\documentstyle[aaspp]{article} %\documentstyle{article}\def\nodata{---}\def\tableline{\hline} \begin{document} \begin{tabular}{lllllll} \hline \multicolumn{1}{c}{HR \#} & \multicolumn{1}{c}{NAME $^a$} & \multicolumn{1}{c}{$m_H^b$} & \multicolumn{1}{c}{ST} & \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{RV (km s$^{-1}$) $^c$} & \multicolumn{1}{c}{vsini (km s$^{-1}$) } \\\hline\hline % 1903 & *46 $\epsilon$ Ori & 2.4 & B0 & Ia & 26SB & 87 \\ 1203 & 44 $\zeta$ Per & 3.4 & B1 & Ib & 20SB & 59 \\ 2827 & 31 $\eta$ CMa & 2.5 & B5 & Ia & 41V & 45 \\ 1713 & *19 $\beta$ Ori & 0.1 & B8 & Ia & 21SB & 33 \\ 3975 & *30 $\eta$ Leo & 3.3 & A0 & Ib & 3V & 20 \\ 7924 & *50 $\alpha$ Cyg & 1.0 & A2 & Ia & -5SBO & 21 \\ 1865 & 11 $\alpha$ Lep & 2.0 & F0 & Ib & 24 & 13 \\ 1017 & *33 $\alpha$ Per & 0.9 & F5 & Ib & -2V & 18 \\ 7796 & *37 $\gamma$ Cyg & 1.1 & F8 & Ib & -8V & 20 \\ 8232 & *22 $\beta$ Aqr & 1.5 & G0 & Ib & 7V? & 18 \\ 7479 & 5 $\alpha$ Sge & 2.4 & G1 & II & 2V? & 0 \\ 7063 & $\beta$ Sct & 2.2 & G4 & IIa & -22SB10 & 10 \\ 8752 & *- & 3.6 & G4v & $>I^d$ & -58V? & 35 \\ 7314 & *21 $\theta$ Lyr & 2.1 & K0 & +II & -31V & $<$19 \\ 6713 & 93 Her & 2.4 & K0.5 & IIb & -24 & $<$17 \\ 8465 & *21 $\zeta$ Cep & 1.1 & K1.5 & Ib & -18SB & $<$17 \\ 6498 & 49 $\sigma$ Oph & 1.9 & K2 & II & -27 & $<$19 \\ 603 & 57 $\gamma^1$ And & -0.5 & K3 & -IIb & -12SB & $<$17 \\ 8089 & *63 Cyg & 1.5 & K4 & Ib-IIa & -26V & -- \\ 8079 & *62 $\xi$ Cyg & 0.5 & K4.5 & Ib-II & -20SB & $<$17 \\ 2061 & 58 $\alpha$ Ori & -2.? & M1-2 & Ia-Iab & 21SB & -- \\ 1155 & *-- & 0.5 & M2 & +IIab & -3V & -- \\ 921 & 25 $\rho$ Per & -1.7 & M4 & II & 28 & -- \\ 7009 & *-- & 0.6 & M4.5-M5 & +II & -19 & -- \\ 6406 & *64 $\alpha^1$ Her & -2.4 & M5 & Ib-II & -33V & 21 \\\hline % \multicolumn{7}{l}{\footnotesize $^a$ ``*'' indicates that the object also appears in the K--band atlas of WH97.} \\ \multicolumn{7}{l}{\footnotesize $^b$ H--band magnitudes estimated from V--band magnitude from the Bright Star} \\ \multicolumn{7}{l}{\footnotesize Catalogue, spectral type, and intrinsic colors (Koornneef, 1983).} \\ \multicolumn{7}{l}{\footnotesize $^c$ ``V'' and ``V?'' indicate variable or suspected variable radial velocity respectively.} \\ \multicolumn{7}{l}{\footnotesize ``SB1'' and ``SB2'' indicate single-- and double--lined spectroscopic binaries respectively.} \\ \multicolumn{7}{l}{\footnotesize ``O'' indicates that orbital data is available in the Bright Star Catalogue.}\\ \multicolumn{7}{l}{\footnotesize $^d$ Previously classified as G0Ia, but it is intrinsically brighter. } \\ \multicolumn{7}{l}{\footnotesize $^e$ Taken from Jaschek, Jaschek, and Condi (1964).} \\ \multicolumn{7}{l}{\footnotesize $^f$ Taken from Henry, Kirkpatrick, and Simons (1994).