\begin{table}%t3 \caption{\label{all-species}List of detected lines, for all species except CH$_3$OH and CH$_3$OCH$_3$.} \par %\centering \par \begin{tabular}{lc|cc|cc|cc|cc|cc} \hline \hline Transition & Freq. & \multicolumn{2}{c|}{L1157-B1} & \multicolumn{2}{c|}{IRAS~16293} & \multicolumn{2}{c|}{OMC2-IRAS~4} & \multicolumn{2}{c|}{AFGL~2591} & \multicolumn{2}{c}{NGC~6334I}\\ & & $T_{\rm mb}\Delta v$ & $\Delta v$ & $T_{\rm mb}\Delta v$ & $\Delta v$ & $T_{\rm mb}\Delta v$ & $\Delta v$ & $T_{\rm mb}\Delta v$ & $\Delta v$ & $T_{\rm mb}\Delta v$ & $\Delta v$ \\ & (GHz) & K km~s$^{-1}$ & km~s$^{-1}$ & K km~s$^{-1}$ & km~s$^{-1}$ & K km~s$^{-1}$ & km~s$^{-1}$ & K km~s$^{-1}$ & km~s$^{-1}$ & K km~s$^{-1}$ & km~s$^{-1}$\\ \hline H$_2$O: $1_{10}{-}1_{01}$& 556.936 & 14.75(0.33) & 11.6 & 17.62(0.49) & 6.8 & 17.26(0.57) & 8.8 & 3.35(0.46) & 3.0 & $\leq$1.51\tablefootmark{a} & --\\ H$_2$O: $5_{32}{-}4_{41}$& 620.701 & $\leq$0.12 & -- & 1.80(0.18) & 9.9 & $\leq$0.15 & -- & $\leq$0.43 & -- & 5.15(0.52)\tablefootmark{a} & 8.8\\ \hline HDO: $2_{11}{-}2_{02}$&599.927 & $\leq$0.12 & -- & 0.73(0.23) & 4.6 & $\leq$0.11 & -- & $\leq$0.35 & -- & 1.67(0.45) & 6.8\\ \hline CO: 5--4& 576.268 & 54.20(0.32) & 4.8 & 87.78(1.82) & 9.7 & 147.59(0.74) & 11.3 & 165.52(0.93) & 7.8 & 133.63(9.63)\tablefootmark{a} & 4.2\\ \hline C$^{17}$O: 5--4& 561.713 & $\leq$0.16 & -- & 2.46(0.32) & 2.9 & 1.09(0.17) & 2.2 & 4.28(0.57) & 3.4 & 15.47(0.89) & 4.6\\ \hline HCO$^+$: 7--6& 624.208 & 0.11(0.03) & -- & 17.70(0.18) & 2.4 & 16.87(0.18) & 4.1 & 9.99(0.40) & 3.8 & 32.36(1.24) & 5.9\\ \hline H$^{13}$CO$^+$: 7--6 & 607.175 & $\leq$0.12 & -- & 0.68(0.24) & 3.0 & $\leq$0.96 & -- & $\leq$0.37 & -- & 4.12(3.60) & 5.0\\ \hline HCN: 7--6& 620.304 & 0.96(0.13) & 7.4 & 5.45(0.16) & 5.2 & 16.87(0.38) & 8.9 & 2.66(0.28) & 3.7 & 21.39(0.70) & 8.0\\ \hline H$^{13}$CN: 7--6& 604.268 & $\leq$0.10 & -- & 0.57(0.14) & 6.0 & 0.77(0.11) & 12.3 & $\leq$0.33 & -- & 6.81(0.43)\tablefootmark{b} & 12.9\\ \hline DCN: 8--7& 579.205 & $\leq$0.09 & -- & 0.29(0.12) & 6.0 & $\leq$0.10 & 2.5 -- & $\leq$0.28 & -- & 1.2(4.38)\tablefootmark{b} & 4.2\\ \hline HNC: 7--6& 634.510 & $\leq$0.18 & -- & 0.58(0.17) & 3.8 & 