Table 4: Photometric results of ISOPHOT and IRAS. All fluxes are colour-corrected and presented in Jy. (*): PHT32 observing mode. Source of IRAS data: PSC - V1735 Cyg, V346 Nor, Z CMa, Parsamian 21; Weaver & Jones (1992) - V1331 Cyg; this work (Sect. 2.4) - V1515 Cyg. In the case of V1057 Cyg the $12{-}60~\mu$m fluxes are from Weaver & Jones (1992), the flux at $100~\mu$m was re-determined in this work (Sect. 2.4).
$\lambda$ [$\mu$m] V1057 Cyg V1515 Cyg V1735 Cyg V346 Nor Z CMa Parsamian 21 V1331 Cyg
4.8 $2.67 \pm 0.67$ $1.57 \pm 0.39$ $1.29 \pm 0.32$ $ 4.59 \pm 1.15$ $53.16 \pm 13.29$    
12 $5.68 \pm 1.42$ $11.64 \pm 2.91$ $1.62 \pm 0.40$ $6.61 \pm 1.65$ $97.33 \pm 24.33$    
25 $23.19 \pm 5.80$ $11.01 \pm 2.75$ $4.94 \pm 1.24$ $30.82 \pm 7.71$ $182.8 \pm 45.7$    
60 $52.99 \pm 14.11$ $25.80 \pm 6.45$ $41.76 \pm 10.44$ $46.54 \pm 13.45$ $290.1 \pm 72.5$    
65* $42.26 \pm 10.57$   $38.68 \pm 9.67$     $18.51 \pm 4.63$  
100 $34.50 \pm 9.28$   $77.23 \pm 19.31$ $39.52 \pm 11.65$ $479.1 \pm 119.8$    
100* $62.06 \pm 15.52$   $86.82 \pm 21.71$     $20.71 \pm 5.18$  
120   $78.45 \pm 24.03$          
IRAS-12 $14.89 \pm 0.11$ $3.7{\pm}1.0$ $2.19 \pm 0.20$ $9.73 \pm 0.39$ $125.1 \pm 5.0$ $0.80 \pm 0.06$ $1.12 \pm 0.03$
IRAS-25 $28.72 \pm 0.08$ $6.8{\pm}2.1$ $8.09 \pm 0.52$ $30.98 \pm 1.33$ $204.5 \pm 8.7$ $4.07 \pm 0.26$ $2.62 \pm 0.02$
IRAS-60 $53.71 \pm 2.48$ $25{\pm}10$ $40.84 \pm 4.90$ $69.07 \pm 4.83$ $312.3 \pm 40.6$ $11.49 \pm 1.03$ $6.88 \pm 0.23$
IRAS-100 $47.0 \pm 10.0$ <110 $92.97 \pm 15.63$ $74.91 \pm 4.20$ $375.5 \pm 63.2$ $15.58 \pm 2.04$ $8.22 \pm 1.19$


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