Table 2: Infrared flux densities of GRS 1915+105. $F_{\rm obs}$ is the observed flux directly measured on ISOCAM images, except for the J, H and K band fluxes which were reported from Mahoney et al. (1997) and transformed into mJy units. $F_{\rm der}$ is the resulting flux after dereddening with two different laws: from Lutz et al. (1996) and from Draine (1989).
Filter $F_{\rm obs}$ (mJy) $F_{\rm der}$ Lutz (mJy)   $F_{\rm der}$ Draine (mJy)   
  1996  1997 1996  1997 1996  1997
LW1 (4-5 $\mu $m) $11.2\pm 3.4$    $42.1\pm 13$    $19.2\pm 5.8$   
LW2 (5-8.5 $\mu $m) $5.39\pm 1.6$   $9.77\pm 2.9$ $17.4\pm 5.2$   $31.5\pm 14$ $7.72\pm 2.3$   $14.0\pm 4.2$
LW4 (5.5-6.5 $\mu $m)     $11.6\pm 3.5$     $37.1\pm 11$     $16.0\pm 4.8$
LW6 (7-8.5 $\mu $m)     $11.9\pm 3.6$     $38.4\pm 12$     $19.5\pm 5.9$
LW7 (8.5-10.7 $\mu $m) $1.53\pm 0.5$   $4.87\pm 1.5$ $7.37\pm 2.2$   $23.5\pm 7.0$ $7.26\pm 2.2$   $23.1\pm 6.9$
LW8 (10.7-12 $\mu $m) $3.54\pm 1.1$   $6.58\pm 2.0$ $10.3\pm 3.1$   $19.2\pm 5.8$ $10.8\pm 3.2$   $20.1\pm 6.0$
LW9 (14-16 $\mu $m)     $13.8\pm 4.1$     $23.9\pm 7.2$     $24.0\pm 7.2$
LW3 (12-18 $\mu $m) $5.34\pm 1.6$   $10.5\pm 3.1$ $9.25\pm 2.8$   $18.2\pm 5.5$ $9.29\pm 2.8$   $18.3\pm 5.5$
LW10 (8-15 $\mu $m)     $14.7\pm 4.4$     $41.3\pm 12$     $36.0\pm 11$
J (1.25 $\pm$ 0.15 $\mu $m) $0.688\pm 0.04$    $121.0\pm 7.8$    $135.2\pm 8.7$   
H (1.65 $\pm$ 0.15 $\mu $m) $3.14\pm 0.14$    $78.3\pm 3.6$    $77.1\pm 3.6$   
$K_{\rm s}$ (2.15 $\pm$ 0.15 $\mu $m) $6.98\pm 0.26$    $52.7\pm 1.9$    $51.8\pm 1.9$   


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