} \\ \end{tabular} \clearpage %\end{document} %\end %\documentstyle[12pt,aaspp]{article} %\begin{document} \begin{tabular}{lllllll} \hline \multicolumn{1}{c}{HR \#} & \multicolumn{1}{c}{NAME $^a$} & \multicolumn{1}{c}{$m_H ^b$} & \multicolumn{1}{c}{ST} & \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{RV (km s$^{-1}$) $^c$} & \multicolumn{1}{c}{vsini (km s$^{-1}$) } \\\hline\hline % 1899 & 44 $\iota$ Ori & 3.5 & O9 & III & 22SB2O & 130 \\ 1552 & 3 $\pi^4$ Ori & 4.1 & B2+B2 & III & 23SBO & 40 \\ 5291 & *11 $\alpha$ Dra & 3.5 & A0 & III & -13SBO & 18 \\ 403 & *37 $\delta$ Cas & 2.3 & A5 & III-IV & 7SB & 113 \\ 1412 & *78 $\theta^2$ Tau & 2.9 & A7 & III & 40SB1O & 78 \\ 4031 & *36 $\zeta$ Leo & 2.8 & F0 & III & -16SB & 84 \\ 21 & * 11 $\beta$ Cas & 1.6 & F2 & III--IV & 12SB & 70 \\ 5017 & *20 CVn & 3.9 & F3 & III & 8V? & 17 \\ 2706 & 48 Gem & 5.0 & F5 & III-IV & 13V & 74 \\ 8905 & *68 $\upsilon$ Peg & 3.3 & F8 & III & -11 & 79 \\ 4883 & *31 Com & 3.0 & G0 & III & -1V? & 77 \\ 4716 & 5 CVn & 2.8 & G6 & III & -12SB & $<$17 \\ 7328 & 1 $\kappa$ Cyg & 1.6 & G9 & III & -29SB & $<$17 \\ 7949 & 53 $\epsilon$ Cyg & 0.2 & K0 & -III & -11SB? & $<$17 \\ 8317 & *11 Cep & 2.3 & K1 & III & -37 & $<$17 \\ 6299 & *27 $\kappa$ Oph & 0.8 & K2 & III & -56V & $<$17 \\ 165 & 31 $\delta$ And & 0.5 & K3 & III & -7SB1O & $<$17 \\ 6705 & *33 $\gamma$ Dra & -1.2 & K5 & III & -28 & $<$17 \\ 152 & -- & 1.7 & K5-M0 & III & -33V & $<$17 \\ 4517 & *3 $\nu$ Vir & 0.3 & M1 & IIIab & 51V? & -- \\ 6242 & -- & 0.4 & M4 & +III-IIIa & -7V? & -- \\ 7886 & *-- & -0.6 & M6 & III & -66V? & -- \\\hline \end{tabular} \clearpage %\end{document} %\end %\documentstyle[12pt,aaspp]{article} %\begin{document} \begin{tabular}{lllllll} \hline \multicolumn{1}{c}{HR \#} & \multicolumn{1}{c}{NAME $^a$} & \multicolumn{1}{c}{$m_H ^b$} & \multicolumn{1}{c}{ST} & \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{RV (km s$^{1}$) $^c$} & \multicolumn{1}{c}{vsini (km s$^{1}$) } \\\hline\hline % 6588 & 85 $\iota$ Her & 4.3 & B3 & IV & -20SB1O & 11 \\ 4033 & *33 $\lambda$ UMa & 3.3 & A2 & IV & 18V & 48 \\ 1351 & 57 Tau & 4.9 & F0 & IV & 42SB1? & 109 \\ 5235 & 8 $\eta$ Boo & 1.5 & G0 & IV & 0SB1O & 13 \\ 5409 & 105 $\phi$ Vir & 2.8 & G2 & IV & -10SB & 0 \\ 6623 & 86 $\mu$ Her & 1.4 & G5 & IV & -16V & 20 \\ 995 & 59 Ari & 3.9 & G6 & IV & 0V & -- \\ 7602 & 60 $\beta$ Aql & 1.7 & G8 & IV & -40V & $<$ 16 \\ 7957 & *3 $\eta$ Cep & 1.2 & K0 & IV & -87 & $<$17 \\ 5901 & 11 $\kappa$ CrB & 2.5 & K1 & IVa & -24 & $<$17 \\ 6014 & -- & 3.6 & K1.5 & IV & -4V & -- \\\hline 2456 & *15 Mon & 5.5 & O7 & V(e) & 33SB & 63 \\ 5191 & *85 $\eta$ UMa$^e$ & 2.4 & B3 & V & -11SB? & 205 \\ 3982 & *32 $\alpha$ Leo$^e$ & 1.6 & B7 & V & 6SB & 329 \\ 7001 & * $\alpha$ Lyr & 0.0 & A0 & V & -14V & 15 \\ 2491 & *9 $\alpha$ CMa & -1.5 & A1 & Vm & -8SBO & 13 \\ 4534 & *94 $\beta$ Leo$^e$ & 2.0 & A3 & V & 0V & 121 \\ 4357 & *68 $\delta$ Leo$^e$ & 2.3 & A4 & V & -20V & 181 \\ 4931 & 78 UMa & 4.1 & F2 & V & -10V? & 92 \\ 1279 & -- & 5.1 & F3 & V & 36SB1? & 25 \\ 2943 & *10 $\alpha$ CMi & -0.6 & F5 & IV-V & -3SBO & 6 \\ 1538 & 59 Eri$^e$ & 2.3 & F6 & V & 35 & -- \\ 4375 & *53 $\xi$ UMa & 3.0 & G0 & V & -16SB1O & 1 \\ 4983 & 43 $\beta$ Com & 3.1 & F9.5 & V & 6SB? & 6 \\ 