0.35(0.20) & 1.7 & $\leq$0.45 & -- & 3.26(0.74) & 6.6\\ \hline CN: $5_{05}{-}4_{04}$ & 566.731& $\leq$0.09 & -- & $\leq$0.09 & -- & 1.77(0.10) & 6.1 & 0.79(0.25) & 3.2 & 4.13(1.49) & 7.8\\ CN: $5_{06}{-}4_{05}$ & 566.947& $\leq$0.11 & -- & $\leq$0.10 & -- & 1.39(0.19) & 3.4 & 0.98(0.26) & 3.0 & 4.12(1.38) & 5.8\\ \hline N$_2$H$^+$: 6--5& 558.967 & $\leq$0.14 & -- & 0.45(0.15) & 1.9 & 6.84(0.12) & 2.2 & $\leq$0.26 & -- & 11.87(1.77) & 4.5\\ \hline NH$_3$: $1,0_{0}{-}0,0_{1}$ & 572.497 & 1.26(0.09) & 7.6 & 2.8(0.15)\tablefootmark{b} & 3.5 & 8.32(0.14) & 4.5 & 3.52(0.27) & 4.2 & 7.79(0.66) & 3.8\\ \hline HCl\tablefootmark{c}: 1--0& 625.902 & $\leq$0.13 & -- & 2.24(0.15) & 2.0 & 0.42(0.14) & 2.2 & 2.05(0.30) & 3.1 & 20.06(1.34)\tablefootmark{b} & 18.5\\ \hline H$^{37}$Cl\tablefootmark{c}:1--0& 624.978 & $\leq$0.13 & -- & 0.76(0.18) & 1.5 & 0.28(0.12) & 4.1 & $\leq$0.33 & -- & 5.63(3.09) & 13.4\\ \hline CCH: $7_{8}{-}6_{7}$ & 611.265 & $\leq$0.11 & -- & $\leq$0.11 & -- & 0.78(0.13) & 2.8 & $\leq$0.26 & -- & 2.15(1.06) & 7.2\\ CCH: $7_{7}{-}6_{6}$ & 611.328 & $\leq$0.11 & -- & $\leq$0.12 & -- & 0.84(0.15) & 3.9 & $\leq$0.26 & -- & 1.33(1.15) & 6.1\\ \hline H$_2$CO: $8_{18}{-}7_{17}$ & 561.899 & 0.63(0.11) & 4.4 & 4.21(0.18) & 4.2 & 6.61(0.16) & 4.3 & $\leq$0.39 & -- & 9.98(0.59) & 6.5\\ H$_2$CO: $8_{08}{-}7_{07}$ & 576.708 & 0.39(0.11) & 7.9 & 2.00(0.10) & 4.5 & 2.65(0.10) & 4.2 & $\leq$0.22 & -- & 7.13(0.48) & 7.1\\ H$_2$CO: $8_{27}{-}7_{26}$ & 581.612 & $\leq$0.09 & -- & 1.19(0.11) & 5.2 & 1.53(0.12) & 4.1 & $\leq$0.26 & -- & 4.40(0.52) & 5.3\\ H$_2$CO: $8_{54}{-}7_{53}$ & 582.382 & $\leq$0.09 & -- & 0.51(0.15) & 6.2 & 0.79(0.14) & 3.4 & $\leq$0.27 & -- & 3.16(0.38) & 5.7\\ H$_2$CO: $8_{35}{-}7_{34}$ & 583.309 & $\leq$0.11 & -- & 1.57(0.14) & 4.9 & 2.01(0.12) & 3.9 & $\leq$0.32 & -- & 5.39(0.83) & 5.9\\ H$_2$CO: $8_{26}{-}7_{25}$ & 587.454 & $\leq$0.12 & -- & 1.18(0.14) & 4.9 & 1.18(0.12) & 3.7 & $\leq$0.35 & -- & 4.05(0.45) & 4.8\\ H$_2$CO: $8_{17}{-}7_{16}$ & 600.331 & 0.19(0.04) & 8.2 & 3.43(0.19) & 4.3 & 5.11(0.14) & 4.6 & $\leq$0.37 & -- & 8.79(0.50) & 6.7\\ H$_2$CO: $8_{19}{-}7_{18}$ & 631.703 & 0.44(0.11) & 3.8 & 3.41(0.15) & 4.4 & 5.08(0.14) & 