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Table A.1

Best fit parameters deduced from our full spectral fitting.

Name T dust1 T dust2 Fraction T cont1 T cont2 Fraction
(K) (K) Tdust1 − Tdust2 (K) (K) Tcont1Tcont2

1 EPLyr
2 HD 131356
3 HD 213985
4 HD 52961
5 IRAS 05208
6 IRAS 06034
7 IRAS 06072
8 IRAS 06338
9 IRAS 09060
10 IRAS 09144
11 IRAS 09538
12 IRAS 10174
13 IRAS 11000
14 IRAS 13258
15 IRAS 15556
16 IRAS 16230
17 IRAS 17038
18 IRAS 17233
19 IRAS 17243
20 IRAS 17530
21 IRAS 18123
22 IRAS 18158
23 IRAS 19125
24 IRAS 19157
25 IRAS 20056
26 RUCen
27 SAO 173329
28 STPup
29 SUGem
30 SXCen
31 TWCam
32 UYAra
33 UYCma
34 HV 12631
35 HV 2281
36 HV 2444
37 HV 2522
38 HV 2862
39 HV 5829
40 HV 915
41 J044458.18-703522.8
42 J045242.93-704737.4
43 J050143.18-694048.7
44 J051159.11-692532.8
45 J051333.74-663419.1
46 J052220.87-655551.6
47 J053605.56-695802.9
48 J054312.52-683356.9
49 MACHO 78.6698.38
50 MACHO 82840515
51 MSX 949
52 NGC 1805SAGEIRS1
53 SAGE 050830
54 SAGE 051453
55 SAGE 052707
56 SAGE 052747
57 SAGE 054310

Notes. Listed the dust and continuum temperatures and their relative fractions.

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