483 & *-- & 3.7 & G1.5 & V & 4V? & 2 \\ 4374 & 53 $\xi$ UMa & 3.5 & G0 & V & -16SB1O & 3 \\ 5072 & 70 Vir & 3.6 & G4 & V & 5V & 1 \\ 4496 & *61 UMa & 3.8 & G8 & V & -5V & $<$17 \\ 7462 & *61 $\sigma$ Dra & 3.0 & K0 & V & 27V & $<$17 \\ 1084 & *18 $\epsilon$ Eri & 1.6 & K2 & V & 15V? & $<$17 \\ 8832 & *-- & 3.2 & K3 & V & -18V & -- \\ -- & GL570A & 3.0 & K4 & V & - & - \\ 8085 & *61 Cyg & 2.4 & K5 & V & -64V & $<$17 \\ 8086 & 61 Cyg & 3.1 & K7 & V & -64V? & =$<$25 \\ -- & GL338A & 4.5 & M0 & V & - & - \\ -- & GL526$^f$ & 4.5 & M1.5 & V & - & - \\ -- & *GL411 & 3.6 & M2 & V & - & - \\ -- & *GL725A & 4.7 & M3 & V & - & - \\\hline \end{tabular} \clearpage %\end{document} %\end %\documentstyle[12pt,aaspp]{article} %\begin{document} \begin{tabular}{lllllll} \hline \multicolumn{1}{c}{HR \#} & \multicolumn{1}{c}{NAME} & \multicolumn{1}{c}{Vmag$^1$} & \multicolumn{1}{c}{ST} & \multicolumn{1}{c}{Class} & \multicolumn{1}{c}{RADV$^2$} & \multicolumn{1}{c}{ROTV$^2$} \\\hline\hline % 2456 & 15 Mon & 4.66 & O7 & V((f)) & 33SB & 63 \\ 5191 & 85 $\eta$ UMa & 1.86 & B3 & V & -11SB? & 205 \\ 3982 & 32 $\alpha$ Leo & 1.35 & B7 & V & 6SB & 329 \\ 2491 & 9 $\alpha$ CMa & -1.4 & A1 & Vm & -8SBO & 13 \\ 4534 & 94 $\beta$ Leo & 2.14 & A3 & V & 0V & 121 \\ 4357 & 68 $\delta$ Leo & 2.56 & A4 & V & -20V & 181 \\ 4931 & 78 UMa & 4.93 & F2 & V & -10V? & 92 \\ 1279 & -- & 6.01 & F3 & V & 36SB1? & 25 \\ 2943 & 10 $\alpha$ CMi & 0.38 & F5 & IV-V & -3SBO & 6 \\ 1538 & 59 Eri & 5.77 & F6 & V & 35 & -- \\ 4375 & 53 $\xi$ UMa & 4.41 & G0 & V & -16SB1O & 1 \\ 4983 & 43 $\beta$ Com & 4.26 & F9.5 & V & 6SB? & 6 \\ 483 & -- & 4.95 & G1.5 & V & 4V? & 2 \\ 4374 & 53 $\xi$ UMa & 4.87 & G0 & V & -16SB1O & 3 \\ 5072 & 70 Vir & 4.98 & G4 & V & 5V & 1 \\ 4496 & 61 UMa & 5.33 & G8 & V & -5V & $<$17 \\ 7462 & 61 $\sigma$ Dra & 4.68 & K0 & V & 27V & $<$17 \\ 1084 & 18 $\epsilon$ Eri & 3.73 & K2 & V & 15V? & $<$17 \\ 8832 & -- & 5.56 & K3 & V & -18V & -- \\ GL570A & - & - & - & - & - & - \\ 8085 & 61 Cyg & 5.21 & K5 & V & -64V & $<$17 \\ 8086 & 61 Cyg & 6.03 & K7 & V & -64V? & =$<$25 \\ GL338A & - & - & - & - & - & - \\ GL411 & - & - & - & - & - & - \\ GL526 & - & - & - & - & - & - \\ GL725A & - & - & - & - & - & - \\\hline \end{tabular} \clearpage %\end{document} %\end \begin{tabular}{rlll} \hline \multicolumn{1}{c}{Spectral Type $^a$} & \multicolumn{1}{c}{T$_{I-II}^b$} & \multicolumn{1}{c}{T$_{III}^{b,c}$} & \multicolumn{1}{c}{T$_{IV-V}^b$} \\\hline % O6-O8-- & \nodata & 37000 & 38000 \\ O9-- & 32500 & 32000 & 33200 \\ O9.5-- & \nodata & \nodata & 31450 \\ B0-- & 26000 & 29000 & 29700 \\ B1-- & 20700 & 24000 & 25600 \\ B2-- & 17800 & 20300 & 22300 \\ B3-- & 15600 & 17100 & 19000 \\ B4 & 13900 & \nodata & 17200 \\ B5-- & 13400 & 15000 & 15400 \\ B6 & 12700 & 14100 & 14100 \\ B7-- & 12000 & 13200 & 13000 \\ B8-- & 11200 & 12400 & 11800 \\ B9-- & 10500 & 11000 & 10700 \\ A0-- & 9730 & 10100 & 9480 \\ A1-- & 9230 & 9480 & \nodata \\ A2 & 9080 & 9000 & 8810 \\ A5-- & 8510 & 8100 & 8160 \\ A7-- & \nodata & 7650 & 7930 \\ F0-- & 7700 & 7150 & 7020 \\ F2-- & 7170 & 6870 & 6750 \\ F5-- & 6640 & 6470 & 6530 \\ F7-- & \nodata & \nodata & 6240 \\ F8-- & 6100 & 6150 & \nodata \\\hline % \multicolumn{4}{l}{\footnotesize $^a$ ``--'' denotes full sub--class in the revised MK system. Other full} \\ \multicolumn{4}{l}{\footnotesize sub--classes for which temperatures are not available without interpolation} \\ \multicolumn{4}{l}{\footnotesize include B0.5, A3, A8, F3, F9, and G5.} \\ \multicolumn{4}{l}{\footnotesize $^b$ Data taken from Tokunaga, 1996, Astrophysical Quantities, in press.}\\ \multicolumn{4}{l}{\footnotesize $^c$ For giant stars G0 and later data taken from Schmidt--Kaler (1982).} \\ \multicolumn{4}{l}{\footnotesize $^d$ Temperature for star of Luminosity Class Iab.} \\ \end{tabular} \clearpage \begin{tabular}{rlll} \hline \multicolumn{1}{c}{Spectral Type $^a$} & \multicolumn{1}{c}{T$_{I-II}^b$} & \multicolumn{1}{c}{T$_{III}^{b,c}$} & \multicolumn{1}{c}{T$_{IV-V}^b$} \\\hline % G0-- & 5510 & 5910 & 5930 \\ G2 & \nodata & \nodata & 5830 \\ G3 & 4980 & \nodata & \nodata \\ G4 & \nodata & 5190 & 5740 \\ G6 & \nodata & 5050 & 5620 \\ G8-- & 4590 & 4960 & \nodata \\ K0-- & 4420 & 4810 & 5240 \\ K1-- & 4330 & 4610 & \nodata \\ K2-- & 4260 & 4500 & 5010 \\ K3-- & 4130$^d$& 4320 & \nodata \\ K4-- & \nodata & 4080 & 4560 \\ K5-- & 3850$^d$& 3980 & 4340 \\ K7 & \nodata & \nodata & 4040 \\ M0-- & 3650$^d$& 3820 & 3800 \\ M1-- & 3550$^d$& 3780 & 3680 \\ M2-- & 3450$^d$& 3710 & 3530 \\ M3-- & 3200$^d$& 3630 & 3380 \\ M4-- & 2980$^d$& 3560 & 3180 \\ M5-- & \nodata & 3420 & 3030 \\ M6-- & \nodata & 3250 & 2850 \\\hline % \end{tabular} \clearpage \begin{tabular}{lll} \hline \multicolumn{1}{c}{Date} & \multicolumn{1}{c}{Type} & \multicolumn{1}{c}{ \# of Stars} \\\hline\hline % March 9--10, 1993 & Day & 17 \\ April 1--3, 1993 & Day/Night & 30 \\ May 18--19, 1993 & Day & 10 \\ January 30--31, 1994 & Day/Night & 42 \\\hline % \end{tabular} \clearpage \begin{table} \caption{H--Band Spectral Indices for Classification of A-M Stars} \begin{tabular}{lllllll} \tableline % \multicolumn{1}{c}{Main Feature \tablenotemark{a}}& \multicolumn{1}{c}{E$_{low}$ (ev) } & \multicolumn{1}{c}{$\sigma$ (cm$^{-1}$) \tablenotemark{a}}& \multicolumn{1}{c}{$\lambda$ ($\mu$m) } & \multicolumn{1}{c}{$\sigma_{cent}$ (cm$^{-1}$)}& \multicolumn{1}{c}{$\Delta \sigma$ (cm$^{-1}$)} & \multicolumn{1}{c}{Other contr. \tablenotemark{a}} \\\tableline\tableline % MgI(4s--4p) & 5.39 \tablenotemark{b}& 5843.41 & 1.71133 & 5844 & 10 & CO, Fe, Ni, OH \\ OH($\Delta v = 2$) & 0.76 \tablenotemark{c}& 5920: & 1.689 & 5920 & 20 & C, CO, Fe, Ni \\ HI(4-11) & 12.75 \tablenotemark{d}& 5948.50 & 1.68110 & 5950 & 20 & CO, Fe, Ni, Si \\ AlI(4p--4d tr) & 4.09 \tablenotemark{e}& 5963.76 & 1.67679 & 5972.5 & 25 & CO, Fe, Ni, OH \\ & & 5968.31 & 1.67552 & & & \\ & & 5979.60 & 1.67235 & & & \\ SiI(4p--3d) & 5.98 \tablenotemark{f}& 5993.29 & 1.66853 & 5993 & 10 & CO, Fe, Ni, OH \\ $^{12}$CO(8,5)bh & 1.55 \tablenotemark{g}& 6018 & 1.662 & 6017.5 & 15 & Fe, OH, S \\ $^{12}$CO(6,3)bh & 1.05 \tablenotemark{g} & 6177 & 1.619 & 6170 & 50 & Ca, Fe, Ni, OH, Si \\ SiI(4p--5s) & 5.98 \tablenotemark{f}& 6263.92 & 1.59644 & 6264 & 10 & Fe, Mg, Ni, OH \\ MgI(4s--4p tr) & 5.93 \tablenotemark{b}& 6341.10 & 1.57701 & 6345 & 20 & CN, CO, Fe, H$_2$O, Ni, OH \\ & & 6347.88 & 1.57533 & & & \\ & & 6351.22 & 1.57450 & & & \\\tableline \end{tabular} \tablenotetext{a}{Species indentification and frequencies from LW91 and WL92.} \tablenotetext{b}{Lower state energy level from Risberg (1965).} \tablenotetext{c}{Coxon and Forester (1982).} \tablenotetext{d}{Garcia and Mack (1965).} \tablenotetext{e}{Eriksson and Isberg (1963).} \tablenotetext{f}{Litzen (1964).} \tablenotetext{g}{George, Urban, \& LeFloch (1994).} \label{ftshband} \end{table} %\end{small} \clearpage \footnotesize \begin{tabular}{llllllllllll} \hline % \multicolumn{1}{c}{Source} & \multicolumn{1}{c}{T$_{e}$ } & \multicolumn{1}{c}{SNR} & \multicolumn{1}{c}{Mg5844} & \multicolumn{1}{c}{OH5920} & \multicolumn{1}{c}{HI5950} & \multicolumn{1}{c}{Al5973} & \multicolumn{1}{c}{Si5993} & \multicolumn{1}{c}{CO6018} & \multicolumn{1}{c}{CO6170} & \multicolumn{1}{c}{Si6264} & \multicolumn{1}{c}{Mg6345} \\\hline\hline % HR1903 & 26000 & 203 & -0.03 & 0.09 & 0.75 & 0.17 & -0.02 & 0.11 & 0.27 & 0.11 & 0.47 \\ HR1903 & 26000 & 167 & 0.01 & 0.07 & 0.73 & 0.11 & -0.00 & 0.09 & 0.19 & 0.12 & 0.32 \\ HR1203 & 20700 & 160 & -0.01 & 0.12 & 0.80 & 0.18 & 0.01 & 0.11 & 0.23 & 0.11 & 0.56 \\ HR2827 & 13400 & 045 & -0.05 & -0.02 & 1.06 & -0.04 & 0.20 & -0.04 & 0.01 & -0.05 & 0.08 \\ HR1713 & 11200 & 218 & 0.04 & 0.06 & 1.27 & 0.23 & 0.05 & 0.09 & 0.19 & 0.17 & 0.50 \\ HR3975 & 9730 & 068 & -0.08 & 0.11 & 2.12 & 0.23 & 0.12 & -0.09 & 0.33 & 0.20 & 0.58 \\ HR7924 & 9080 & 225 & -0.05 & 0.00 & 1.40 & 0.20 & -0.02 & 0.03 & -0.14 & 0.08 & 0.08 \\ HR1865 & 7700 & 196 & -0.01 & 0.22 & 2.21 & 0.32 & 0.14 & -0.13 & 0.30 & 0.25 & 0.52 \\ HR1017 & 6640 & 248 & 0.08 & 0.25 & 1.88 & 0.43 & 0.06 & -0.02 & 0.53 & 0.41 & 1.05 \\ HR7796 & 6100 & 324 & 0.10 & 0.29 & 1.58 & 0.69 & 0.14 & 0.03 & 0.79 & 0.60 & 0.94 \\ HR8232 & 5510 & 290 & 0.09 & 0.37 & 1.28 & 0.67 & 0.17 & 0.03 & 1.18 & 0.67 & 1.19 \\ HR8752 & 5510 & 084 & -0.13 & 0.34 & 1.16 & 0.14 & 0.07 & 0.02 & 0.16 & 0.16 & 0.41 \\ HR7479 & 5333 & 096 & 0.15 & 0.13 & 1.13 & 0.70 & 0.10 & 0.00 & 0.92 & 0.41 & 0.69 \\ HR7479 & 5333 & 109 & 0.10 & 0.22 & 1.07 & 0.49 & 0.11 & 0.02 & 0.76 & 0.54 & 1.04 \\ HR7479 & 5333 & 182 & 0.13 & 0.12 & 1.08 & 0.56 & 0.05 & 0.07 & 0.94 & 0.49 & 1.06 \\ HR7479 & 5333 & 093 & 0.06 & -0.02 & 1.20 & 0.53 & 0.03 & 0.14 & 1.05 & 0.54 & 0.93 \\ HR7063 & 4902 & 260 & 0.17 & 0.12 & 0.94 & 0.84 & 0.14 & 0.25 & 1.66 & 0.76 & 1.06 \\ HR7314 & 4420 & 193 & 0.23 & 0.15 & 0.84 & 0.88 & 0.15 & 0.46 & 2.25 & 1.00 & 1.60 \\ HR7314 & 4420 & 257 & 0.15 & 0.17 & 0.67 & 0.59 & 0.10 & 0.37 & 1.91 & 0.86 & 1.36 \\ HR6713 & 4375 & 265 & 0.22 & 0.19 & 0.81 & 0.80 & 0.16 & 