Table 3: IRAS point sources of TMR south. The first 4 sources are inside the region of the ISOPHOT frame, the rest are $\approx $ $1\hbox {$^\prime $ }$ outside the field, but still seen at the boundary due to the IRAS point spread function.
Source RA Dec F12 F25 F60 F100 Other name, classification and reference for class
  (2000) (2000) Jy Jy Jy Jy  
IRAS 04377+2518 04$^{\rm h}$40$^{\rm m}$37 $.\!\!^{\rm s}$9 +25$^\circ $23$^\prime $53 $^{\prime \prime }$     0.7(.1)   60 $\mu $m only point source, this paper
IRAS 04378+2521 04$^{\rm h}$40$^{\rm m}$42.6 +25$^\circ $27$^\prime $21 $^{\prime \prime }$ 1.1(.05) 1.1(.1) 0.7(.1)   HCL2-SE 2, T Tauri type, this paper
IRAS 04382+2527 04   41    17.2 +25  32  52       3.1(0.5) Cirrus knot, Harju et al. (2001)
IRAS 04379+2534 04   41    03.1 +25  39  47 0.44(.04)       TNS87 12, star, Tamura et al. (1987)
IRAS 04381+2540 04   41    12.5 +25  46  37 0.44(.06) 2.7(.2) 10.3(.8) 13.9(1.5) Protostar at the edge of TMC-1, Brown & Chandler (1999)
IRAS 04369+2539 04   39    58.4 +25  45  06 5.0(.2) 6.8(.5) 7.3(.7) 18.2(2.5) IC 2087, refl. nebula, and T Tauri stars, Koenig et al. (2001)
IRAS 04390+2517 04   42    07.6 +25  23  10 0.6(.1) 0.8(.1) 1.6(.2) 7.7(1.4) V955 Tau, T Tauri type, Rydgren & Vrba (1983)


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