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Table 2:

Erratum for Table A.2 in Gielen et al. (2008): best-fit parameters deduced from our full spectral fitting.

N$^\circ$
Name Olivine Pyroxene Forsterite Enstatite Continuum
    small-large small-large small-large small-large  

1
EP Lyr $ 0.00_{\rm0.00}^{ 0.00}{-}0.00_{\rm0.00}^{ 0.00}$ $15.36_{\rm 9.25}^{12.96}{-}61.34_{\rm 23.01}^{10.
71}$ $14.43_{\rm 2.17}^{ 4.61}{-}0.02_{\rm0.02}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}8.85_{\rm 3.90}^{ 4.49}$ $5
3.51_{\rm 1.43}^{ 3.36}$
2 HD 131356 $ 0.00_{\rm0.00}^{ 0.00}{-}30.48_{\rm 1.44}^{ 1.50}$ $ 2.87_{\rm 1.77}^{ 1.79}{-}53.91_{\rm 2.72}^{
2.57}$ $12.06_{\rm0.62}^{ 0.65}{-}0.03_{\rm0.03}^{ 1.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.65_{\rm0.56}^{ 1.34}$ $76.34_{\rm0.24}^{ 0.30}$
3 HD 213985 $ 0.00_{\rm0.00}^{ 0.00}{-}36.08_{\rm 2.21}^{ 2.20}$ $12.58_{\rm 9.92}^{ 3.42}{-}29.27_{\rm 6.99}^{
25.84}$ $ 8.02_{\rm 1.63}^{ 1.79}{-}7.74_{\rm 4.86}^{ 3.26}$ $ 0.00_{\rm0.00}^{ 0.00}{-}6.31_{\rm 4.45}^{ 2.09}$ $76.21_{\rm 1.51}^{ 0.57}$
4 HD 52961 $ 0.00_{\rm0.00}^{ 0.00}{-}0.00_{\rm0.00}^{ 0.00}$ $70.65_{\rm 1.93}^{ 1.61}{-}0.00_{\rm0.00}^{
0.00}$ $20.84_{\rm 3.57}^{ 3.81}{-}8.40_{\rm 4.94}^{ 5.18}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.12_{\rm0.12}^{ 2.07}$ $65.66_{\rm0.62}^{ 0.57}$
5 IRAS 05208 $ 0.00_{\rm0.00}^{ 0.00}{-}9.52_{\rm 2.52}^{ 2.49}$ $33.16_{\rm 1.29}^{ 1.52}{-}0.00_{\rm0.00}^
{ 0.00}$ $25.76_{\rm 1.10}^{ 1.34}{-}0.00_{\rm0.00}^{ 0.00}$ $ 2.10_{\rm 1.67}^{ 2.13}{-}29.47_{\rm 3.27}^{ 2.80}$ $69.06_{\rm0.38}^{ 0.38}$
6 IRAS 09060 $ 0.06_{\rm0.06}^{ 1.80}{-}32.70_{\rm 4.58}^{ 4.64}$ $39.74_{\rm 2.66}^{ 3.00}{-}0.48_{\rm0.49}^
{ 4.21}$ $14.95_{\rm 1.81}^{ 1.37}{-}1.11_{\rm 1.11}^{ 2.97}$ $ 0.01_{\rm0.01}^{ 0.40}{-}10.95_{\rm 2.51}^{ 3.37}$ $72.43_{\rm 2.20}^{ 1.24}$
7 IRAS 09144 $ 0.00_{\rm0.00}^{ 0.00}{-}39.21_{\rm 4.59}^{ 2.04}$ $17.77_{\rm 2.65}^{ 1.54}{-}34.88_{\rm 3.03}^
{ 7.04}$ $ 7.99_{\rm0.63}^{ 0.75}{-}0.00_{\rm0.00}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.14_{\rm0.14}^{ 1.21}$ $72.51_{\rm0.30}^{ 0.39}$