0.40 & 1.86 & 0.79 & 1.25 \\ HR8465 & 4295 & 308 & 0.13 & 0.28 & 0.68 & 0.70 & 0.19 & 0.63 & 2.35 & 1.02 & 1.79 \\ HR6498 & 4260 & 247 & 0.24 & 0.30 & 0.84 & 1.00 & 0.21 & 0.83 & 2.75 & 1.11 & 1.84 \\ HR603 & 4130 & 453 & 0.24 & 0.34 & 0.69 & 0.61 & 0.19 & 0.49 & 2.09 & 0.87 & 1.46 \\ HR8089 & 3990 & 202 & 0.21 & 0.45 & 0.50 & 0.67 & 0.14 & 0.68 & 2.26 & 0.94 & 1.59 \\ HR8079 & 3920 & 445 & 0.24 & 0.67 & 0.62 & 0.80 & 0.24 & 1.05 & 2.70 & 1.05 & 1.72 \\ HR2061 & 3550 & 327 & 0.54 & 1.08 & 0.36 & 1.39 & 0.23 & 1.46 & 3.92 & 0.89 & 2.22 \\ HR1155 & 3450 & 237 & 0.46 & 1.31 & 0.58 & 1.12 & 0.38 & 1.37 & 3.35 & 1.12 & 2.03 \\ HR921 & 2980 & 225 & 0.77 & 1.41 & 0.29 & 1.27 & 0.37 & 1.10 & 4.08 & 0.67 & 1.52 \\ HR7009 & 2925 & 292 & 0.63 & 1.43 & 0.79 & 1.55 & 0.54 & 1.79 & 4.68 & 1.26 & 2.21 \\ HR6406 & 2800 & 319 & 0.59 & 1.41 & 0.80 & 1.66 & 0.54 & 1.85 & 4.98 & 1.31 & 2.31 \\ \end{tabular} \clearpage \begin{tabular}{llllllllllll} \hline % \multicolumn{1}{c}{Source} & \multicolumn{1}{c}{T$_{e}$ } & \multicolumn{1}{c}{SNR} & \multicolumn{1}{c}{Mg5844} & \multicolumn{1}{c}{OH5920} & \multicolumn{1}{c}{HI5950} & \multicolumn{1}{c}{Al5973} & \multicolumn{1}{c}{Si5993} & \multicolumn{1}{c}{CO6018} & \multicolumn{1}{c}{CO6170} & \multicolumn{1}{c}{Si6264} & \multicolumn{1}{c}{Mg6345} \\\hline\hline % HR1899 & 32000 & 164 & -0.03 & 0.17 & 0.54 & 0.15 & -0.04 & 0.03 & 0.18 & 0.10 & 0.49 \\ HR1899 & 32000 & 182 & -0.04 & 0.20 & 0.62 & 0.11 & 0.05 & -0.03 & 0.07 & -0.00 & 0.07 \\ HR1552 & 20300 & 115 & -0.07 & 0.13 & 1.29 & 0.31 & 0.10 & -0.09 & 0.12 & -0.01 & 0.09 \\ HR5291 & 10100 & 159 & -0.07 & 0.19 & 2.65 & 0.78 & 0.02 & 0.05 & 0.28 & 0.11 & 0.41 \\ HR403 & 8100 & 202 & -0.02 & 0.39 & 2.79 & 0.77 & 0.09 & -0.13 & 0.25 & 0.08 & 0.54 \\ HR1412 & 7650 & 186 & -0.02 & 0.43 & 2.70 & 0.71 & 0.05 & -0.10 & 0.60 & 0.25 & 0.91 \\ HR4031 & 7150 & 193 & 0.02 & 0.29 & 2.30 & 0.54 & 0.12 & -0.09 & 0.25 & 0.13 & 0.48 \\ HR21 & 6870 & 245 & 0.03 & 0.32 & 1.99 & 0.55 & 0.04 & -0.11 & 0.20 & 0.22 & 0.82 \\ HR21 & 6870 & 179 & 0.01 & 0.25 & 2.21 & 0.63 & 0.13 & -0.14 & 0.46 & 0.24 & 0.69 \\ HR5017 & 6700 & 174 & 0.04 & 0.28 & 2.58 & 0.83 & 0.07 & -0.03 & 0.43 & 0.36 & 0.96 \\ HR2706 & 6470 & 086 & 0.01 & 0.39 & 2.08 & 0.47 & 0.16 & -0.10 & 0.13 & 0.20 & 0.64 \\ HR8905 & 6270 & 059 & 0.06 & 0.13 & 1.06 & 0.45 & -0.01 & -0.16 & 0.30 & 0.28 & 1.02 \\ HR4883 & 5910 & 280 & 0.15 & 0.20 & 1.07 & 0.52 & 0.09 & 0.04 & 0.90 & 0.43 & 1.02 \\ HR4716 & 5050 & 133 & 0.17 & 0.10 & 0.97 & 0.47 & 0.13 & 0.07 & 1.29 & 0.54 & 0.92 \\ HR7328 & 4885 & 281 & 0.19 & 0.20 & 0.78 & 0.57 & 0.11 & 0.11 & 1.33 & 0.67 & 1.35 \\ HR7949 & 4810 & 369 & 0.21 & 0.24 & 0.77 & 0.59 & 0.13 & 0.18 & 1.39 & 0.67 & 1.38 \\ HR8317 & 4710 & 191 & 0.29 & 0.14 & 0.63 & 0.58 & 0.08 & 0.26 & 1.79 & 0.83 & 1.64 \\ HR6299 & 4500 & 532 & 0.26 & 0.09 & 0.77 & 0.81 & 0.10 & 0.44 & 1.92 & 0.76 & 1.40 \\ HR165 & 4320 & 266 & 0.34 & 0.24 & 0.64 & 0.58 & 0.18 & 0.41 & 1.98 & 0.89 & 1.45 \\ HR6705 & 3990 & 298 & 0.39 & 0.60 & 0.77 & 1.12 & 0.26 & 0.96 & 3.05 & 1.12 & 1.75 \\ HR6705 & 3990 & 694 & 0.41 & 0.61 & 0.76 & 1.07 & 0.25 & 0.89 & 2.87 & 1.06 & 1.66 \\ HR152 & 3956 & 270 & 0.37 & 0.86 & 0.58 & 0.92 & 0.34 & 0.87 & 2.59 & 0.78 & 1.40 \\ HR4517 & 3780 & 673 & 0.66 & 1.06 & 0.33 & 1.07 & 0.21 & 0.89 & 3.14 & 0.70 & 1.93 \\ HR6242 & 3560 & 458 & 0.52 & 1.12 & 0.57 & 1.18 & 0.39 & 1.45 & 3.93 & 1.16 & 1.96 \\ HR7886 & 3250 & 574 & 0.61 & 1.54 & 0.89 & 1.71 & 0.64 & 2.25 & 5.69 & 1.41 & 2.42 \\ \end{tabular} \clearpage \begin{tabular}{llllllllllll} \hline % \multicolumn{1}{c}{Source} & \multicolumn{1}{c}{T$_{e}$ } & \multicolumn{1}{c}{SNR} & \multicolumn{1}{c}{Mg5844} & \multicolumn{1}{c}{OH5920} & \multicolumn{1}{c}{HI5950} & \multicolumn{1}{c}{Al5973} & \multicolumn{1}{c}{Si5993} & \multicolumn{1}{c}{CO6018} & \multicolumn{1}{c}{CO6170} & \multicolumn{1}{c}{Si6264} & \multicolumn{1}{c}{Mg6345} \\\hline\hline % HR6588 & 19000 & 162 & -0.03 & 0.10 & 1.65 & 0.48 & -0.03 & 0.02 & 0.17 & 0.07 & 0.40 \\ HR4033 & 8810 & 146 & -0.00 & 0.33 & 2.62 & 0.73 & 0.06 & 0.02 & 0.27 & 0.13 & 0.35 \\ HR1351 & 7020 & 094 & -0.06 & 0.40 & 2.18 & 0.62 & 0.19 & -0.19 & -0.01 & 0.10 & 0.24 \\ HR5235 & 5930 & 341 & 0.16 & 0.12 & 1.21 & 0.83 & 0.11 & 0.03 & 1.30 & 0.64 & 1.14 \\ HR5235 & 5930 & 263 & 0.17 & 0.26 & 1.26 & 0.68 & 0.18 & -0.01 & 0.97 & 0.50 & 1.03 \\ HR5409 & 5830 & 158 & 0.16 & 0.16 & 1.02 & 0.51 & 0.12 & -0.03 & 0.91 & 0.44 & 0.95 \\ HR6623 & 5680 & 211 & 0.33 & 0.12 & 0.87 & 0.87 & 0.09 & 0.09 & 1.21 & 0.69 & 1.38 \\ HR995 & 5620 & 143 & 0.22 & 0.08 & 0.80 & 0.61 & 0.23 & 0.03 & 1.09 & 0.48 & 1.14 \\ HR7602 & 5430 & 056 & 0.46 & 0.15 & 0.71 & 0.86 & 0.01 & 0.17 & 1.40 & 0.57 & 1.49 \\ HR7957 & 5240 & 189 & 0.22 & 0.09 & 0.68 & 0.70 & 0.07 & 0.15 & 1.04 & 0.46 & 0.99 \\ HR7957 & 5240 & 192 & 0.09 & 0.18 & 0.56 & 0.52 & -0.01 & 0.09 & 0.75 & 0.40 & 1.17 \\ HR5901 & 5125 & 395 & 0.37 & 0.13 & 0.55 & 0.62 & 0.08 & 0.21 & 1.61 & 0.74 & 1.60 \\ HR5901 & 5125 & 153 & 0.37 & 0.09 & 0.75 & 0.93 & 0.15 & 0.30 & 1.54 & 0.71 & 1.13 \\ HR6014 & 5068 & 072 & 0.31 & -0.12 & 0.39 & 0.59 & 0.14 & 0.05 & 1.10 & 0.70 & 1.40 \\ HR6014 & 5068 & 133 & 0.42 & 0.11 & 0.58 & 0.55 & 0.18 & 0.09 & 1.48 & 0.65 & 1.24 \\ \end{tabular} \clearpage \begin{tabular}{llllllllllll} \hline % \multicolumn{1}{c}{Source} & \multicolumn{1}{c}{T$_{e}$ } & \multicolumn{1}{c}{SNR} & \multicolumn{1}{c}{Mg5844} & \multicolumn{1}{c}{OH5920} & \multicolumn{1}{c}{HI5950} & \multicolumn{1}{c}{Al5973} & \multicolumn{1}{c}{Si5993} & \multicolumn{1}{c}{CO6018} & \multicolumn{1}{c}{CO6170} & \multicolumn{1}{c}{Si6264} & \multicolumn{1}{c}{Mg6345} \\\hline\hline % HR2456 & 38000 & 053 & -0.03 & 0.36 & 0.39 & 0.26 & 0.16 & 0.12 & -0.32 & 0.11 & 0.31 \\ HR2456 & 38000 & 073 & -0.12 & 0.18 & 0.48 & 0.10 & 0.06 & -0.15 & 0.15 & 0.03 & 0.10 \\ HR5191 & 19000 & 282 & -0.05 & 0.19 & 1.71 & 0.57 & 0.08 & -0.07 & 0.22 & 0.07 & 0.24 \\ HR3982 & 13000 & 241 & -0.08 & 0.13 & 2.22 & 0.47 & 0.04 & -0.09 & 0.28 & 0.03 & 