\begin{table}%t4 \par \caption {\label{tab:droxo_irs_results}Results from the analysis of the {\it Spitzer}/IRS and DROXO datasets (cf. Sects.~\ref{sect:ana_X} and~\ref{sect:ana_Ne}).} %\centerline $$ {\begin{tabular}{lr@{}lrr@{}lr|cr@{}lr@{}lr@{}l} \hline\hline Name& \multicolumn{2}{c}{$\rm L_{\rm [NeII]}$}& $\rm F_{\rm [NeII]}^{\rm cont}$& \multicolumn{2}{c}{$L_{\rm [NeIII]}$}& $F_{\rm [NeIII]}^{\rm cont.}$& Instr.&\multicolumn{2}{c}{$N_{\rm H}$}& \multicolumn{2}{c}{$kT$}& \multicolumn{2}{c}{$L_{\rm X}$}\\ & \multicolumn{2}{c}{[$10^{28}$~erg~s$^{-1}$]}& [Jy]& \multicolumn{2}{c}{[$10^{28}$~erg~s$^{-1}$]}& [Jy]& &\multicolumn{2}{c}{[$10^{22}$~cm$^{-2}$]}&\multicolumn{2}{c}{[keV]}& \multicolumn{2}{c}{[$10^{28}$~erg~s$^{-1}$]}\\ \hline DoAr25/GY17& $1.00$&$_{ 0.80}^{ 1.19}$& 0.26& $<$0.49& & 0.28& pn & $0.97$& $_{ 0.92}^{ 1.03}$& $2.74$& $_{ 2.54}^{ 2.95}$& $180.64$& $_{ 170.89}^{ 193.12}$\\ IRS14/GY54 & $<$5.43& & 0.28& $<$2.18& & 0.12& ACIS$^1$& & & & & $2.14$& $_{ 1.07}^{ 3.21}$\\ WL12/GY111 & $43.29$&$_{ 21.48}^{ 59.14}$& 39.20& $<$20.44& & 28.55& all & $14.62$& $_{ 7.12}^{ 39.18}$& $64.00$& & $12.14$& $_{ 6.88}^{ 49.82}$\\ WL22/GY174 & $<$397.59& & 73.63& $<$26.61& & 11.97& m1+pn & $14.11$& $_{ 10.74}^{ 18.30}$& $2.35$& $_{ 1.72}^{ 3.49}$& $98.80$& $_{ 49.56}^{ 216.32}$\\ WL16/GY182 & $<$80.07& & 29.03& $<$36.24& & 8.29& ACIS$^1$& & & & & $2.19$& $_{ 0.69}^{ 6.92}$\\ WL17/GY205 & $<$23.40& & 2.01& $<$17.84& & 2.09& all & $3.73$& $_{ 2.20}^{ 5.91}$& $3.43$& $_{ 1.97}^{ 10.71}$& $7.88$& $_{ 3.97}^{ 17.53}$\\ WL10/GY211 & $5.44$&$_{ 4.43}^{ 6.45}$& 0.41& $<$2.79& & 0.40& pn & $2.80$& $_{ 2.29}^{ 3.30}$& $4.85$& $_{ 3.73}^{ 7.56}$& $39.66$& $_{ 30.92}^{ 49.58}$\\ EL29/GY214 & $<$78.98& & 67.46& $<$40.82& & 47.74& m2 & $6.37$& $_{ 5.81}^{ 7.15}$& $4.23$& $_{ 3.57}^{ 4.90}$& $159.79$& $_{ 131.08}^{ 200.10}$\\ GY224 & $<$5.51& & 1.36& $<$4.33& & 1.38& m1+m2 & $3.42$& $_{ 2.66}^{ 4.50}$& $8.62$& $_{ 4.35}^{ 32.06}$& $20.58$& $_{ 17.21}^{ 30.18}$\\ WL19/GY227 & $<$15.17& & 1.63& $<$9.32& & 1.06& all & $9.92$& $_{ 8.47}^{ 11.55}$& $3.49$& $_{ 2.84}^{ 4.53}$& $75.45$& $_{ 54.90}^{ 104.74}$\\ WL11/GY229 & $<$0.31& & 0.03& $<$0.37& & 0.04& all$^2$ & & & & & $<$2.69& \\ WL20/GY240 & $19.80$&$_{ 19.00}^{ 20.60}$& 1.74& $<$4.87& & 3.09& pn & $2.28$& $_{ 2.16}^{ 2.39}$& $2.48$& $_{ 2.41}^{ 2.64}$& $115.98$& $_{ 107.26}^{ 124.97}$\\ IRS37/GY244& $20.49$&$_{ 14.12}^{ 30.52}$& 1.59& $<$4.72& & 1.50& ACIS$^3$& $5.80$& $_{ 4.00}^{ 8.80}$& $>$$1.70$& & $18.20$& $_{ 5.75}^{ 57.54}$\\ WL5/GY246 & $5.25$&$_{ 4.05}^{ 6.45}$& 0.81& $1.40$&$_{ 1.09}^{ 1.71}$& 0.38& all & $6.62$& $_{ 5.93}^{ 7.30}$& $4.05$& $_{ 3.37}^{ 5.20}$& $621.86$& $_{ 496.86}^{ 762.79}$\\ IRS42/GY252& $<$7.73& & 