5727081 2011/12/07
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0746425+200032 2007/11/14
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0820299+450031 2007/11/14
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08230838+6125208 2011/12/07
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0825196+211552 2005/03/23
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08300825+4828482 2004/11/08
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0835425-081923 2004/11/08
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08355829+0548308 2011/12/07
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0847287-153237 2004/11/08
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0850359+105715 2005/03/24
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0908380+503208 2004/11/08
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09153413+0422045 2005/03/24
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09153413+0422045 2005/03/24
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09211410-2104446 2004/11/08
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0928397-160312 2011/12/07
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1010148-040649 2005/03/24
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10224821+5825453 2005/03/23
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1043075+222523 2004/11/07
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1045240-014957 2005/03/24
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10484281+0111580 2005/03/24
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1058478-154817 2005/03/24
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11000965+4957470 2004/11/08
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11544223-3400390 2008/01/09
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12070374-3151298 2005/03/24
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1231214+495923 2011/12/08
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1300425+191235 2005/03/24
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1300425+191235 2006/04/10
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1343167+394508 2011/12/08
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1404449+463429 2008/07/13
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14213145+1827407 2008/07/30
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14283132+5923354 2003/09/05
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1430435+291540 2008/07/13
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1506544+132106 2005/03/23
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1507476-162738 2003/08/12
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1515009+484739 2003/09/05
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15382417-1953116 2003/09/04
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15515237+0941148 2003/09/05
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15515237+0941148 2006/08/21
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15515237+0941148 2008/07/13
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15525906+2948485 2008/07/30
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1615425+495321 2005/03/23
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16322911+1904407 2003/09/05
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1645220+300407 2003/08/11
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1645220+300407 2008/07/13
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16585033+1819597 2010/07/07
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1707333+430130 2008/09/08
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1711135+232633 2008/07/13
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17224432+6329470 2009/06/30
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1726000+153819 2003/08/11
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1726000+153819 2008/07/13
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1728114+394859 2006/08/21
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17312974+2721233 2005/03/24
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17461199+5034036 2003/09/04
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1807159+501531 2003/08/12
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19223062+6610194 2003/09/03
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20343769+0827009 2007/11/13
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2041428-350644 2008/08/09
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2057540-025230 2003/09/05
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2104149-103736 2003/09/05
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21373742+0808463 2007/11/14
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2151254-244100 2003/08/12
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2151254-244100 2006/08/21
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21522609+0937575 2004/11/08
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21522609+0937575 2004/11/08
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2206449-421720 2006/08/21
128+
2206449-421720 2008/07/14
129+
22081363+2921215 2007/11/14
130+
22120703+3430351 2003/09/04
131+
2213449-213607 2005/10/17
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2213449-213607 2008/08/29
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2224438-015852 2003/09/05
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2238074+435317 2011/12/07
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2249091+320549 2003/08/12
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22521073-1730134 2005/08/10
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%2254519-284025 2008/07/14
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2310185-175909 2008/07/14
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23153135+0617146 2003/09/04
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23153135+0617146 2007/11/14
141+
2325453+425148 2003/08/12
142+
2330225-034718 2008/07/14
143+
23392527+3507165 2003/09/04

tab_newopt.tex

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%!TEX root = /Users/kelle/Dropbox/Pubs IN PROGRESS/Paper XII NIR DATA/Cruz-Nunez/NIRLdwarfs.tex
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\begin{deluxetable}{lccllll}
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\tabletypesize{\scriptsize}
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%\tabletypesize{\tiny}
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%\rotate
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\tablewidth{0pt}
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\tablecolumns{7}
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\tablecaption{New Far-Red Optical Observations\label{tab:newopt}}
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\tablehead{
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\colhead{} & \colhead{} & \colhead{} & \colhead{Obs Date} & \colhead{Optical} & \colhead{Sp. Type} & \colhead{Discovery and Previous} \\
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\colhead{Object} & \colhead{Telescope} & \colhead{Instrument} & \colhead{(UT)} & \colhead{Sp. Type} & \colhead{Ref.} & \colhead{Sp. Type Refs.}
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}
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\startdata
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00325584$-$4405058 & Keck I & LRIS & 2009 Oct 11 & L0$\gamma$ & \cite{Cruz09_lowg} & (L0) in \cite{Reid08} \\
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00550564+0134365 & Keck I & LRIS & 2009 Oct 11 & L2$\gamma$ & This paper & \\
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0117474$-$340325 & Keck I & LRIS & 2009 Oct 12 & L1$\gamma$ & This paper & L2? in \cite{Cruz03} \\
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02103857$-$3015313 & Keck I & LRIS & 2009 Oct 11 & L0$\gamma$ & This paper & \\
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0241115$-$032658 & Keck I & LRIS & 2009 Oct 12 & L0$\gamma$ & \cite{Cruz09_lowg} & (L1) in \cite{Cruz07} \\
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0518461$-$275645 & Keck I & LRIS & 2009 Feb 17 & L1$\gamma$ & This paper & L0: in \cite{Cruz07} \\
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0536199$-$192039 & Keck I & LRIS & 2009 Feb 17 & L2$\gamma$ & This paper & L1: in \cite{Cruz07} \\
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13313310+3407583 & Keck I & LRIS & 2009 Feb 17 & L0 & \cite{Reid08} & \cite{Reid08} \\
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15382417$-$1953116 & Keck I & LRIS & 2010 Jul 17 & L4$\gamma$ & This paper & \\
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15515237+0941148 & Keck I & LRIS & 2010 Jun 18 & L3.5$\gamma$ & This paper & (L2) in \cite{Reid08} \\
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\nodata & Keck I & LRIS & 2009 Feb 17 & & & \\
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1615425+495321 & Keck I & LRIS & 2010 Jun 18 & L4$\gamma$ & This paper & (L4) in \cite{Cruz07} \\
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\nodata & Keck I & LRIS & 2009 Feb 17 & & & \\
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1711135+232633 & Keck I & LRIS & 2010 Jun 18 & L0$\gamma$ & This paper & L0: in \cite{Cruz07} \\
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1726000+153819 & Keck I & LRIS & 2010 Jun 18 & L3.5$\gamma$ & \cite{Cruz09_lowg} & L2 in \cite{K00} \\
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20343769+0827009 & Clay & LDSS-3 & 2008 Oct 07 & L1 & This paper & \\
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21373742+0808463 & Keck I & LRIS & 2010 Jul 17 & L5 & This paper & \cite{Reid08} \\
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22495345+0044046AB & Keck I & LRIS & 2009 Oct 11 & L4$\gamma$ & This Paper & \cite{Geballe02,Allers:2010cg} \\
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\nodata & \nodata & \nodata & \nodata & \nodata & \nodata & L3 in \cite{Hawley02} \\
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23153135+0617146 & Keck I & LRIS & 2009 Oct 11 & L0$\gamma$ & This paper & \\
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\enddata
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\tablecomments{Spectra shown in Figure Set~\ref{fig:newopt} and publicly available from the RIZzo Spectral Library.}
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%\tablenotetext{a}{References listed pertain to discovery and previous \emph{optical} classifications.}
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\end{deluxetable}

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