0.15 \\ HR3982 & 13000 & 241 & -0.07 & 0.09 & 2.14 & 0.51 & 0.06 & -0.09 & 0.32 & 0.12 & 0.26 \\ HR7001 & 9480 & 678 & -0.05 & 0.36 & 2.83 & 1.06 & 0.03 & -0.03 & 0.41 & 0.15 & 0.52 \\ HR7001 & 9480 & 146 & -0.10 & 0.38 & 2.81 & 1.02 & 0.10 & -0.05 & 0.43 & 0.17 & 0.41 \\ HR2491 & 9145 & 111 & -0.07 & 0.36 & 2.71 & 0.83 & 0.16 & -0.14 & 0.37 & -0.08 & 0.10 \\ HR2491 & 9145 & 148 & -0.14 & 0.40 & 2.67 & 0.93 & 0.12 & -0.13 & 0.39 & 0.05 & 0.20 \\ HR4534 & 8593 & 205 & -0.04 & 0.45 & 2.67 & 1.01 & 0.11 & -0.12 & 0.30 & 0.07 & 0.34 \\ HR4357 & 8377 & 192 & -0.05 & 0.40 & 2.83 & 0.96 & 0.09 & -0.12 & 0.24 & 0.06 & 0.38 \\ HR4931 & 6750 & 119 & 0.04 & 0.24 & 1.47 & 0.62 & -0.01 & -0.06 & 0.09 & 0.09 & 0.86 \\ HR1279 & 6677 & 080 & 0.10 & 0.32 & 1.62 & 0.67 & 0.15 & -0.09 & 0.26 & 0.12 & 0.64 \\ HR2943 & 6530 & 327 & 0.04 & 0.33 & 1.60 & 0.57 & 0.15 & -0.14 & 0.54 & 0.27 & 0.74 \\ HR1538 & 6385 & 281 & 0.06 & 0.34 & 1.26 & 0.53 & 0.18 & -0.11 & 0.51 & 0.22 & 0.90 \\ HR4375 & 6085 & 254 & 0.26 & 0.15 & 0.63 & 0.56 & 0.15 & -0.06 & 0.68 & 0.37 & 1.09 \\ HR4983 & 5930 & 123 & 0.21 & 0.16 & 0.75 & 0.66 & 0.09 & 0.04 & 0.71 & 0.45 & 1.20 \\ HR4983 & 5930 & 173 & 0.19 & 0.21 & 0.90 & 0.52 & 0.19 & -0.06 & 0.87 & 0.47 & 0.96 \\ HR483 & 5855 & 059 & 0.24 & 0.02 & 0.68 & 0.29 & 0.04 & -0.17 & 0.18 & 0.37 & 1.09 \\ HR483 & 5855 & 079 & 0.24 & 0.19 & 0.90 & 0.46 & 0.19 & -0.11 & 0.67 & 0.48 & 1.30 \\ HR4374 & 5830 & 250 & 0.28 & 0.20 & 0.62 & 0.63 & 0.10 & -0.01 & 0.90 & 0.47 & 1.35 \\ HR5072 & 5740 & 197 & 0.26 & 0.15 & 0.74 & 0.53 & 0.16 & -0.04 & 0.99 & 0.53 & 1.28 \\ HR4496 & 5430 & 105 & 0.35 & 0.17 & 0.59 & 0.59 & 0.21 & -0.08 & 1.12 & 0.61 & 1.45 \\ HR4496 & 5430 & 090 & 0.31 & 0.16 & 0.39 & 0.50 & 0.13 & -0.04 & 0.69 & 0.43 & 1.08 \\ HR7462 & 5240 & 131 & 0.52 & 0.04 & 0.38 & 0.72 & 0.09 & 0.09 & 1.20 & 0.62 & 1.89 \\ HR7462 & 5240 & 095 & 0.51 & 0.07 & 0.37 & 0.69 & 0.13 & 0.06 & 1.16 & 0.72 & 2.05 \\ HR1084 & 5010 & 223 & 0.61 & 0.19 & 0.44 & 0.74 & 0.24 & -0.01 & 1.59 & 0.76 & 2.00 \\ HR8832 & 4785 & 111 & 0.88 & 0.14 & 0.29 & 1.06 & 0.17 & 0.18 & 1.88 & 0.90 & 2.50 \\ GL570A & 4560 & 120 & 0.90 & 0.22 & 0.37 & 1.13 & 0.28 & 0.04 & 2.02 & 0.90 & 2.29 \\ HR8085 & 4340 & 125 & 0.65 & 0.18 & 0.01 & 1.15 & 0.11 & 0.15 & 1.59 & 0.60 & 2.38 \\ HR8086 & 4040 & 170 & 0.72 & 0.39 & 0.06 & 1.46 & 0.14 & 0.11 & 1.78 & 0.50 & 2.07 \\ HR8086 & 4040 & 181 & 0.72 & 0.32 & 0.07 & 1.48 & 0.15 & 0.12 & 1.86 & 0.52 & 2.18 \\ GL338A & 3800 & 072 & 0.98 & 0.37 & 0.08 & 1.36 & 0.13 & 0.02 & 1.51 & 0.34 & 1.80 \\ GL526 & 3605 & 068 & 0.62 & 0.42 & -0.13 & 1.32 & 0.16 & 0.10 & 1.04 & 0.04 & 0.92 \\ GL411 & 3530 & 202 & 0.48 & 0.53 & -0.04 & 1.29 & 0.16 & 0.01 & 1.17 & 0.10 & 1.19 \\ GL411 & 3530 & 189 & 0.47 & 0.55 & -0.07 & 1.29 & 0.18 & 0.06 & 1.21 & 0.12 & 1.23 \\ GL725A & 3380 & 083 & 0.52 & 0.57 & -0.10 & 1.15 & 0.06 & 0.03 & 0.93 & -0.00 & 0.99 \\ GL725A & 3380 & 107 & 0.54 & 0.56 & -0.12 & 1.25 & 0.02 & 0.08 & 1.20 & -0.02 & 1.09 \\ \end{tabular} \end{document}