Table 1:

Target information and Herschel flux densities.

Name
RA, Dec (J2000) Type $F_\nu$ (mJy)
      100 $\mu $m 160 $\mu $m 250 $\mu $m 350 $\mu $m 500 $\mu $m

R71
05$^{\rm h}$02$^{\rm m}$07.39$^{\rm s}$, -71 ${\hbox{$^\circ$ }}$20 ${\hbox{$^\prime$ }}$13.1 ${\hbox{$^{\prime\prime}$ }}$ LBV $447\pm8$ $105\pm10$ $50\pm6$ $49\pm13$ $27\pm9$
IRAS05280-6910 05$^{\rm h}$27$^{\rm m}$40.11$^{\rm s}$, -69 ${\hbox{$^\circ$ }}$08 ${\hbox{$^\prime$ }}$04.5 ${\hbox{$^{\prime\prime}$ }}$ RSG, OH/IR ... ... $205\pm8$ $46\pm13$ <$11\pm10$
HD 36402 05$^{\rm h}$26$^{\rm m}$03.94$^{\rm s}$, -67 ${\hbox{$^\circ$ }}$29 ${\hbox{$^\prime$ }}$57.9 ${\hbox{$^{\prime\prime}$ }}$ WC4(+O?)+O8I ... ... ... ... ...
HD 36402 IR1/YSO2 05$^{\rm h}$26$^{\rm m}$02.99$^{\rm s}$, -67 ${\hbox{$^\circ$ }}$29 ${\hbox{$^\prime$ }}$57.7 ${\hbox{$^{\prime\prime}$ }}$ YSO? $531\pm10$ $872\pm33$ $677\pm33$ <$431\pm23$ <$132\pm21$

Notes. Quoted uncertainties are 1$\sigma$. Upper limits are either below the 3$\sigma$ detection level or include substantial flux from an adjacent unresolved source. IRAS05280-6910 does not fall within the PACS coverage. The WR star itself is not resolved in Herschel images; it is severely blended with an IR source (IR1/YSO2). The 350 and 500 $\mu $m fluxes of IR1/YSO2 include a nearby YSO (N51-YSO1), which is unresolved from IR1/YSO2 at these wavelengths. Aperture corrections for PACS and SPIRE were estimated using the current point-spread functions, and are roughly 1.4 and 1.2, respectively. None of the sources are heavily affect by high and/or variable backgrounds (Fig. 1).


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