6.32& $<$6.89& & 5.48& ACIS$^4$& $3.90$& $_{ 2.70}^{ 5.20}$& $1.30$& $_{ 0.90}^{ 2.00}$& $28.18$& $_{ 12.02}^{ 72.44}$\\ GY253 & $<$0.63& & 0.01& $<$0.43& & 0.01& pn & $3.42$& $_{ 3.21}^{ 3.62}$& $2.62$& $_{ 2.44}^{ 2.83}$& $122.82$& $_{ 110.46}^{ 135.85}$\\ WL6/GY254 & $<$41.10& & 28.77& $<$22.26& & 19.70& all & $5.73$& $_{ 4.22}^{ 7.36}$& $8.00$& $_{ 4.53}^{ 43.45}$& $40.21$& $_{ 31.00}^{ 59.38}$\\ CRBR85 & $<$10.72& & 4.98& $<$7.31& & 4.21& all$^2$ & & & & & $<$7.41& \\ IRS43/GY265& $261.59$&$_{251.96}^{271.32}$& 12.30& $<$35.94& & 12.44& pn & $4.57$& $_{ 4.40}^{ 4.75}$& $3.00$& $_{ 2.85}^{ 3.16}$& $277.03$& $_{ 258.23}^{ 296.42}$\\ IRS44/GY269& $90.62$&$_{ 63.85}^{117.43}$& 62.53& $<$87.12& & 69.45& pn & $7.17$& $_{ 6.81}^{ 7.55}$& $3.71$& $_{ 3.42}^{ 4.04}$& $242.14$& $_{ 218.22}^{ 267.08}$\\ IRS45/GY273& $9.99$&$_{ 8.12}^{ 11.86}$& 1.22& $<$2.82& & 1.15& all & $1.00$& $_{ 0.33}^{ 1.86}$& $4.77$& $_{ 1.59}^{ 0.00}$& $6.58$& $_{ 3.66}^{ 16.27}$\\ IRS46/GY274& $<$13.05& & 6.63& $<$11.69& & 5.44& pn & $8.43$& $_{ 5.63}^{ 13.20}$& $4.78$& $_{ 2.99}^{ 8.92}$& $14.72$& $_{ 8.75}^{ 29.62}$\\ IRS47/GY279& $10.29$&$_{ 7.68}^{ 12.89}$& 4.74& $<$5.73& & 3.81& all & $1.95$& $_{ 1.30}^{ 2.90}$& $2.12$& $_{ 1.23}^{ 3.83}$& $18.83$& $_{ 10.90}^{ 39.40}$\\ GY289 & $<$0.49& & 0.05& $<$0.42& & 0.06& all & $1.93$& $_{ 1.68}^{ 2.20}$& $3.09$& $_{ 2.55}^{ 3.85}$& $27.79$& $_{ 23.16}^{ 33.36}$\\ GY291 & $<$1.01& & 0.19& $<$0.70& & 0.16& all & $2.33$& $_{ 2.04}^{ 2.60}$& $2.50$& $_{ 2.14}^{ 3.07}$& $34.87$& $_{ 28.39}^{ 41.50}$\\ IRS48/GY304& $<$37.55& & 15.80& $<$18.56& & 23.48& all$^2$ & & & & & $<$25.70& \\ IRS51/GY315& $<$19.38& & 7.23& $<$13.53& & 6.31& m1 & $3.46$& $_{ 3.09}^{ 3.83}$& $2.67$& $_{ 2.33}^{ 3.20}$& $111.89$& $_{ 91.87}^{ 133.90}$\\ IRS54/GY378& $<$19.34& & 2.76& $<$8.87& & 3.21& all & $20.05$& $_{ 6.48}^{ 42.87}$& $2.32$& & $45.21$& $_{ 0.00}^{1368.17}$\\ \hline \end{tabular}} $$ \smallskip Notes: IR and X-ray fluxes and luminosities are corrected for extinction. Column~6 indicates the {\rm XMM-Newton}/EPIC or {\it Chandra} (ACIS) detector(s) whose data was used for the fitting of the X-ray spectra: m1~=~MOS1, m2~=~MOS2, pn~=~pn, all~=~MOS1~+~MOS2~+~pn. Notes indicate the origin of $N_{\rm H}$, $kT$, and $L_{\rm X}$ for objects with no usable DROXO detection (Sect.~\ref{sect_ana_X_noDROXO}): $^1$ $L_{\rm X}$ from ACIS count-rate; $^2$ $L_{\rm X}$ upper limit from DROXO data; $^3$ $N_{\rm H}$ and $kT$ from the spectral analysis of {\it Chandra} ACIS data by \citet{ima01}, $L_{\rm X}$ from ACIS count-rate; $^4$ $N_{\rm H}$, $kT$, and $L_{\rm X}$ from \citet[][$L_{\rm X}$ corrected for the differences in the assumed distance and energy band]{ima01}. \end{table}