8 IRAS 10174 $ 8.70_{\rm 3.38}^{ 4.93}{-}39.99_{\rm 6.00}^{ 4.24}$ $26.10_{\rm 3.10}^{ 2.29}{-}25.21_{\rm 3.46}^
{ 4.19}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.00_{\rm0.00}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.00_{\rm0.00}^{ 0.00}$ $31.48_{\rm0.49}^{ 0.54}$
9 IRAS 16230 $ 0.00_{\rm0.00}^{ 0.00}{-}47.54_{\rm 2.30}^{ 2.35}$ $ 0.00_{\rm0.00}^{ 0.00}{-}29.46_{\rm 2.39}^
{ 2.01}$ $18.20_{\rm0.98}^{ 0.90}{-}4.23_{\rm 1.50}^{ 1.38}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.58_{\rm0.54}^{ 1.51}$ $75.74_{\rm0.25}^{ 0.29}$
10 IRAS 17038 $ 0.00_{\rm0.00}^{ 0.00}{-}31.29_{\rm 2.85}^{ 2.25}$ $ 0.03_{\rm0.03}^{ 0.92}{-}31.02_{\rm 2.54}^
{ 4.33}$ $21.65_{\rm0.91}^{ 0.77}{-}0.00_{\rm0.00}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}16.00_{\rm 2.13}^{ 1.89}$ $81.71_{\rm0.35}^{ 0.23}$
11 IRAS 17243 $ 0.49_{\rm0.49}^{ 7.03}{-}42.74_{\rm 2.29}^{ 2.73}$ $20.13_{\rm 3.29}^{10.90}{-}14.61_{\rm 9.18}^
{ 5.25}$ $17.34_{\rm0.95}^{ 0.90}{-}0.00_{\rm0.00}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}4.69_{\rm 2.60}^{ 1.76}$ $83.22_{\rm0.29}^{ 0.41}$
12 IRAS 19125 $ 8.22_{\rm 6.32}^{ 7.72}{-}6.24_{\rm 4.96}^{ 6.47}$ $ 8.66_{\rm 4.28}^{ 8.00}{-}45.53_{\rm 20.03}^
{ 5.92}$ $ 7.98_{\rm0.74}^{ 0.98}{-}7.87_{\rm 1.22}^{ 1.34}$ $ 0.00_{\rm0.00}^{ 0.00}{-}15.50_{\rm 1.34}^{ 2.65}$ $69.72_{\rm0.44}^{ 7.00}$
13 IRAS 19157 $ 0.00_{\rm0.00}^{ 0.00}{-}63.21_{\rm 3.12}^{ 5.31}$ $ 8.43_{\rm 3.41}^{ 4.28}{-}12.05_{\rm 8.01}^
{ 6.89}$ $14.58_{\rm 1.49}^{ 1.36}{-}0.02_{\rm0.02}^{ 0.94}$ $ 0.00_{\rm0.00}^{ 0.00}{-}1.70_{\rm 1.35}^{ 2.00}$ $82.28_{\rm0.53}^{ 0.61}$
14 IRAS 20056 $ 0.45_{\rm0.45}^{ 2.96}{-}31.83_{\rm 3.94}^{ 3.62}$ $34.60_{\rm 2.66}^{ 2.35}{-}0.30_{\rm0.30}^
{ 5.33}$ $15.86_{\rm 1.10}^{ 1.04}{-}0.02_{\rm0.02}^{ 0.85}$ $ 0.00_{\rm0.00}^{ 0.00}{-}16.93_{\rm 1.77}^{ 1.80}$ $83.48_{\rm0.64}^{ 0.20}$
15 RU Cen $ 0.00_{\rm0.00}^{ 0.00}{-}27.92_{\rm 2.49}^{ 2.17}$ $ 1.24_{\rm 1.06}^{ 2.06}{-}27.81_{\rm 3.95}^{ 3.
