\begin{table}%t4 \caption{Candidate young stellar objects of the region: reddened NIR point sources and nebulosities with T~Tauri-like NIR colours, X-ray point sources. The classification, as indicated, is based on $J$, $H$, $K$~photometry, NIR~spectroscopy, or X-ray hardness ratio (HR). The columns are: (1)~object name, (2--3) equatorial coordinates, (4) classification method, (5) associated cloud and separation, (6) other identifications of the same source. \label{YSO} } { \begin{tabular}{lllllcc} \hline \hline Source & RA (2000) & Dec(2000)& Class & Cloud & Sep. & Other identifications \\ \hline %2MASS TMRS20 &04$^{\rm h}$41$^{\rm m}$11\fs2& +25\degr 25\arcmin 16\arcsec &JHK&HCL2-ES&0\arcmin&\\ %2MASS TMRS22 &04~~ 41~~ 37.7 & +25~ 24 39& JHK& HCL2-ES &1\arcmin&\\ % 2MASS TMRS1& 04$^{\rm h}$39$^{\rm m}$59\fs3& +25\degr 26\arcmin 43\arcsec& {\it JHK}&&\\ 2MASS TMRS2& 04~~ 39~~ 54.9& +25~~26~~49& {\it JHK}&&\\ 2MASS TMRS3& 04~~ 39~~ 56.7& +25~~38~~36& {\it JHK}&HCL2-B&1\arcmin &\\ 2MASS TMRS4& 04~~ 40~~ 20.3& +25~~15~~10& {\it JHK}&&\\ 2MASS TMRS5& 04~~ 40~~ 34.4& +25~~25~~23& {\it JHK}&&\\ 2MASS TMRS6& 04~~ 40~~ 47.2& +25~~24~~21& {\it JHK}&&\\ 2MASS TMRS7& 04~~ 41~~ 41.3& +25~~25~~14& {\it JHK}& HCL2-ES&2\arcmin &\\ 2MASS TMRS8& 04~~ 42~~ 03.4& +25~~25~~36& {\it JHK}&&\\ 2MASS TMRS9& 04~~ 40~~ 04.6& +25~~27~~31& {\it JHK}&&\\ 2MASS TMRS10& 04~~ 40~~ 41.1& +25~~28~~35& {\it JHK}& HCL2-E &0\arcmin& IRAS~04378+2521 (within err. ellipse)\\ 2MASS TMRS11& 04~~ 41~~ 17.6& +25~~29~~28& {\it JHK}&&\\ 2MASS TMRS12& 04~~ 41~~ 53.4& +25~~28~~32& {\it JHK}&&\\ 2MASS TMRS13& 04~~ 42~~ 01.8& +25~~26~~35& {\it JHK}&&\\ 2MASS TMRS14& 04~~ 40~~ 07.9& +25~~30~~07& {\it JHK}& HCL2-E &2\arcmin&\\ 2MASS TMRS15& 04~~ 40~~ 27.5& +25~~30~~33& {\it JHK}& HCL2-E &0\arcmin&\\ 2MASS TMRS16& 04~~ 40~~ 02.2& +25~~37~~25& {\it JHK}& HCL2-B&3\arcmin &\\ 2MASS TMRS17& 04~~ 40~~ 00.0& +25~~33~~56& {\it JHK}&&\\ 2MASS TMRS18& 04~~ 40~~ 49.1& +25~~36~~18& {\it JHK}&&\\ 2MASS TMRS19& 04~~ 40~~ 59.9& +25~~34~~06& {\it JHK}&&\\ 2MASS TMRS20& 04~~ 41~~ 31.9& +25~~36~~50& {\it JHK}& TMC-1~CP& 1\arcmin&\\ 2MASS TMRS21& 04~~ 41~~ 59.0& +25~~34~~02& {\it JHK}& TMC-1~CP& 0\arcmin&\\ 2MASS TMRS22& 04~~ 41~~ 48.3& +25~~34~~31& {\it JHK}& TMC-1~CP& 0\arcmin&\\ 2MASS TMRS23& 04~~ 41~~ 46.8& +25~~38~~25& {\it JHK}& TMC-1~CP& 0\arcmin&\\ 2MASS TMRS24& 04~~ 42~~ 02.0& +25~~40~~11& {\it JHK}& TMC-1~CP& 0\arcmin&\\ 2MASS TMRS25& 04~~ 41~~ 13.2& +25~~41~~25& {\it JHK}& TMC-1~CP& 3\arcmin&\\ \hline \object{ITG 26} & 04$^{\rm h}$40$^{\rm m}$28\fs3 & +25\degr 26\arcmin 56\arcsec&{\it JHK}&HCL2-E&4\arcmin& 2MASS~J043959.39+253120.8 \\ \object{ITG 31} & 04~~ 41~~ 02.7 & +25~~ 39~ 48& {\it JHK} & TMC-1~CP & 6\arcmin& 2MASS~J043922.60+253428.2\\ \object{ITG 32} & 04~~ 41~~ 04.0 & +25~~ 30~ 23& {\it JHK} & HCL2-ES & 2\arcmin& 2MASS~J043940.80+253544.6\\ \object{ITG 37} & 04~~ 41~~ 17.9 & +25~~ 42~ 08& {\it JHK} & TMC-1~CP & 3\arcmin& 2MASS~J043912.01+254110.1\\ \object{ITG 38} & 04~~ 41~~ 19.2 & +25~~ 24~ 26& {\it JHK} & HCL2-ES & 2\arcmin& 2MASS~J043922.51+254032.4\\ \object{ITG 40} & 04~~ 41~~ 24.7 & +25~~ 43~ 53& NIRspec.& TMC-1~CP & 0\arcmin& 2MASS~J043956.66+253836.3\\ \object{ITG 44} & 04~~ 41~~ 43.3 & +25~~ 24~ 11& {\it JHK} & TMC-1NH$_3$ & 3\arcmin& 2MASS~J043944.58+254308.3\\ \object{ITG 47} & 04~~ 42~~ 00.0 & +25~~ 22~ 50& {\it JHK} & TMC-1NH$_3$ & 3\arcmin& 2MASS~J043840.03+254518.6\\ \object{ITG 48} & 04~~ 42~~ 05.0 & +25~~ 22~ 57& {\it JHK} & TMC-1NH$_3$ & 3\arcmin& 2MASS~J043835.16+254825.6\\ \object{ITG 49} & 04~~ 42~~ 06.0 & +25~~ 39~ 11& {\it JHK} & TMC-1NH$_3$ & 3\arcmin& 2MASS~J043920.91+254502.1\\ \hline \object{HCL2 SE-2} & 04$^{\rm h}$40$^{\rm m}$42\fs6 & +25\degr 26\arcmin 21\arcsec &HR, FIR, {\it JHK} & HCL2-E & 3\arcmin & IRAS~04378+2521, 2MASSX J04404265+2525466\\ \object{1RXS J044001.3+253408} & 04~~ 40~~ 01.3 & +25~~ 34~~ 08 &HR & HCL2-E & 3\arcmin & \\ \object{1RXS J044009.8+253533} & 04~~ 40~~ 09.8 & +25~~ 35~~ 33 &HR & HCL2-E & 4\arcmin & \\ \hline \end{tabular}} \end{table}