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Table D.2:

Photometric data.

Star 		$\lambda$ $F_{\nu}$ Reference Star $\lambda$ $F_{\nu}$ Reference Star $\lambda$ $F_{\nu}$ Reference
  [$\mu $m] [Jy]     [$\mu $m] [Jy]     [$\mu $m] [Jy]  
o Cet 0.55 229.94 (1) CW Leo 1.25 2.3 (21) WX Psc 1.23 3.17 (1)
  0.55 9.76 (9)   1.25 2.7 (2)   1.25 1.69 (2)
  0.7 1104.27 (10)   1.65 74.9 (2)   1.65 14.25 (2)
  0.7 1138.92 (1)   1.65 39.6 (21)   2.17 86.52 (2)
  0.88 2131.97 (1)   2.17 469 (2)   2.2 113.8 (1)
  0.88 5871.93 (1)   2.2 388.8 (21)   3.5 220 (3)
  0.9 5027.64 (10)   2.2 321.9 (3)   3.5 330.67 (1)
  1.04 7193.59 (10)   3.5 3046.1 (3)   4.9 365.1 (3)
  1.25 3128.15 (2)   3.6 9072 (21)   12 1120 (4)
  1.25 9698.38 (10)   4.9 9010.7 (3)   12 646.9 (3)
  1.25 3845.33 (1)   10.2 39188.4 (21)   25 929.3 (3)
  1.25 9748.4 (1)   12 47500 (6)   25 921 (4)
  1.65 4364.15 (2)   12 31773.4 (3)   34.6 498.5 (5)
  2.17 5118.35 (2)   25 23100 (6)   60 212 (4)
  2.2 11275.24 (1)   25 28610.8 (3)   60 175.3 (3)
  2.2 5446.6 (1)   60 5650 (6)   100 68.8 (3)
  2.2 5927.1 (3)   60 5585 (3)   100 67.5 (4)
  2.25 11149.2 (10)   100 2017.5 (3)   400 3 (14)
  3.5 4334.9 (3)   100 922 (6)   1200 0.16 (19)
  3.5 10023.4 (10)   140 1051.5 (3)   1200 0.33 (19)
  3.5 4606.73 (1)   377 35.2 (22)   1300 0.08 (13)
  4.9 3220.5 (3)   400 32 (14)        
  5 5425.61 (1)   450 18.45 (12) $\pi $ Gru 0.55 8.5 (1)
  12 2415.6 (3)   450 29 (14)   0.55 10.22 (9)
  12 4880 (6)   450 33.2 (16)   0.7 157.21 (1)
  25 2322.8 (3)   800 6.66 (16)   0.88 1602.43 (1)
  25 2260 (6)   811 9.8 (22)   1.25 3079.56 (2)
  60 301 (6)   850 9.45 (12)   1.25 2943.97 (1)
  60 263.2 (3)   900 9 (14)   1.65 5795.62 (2)
  100 108.9 (3)   1000 4 (17)   2.17 5812.06 (2)
  100 88.4 (6)   1100 1.85 (16)   2.2 4657.21 (1)
  450 1.09 (12)   1100 3.5 (16)   2.2 4552.7 (3)
  850 0.35 (12)   1136 3.5 (22)   3.5 2952.2 (3)
  1200 0.13 (11)   1200 1.58 (11)   4.9 1323.7 (3)
  1200 0.18 (19)   1200 3.8 (19)   12 908 (6)
  1300 0.12 (13)   1300 1.52 (18)   12 729.6 (3)
                  25 437 (6)

VY CMa

 0.55 2.1 (9) IRAS 16342-3814 1.25 0.04 (2)   25 506.2 (3)
  0.7 27.74 (10)   1.65 0.06 (2)   60 77.3 (6)
  1.25 118.6 (2)   2.17 0.1 (2)   60 86 (3)
  1.65 239.8 (2)   12 16.2 (6)   100 23.3 (6)
  2.17 510 (2)   25 200 (6)   100 40.9 (3)
  4.9 3042.78 (10)   34.6 365.6 (5)        
  12 9920 (6)   60 290 (6) AFGL 3068 2.17 0.04 (2)
  12 9278.1 (3)   100 139 (6)   12 690 (4)
  25 6650 (6)           25 736 (4)
  25 12345.5 (3) IRC +10420 1.23 10.94 (8)   60 244 (4)
  34.6 4387.5 (5)   1.25 10.38 (2)   100 72.7 (4)
  60 1450 (6)   1.65 15.58 (2)   400 3 (14)
  60 2318.4 (3)   2.15 25.52 (8)   450 1.61 (12)
  100 331 (6)   2.17 23.94 (2)   800 0.3 (15)
  100 2084.5 (3)   3.5 104.1 (3)   850 0.38 (12)
  400 10 (14)   4.35 152.1 (7)   1100 0.2 (15)
  450 9.5 (12)   4.9 179.2 (3)   1200 0.43 (19)
  800 2.81 (16)   8.28 148.7 (7)        
  780 1.99 (20)   12 1280.8 (3) AFGL 5379 1.25 0.01 (2)
  780 2.66 (20)   12 1350 (6)   1.65 0.02 (2)
  850 2.18 (20)   12.13 1292 (7)   2.17 0.04 (2)
  850 1.77 (12)   14.65 1263 (7)   4.35 158.5 (7)
  1100 0.79 (20)   21.34 2221 (7)   8.28 173.8 (7)
  1100 0.92 (20)   25 2911.5 (3)   12 1260 (4)
  1100 0.83 (16)   25 2310 (6)   12.13 1318 (7)
  1200 0.34 (11)   60 718 (6)   14.65 1204 (7)
  1200 0.69 (19)   60 566.9 (3)   21.34 1679 (7)
  1250 0.79 (20)   100 186 (6)   25 2720 (4)
  1250 0.58 (20)   450 0.95 (12)   60 1360 (4)
  1300 0.38 (13)   850 0.31 (12)   100 406 (4)
  1840 0.42 (20)   1200 0.5 (19)        
  1840 0.27 (20)   1300 0.1 (13)        

References. (1)  UBVRIJKLMNH Photoelectric Catalogue (Morel+ 1978); (2) 2MASS catalogue (Cutri+ 2003); (3) COBE DIRBE point source catalogue (Smith+ 2004); (4) IRAS faint source catalogue, version 2.0 (Moshir+ 1989); (5) The 35 um absorption line towards 1612 MHz masers (He+ 2005); (6) IRAS catalogue of point sources, version 2.0 (IPAC 1986); (7) MSX6C Infrared point source catalogue (Egan+ 2003); (8) DENIS photometry of bright southern stars (Kimeswenger+ 2004); (9) The Hipparcos and Tycho catalogues (ESA 1997); (10) Catalogue of late type stars with maser emission (Engels 1979); (11) Radio emission from stars at 250 GHz (Altenhoff+ 1994); (12) Submillimeter continuum SCUBA detections (Di Francesco+ 2008); (13) Walmsley et al. (1991); (14) Sopka et al. (1985); (15) Groenewegen et al. (1993); (16) Marshall et al. (1992); (17) Campbell et al. (1976); (18) Groenewegen (1997), Groenewegen et al. (1997); (19) Dehaes et al. (2007); (20) Knapp et al. (1993); (21) Le Bertre (1987); (22) Phillips et al. (1982).


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