4.4 & $\leq$0.35 & -- & 8.14(0.69) & 6.4\\ \hline H$_2$S: $6_{42}{-}6_{33}$ & 567.080 & $\leq$0.09 & -- & $\leq$0.10 & -- & $\leq$0.09 & -- & $\leq$0.21 & -- & 1.46(0.73) & 9.2\\ H$_2$S: $3_{31}{-}3_{22}$ & 568.051 & $\leq$0.08 & -- & 0.48(0.13) & 4.5 & $\leq$0.14 & -- & $\leq$0.22 & -- & 3.40(0.50) & 5.0\\ H$_2$S: $5_{50}{-}5_{41}$ & 579.795 & $\leq$0.09 & -- & $\leq$0.13 & -- & $\leq$0.14 & -- & $\leq$0.23 & -- & 2.84(0.50) & 5.2\\ H$_2$S: $5_{32}{-}5_{23}$ & 611.442 & $\leq$0.10 & -- & 0.40(0.14) & 6.4 & $\leq$0.11 & -- & $\leq$0.25 & -- & 1.98(0.72) & 6.4\\ \hline CS: 12--11& 587.616 & 0.19(0.03) & 5.2 & 3.18(0.17) & 4.2 & 4.10(0.14) & 10.9 & 0.92(0.28) & 4.5 & 15.13(0.49) & 6.7\\ \hline C$^{34}$S: 12--11& 578.216 & $\leq$0.09 & -- & 0.42(0.11) & 5.4 & $\leq$0.11 & -- & $\leq$0.24 & -- & 8.68(0.50) & 7.7\\ C$^{34}$S: 13--12& 626.349 & $\leq$0.11 & -- & 0.40(0.14) & 5.0 & $\leq$0.15 & -- & $\leq$0.31 & -- & 3.92(0.69) & 5.4\\ \hline SO: $13_{12}{-}12_{11}$ & 558.087 & $\leq$0.14 & -- & 2.77(0.14) & 5.2 & $\leq$0.14 & -- & $\leq$0.30 & -- & 3.55(0.33) & 4.9\\ SO: $13_{13}{-}12_{12}$ & 559.319 & $\leq$0.11 & -- & 2.88(0.14) & 5.4 & $\leq$0.12 & -- & $\leq$0.33 & -- & 3.64(0.35) & 5.6\\ SO: $13_{14}{-}12_{13}$ & 560.178 & $\leq$0.11 & -- & 3.12(0.17) & 5.1 & $\leq$0.12 & -- & 0.76(0.22) & 4.4 & 4.83(0.37) & 6.6\\ SO: $14_{13}{-}13_{12}$ & 601.258 & $\leq$0.09 & -- & 2.53(0.14) & 5.5 & $\leq$0.12 & -- & 0.92(0.24) & 5.4 & 2.89(0.52) & 5.0\\ SO: $14_{14}{-}13_{13}$ & 602.292 & $\leq$0.12 & -- & 2.25(0.21) & 5.1 & $\leq$0.16 & -- & $\leq$0.38 & -- & 2.28(0.69) & 4.3\\ SO: $14_{15}{-}13_{14}$ & 603.021 & $\leq$0.10 & -- & 2.84(0.13) & 5.5 & $\leq$0.14 & -- & $\leq$0.31 & -- & 3.94(0.38) & 5.6\\ \hline SO$_2$: $5_{51}{-}4_{40}$ & 555.666 & $\leq$0.26 & -- & 0.77(0.22) & 4.1 & $\leq$0.18 & -- & $\leq$0.52 & -- & $\leq$1.43) & --\\ SO$_2$: $15_{610}{-}15_{511}$ & 560.891 & $\leq$0.10 & -- & 0.49(0.12) & 8.3 & $\leq$0.11 & -- & $\leq$0.26 & -- & 0.69(0.33) & 3.6\\ SO$_2$: $13_{68}{-}13_{59}$& 561.266 & $\leq$0.12 & -- & $\leq$0.13 & -- & $\leq$0.13 & -- & $\leq$0.29 & -- & 2.49(0.39)\tablefootmark{b} & 5.2\\ SO$_2$: $11_{66}{-}11_{57}$& 561.491 & $\leq$0.10 & -- & $\leq$0.11 & -- & $\leq$0.12 & -- & $\leq$0.25 & -- & 1.02(0.38) & 6.1\\ SO$_2$: $10_{64}{-}10_{55}$& 561.560 & $\leq$0.09 & -- & $\leq$0.14 & -- & $\leq$0.11 & -- & $\leq$0.27) & -- & 0.86(0.55) & 5.0\\ SO$_2$: $11_{48}{-}10_{37}$& 567.593 & $\leq$0.10 & -- & 0.61(0.10) & 4.7 & $\leq$0.12 & -- & $\leq$0.24 & -- & 1.00(0.31) & 4.4\\ SO$_2$: $6_{51}{-}5_{42}$& 574.807 & $\leq$0.07 & -- & 0.72(0.10) & 4.2 & $\leq$0.11 & -- & $\leq$0.25 & -- & 1.31(0.26) & 5.9\\ SO$_2$: $12_{48}{-}11_{39}$& 587.568 & $\leq$0.11 & -- & 0.69(0.14) & 5.5 & $\leq$0.69 & -- & $\leq$0.37 & -- & 2.15(1.92) & 7.0\\ SO$_2$: $7_{53}{-}6_{42}$& 593.945 & $\leq$0.12 & -- & 0.60(0.12) & 3.9 & $\leq$0.14 & -- & $\leq$0.37 & -- & 0.66(0.58) & 3.3\\ SO$_2$: $13_{410}{-}12_{39}$& 604.367 & $\leq$0.07 & -- & 0.88(0.11) & 5.9 & $\leq$0.12 & -- & $\leq$0.30 & -- & 1.16(0.34) & 4.2\\ SO$_2$: $8_{53}{-}7_{44}$& 613.076 & $\leq$0.08 & -- & 0.62(0.12) & 4.1 & $\leq$0.10 & -- & $\leq$0.19 & -- & 1.33(0.62) & 5.9\\ SO$_2$: $14_{410}{-}13_{311}$& 626.087 & $\leq$0.09 & -- & 0.56(0.15) & 4.4 & $\leq$0.12 & -- & $\leq$0.28 & -- & $\leq$1.14 & --\\ SO$_2$: $9_{55}{-}8_{44}$& 632.193 & $\leq$0.12 & -- & 0.63(0.16) & 4.2 & $\leq$0.16 & -- & $\leq$0.26 & -- & 1.63(0.47) & 5.1\\ \hline \end{tabular} \tablefoot {The CH$_3$OH lines detected in at least a source other than NGC~6334I are reported in Table~4. Note that we did not report the list of CH$_3$OCH$_3$~lines as they are detected in NGC~6334I only and are the focus of a forthcoming paper. For each source, we report the main beam temperature integrated intensity~$T_{\rm mb}\Delta v$ (K~km~s$^{-1}$), and the FWHM $\Delta v$ (km~s$^{-1}$) obtained by fittting the line with a gaussian. In parenthesis we report the rms over the same integration interval of the line intensity. Only lines with rms larger than~3 are considered detected, except in the case of NGC~6334I, where~1$\sigma$ was taken since the rms is artificially higher because of the line-crowed spectrum. Upper limits refer to~1$\sigma$. \\ \tablefoottext{a}{Line is heavily absorbed;} \tablefoottext{b}{line is merged;} \tablefoottext{c}{only the central component.}} \end{table}