82}$ $28.63_{\rm 1.80}^{ 1.83}{-}3.34_{\rm 2.68}^{ 2.71}$ $ 0.00_{\rm0.00}^{ 0.00}{-}11.06_{\rm 2.11}^{ 1.71}$ $8
0.62_{\rm0.76}^{ 0.34}$
16 SAO 173329 $ 0.00_{\rm0.00}^{ 0.00}{-}52.55_{\rm 2.35}^{ 1.74}$ $ 0.02_{\rm0.02}^{ 0.50}{-}28.64_{\rm 2.47}^
{ 2.15}$ $ 9.21_{\rm0.77}^{ 1.09}{-}0.02_{\rm0.02}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}9.56_{\rm 1.85}^{ 2.63}$ $82.54_{\rm0.20}^{ 0.44}$
17 ST Pup $ 0.00_{\rm0.00}^{ 0.00}{-}32.87_{\rm 1.23}^{ 1.29}$ $ 0.71_{\rm0.66}^{ 1.86}{-}51.93_{\rm 3.17}^{ 1.
79}$ $13.19_{\rm0.46}^{ 0.57}{-}0.03_{\rm0.03}^{ 0.83}$ $ 0.00_{\rm0.00}^{ 0.00}{-}1.27_{\rm0.90}^{ 1.16}$ $5
4.60_{\rm0.37}^{ 0.53}$
18 SU Gem $ 0.00_{\rm0.00}^{ 0.00}{-}58.69_{\rm 3.77}^{ 3.60}$ $ 0.70_{\rm0.69}^{ 2.88}{-}12.03_{\rm 5.11}^{ 3.
93}$ $23.41_{\rm 1.75}^{ 2.31}{-}2.30_{\rm 1.96}^{ 3.69}$ $ 0.00_{\rm0.00}^{ 0.00}{-}2.87_{\rm 2.11}^{ 3.03}$ $8
8.40_{\rm0.43}^{ 0.44}$
19 SX Cen $ 0.00_{\rm0.00}^{ 0.00}{-}48.37_{\rm 4.76}^{ 3.30}$ $ 9.19_{\rm 5.82}^{11.44}{-}23.70_{\rm 23.67}^{12.
70}$ $10.82_{\rm 1.97}^{ 3.64}{-}0.53_{\rm0.53}^{ 4.29}$ $ 0.00_{\rm0.00}^{ 0.00}{-}7.39_{\rm 3.15}^{ 4.69}$ $7
6.16_{\rm 1.16}^{ 1.50}$
20 TW Cam $ 0.00_{\rm0.00}^{ 0.00}{-}84.42_{\rm 2.04}^{ 1.81}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.00_{\rm0.00}^{ 0.00}$ $15.20_{\rm 1.73}^{ 1.47}{-}0.00_{\rm0.00}^{ 0.00}$ $ 0.00_{\rm0.00}^{ 0.00}{-}0.37_{\rm0.37}^{ 1.84}$ $9
0.63_{\rm0.18}^{ 0.15}$
21 UY CMa $ 0.00_{\rm0.00}^{ 0.00}{-}15.55_{\rm 1.96}^{ 2.31}$ $ 2.54_{\rm 2.02}^{ 2.53}{-}58.59_{\rm 3.68}^{ 3.
01}$ $16.18_{\rm 1.78}^{ 2.50}{-}4.48_{\rm 3.42}^{ 2.93}$ $ 0.00_{\rm0.00}^{ 0.00}{-}2.65_{\rm 1.43}^{ 1.53}$ $7
8.14_{\rm0.42}^{ 0.62}$

Notes. The abundances of small (2.0 $\mu $m) and large (4.0 $\mu $m) grains of the various dust species are given as fractions of the total mass, excluding the dust responsible for the continuum emission. The last column gives the continuum flux contribution, listed as a percentage of the total integrated flux over the full wavelength range.


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