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Table 1
Objects used for detailed tests.
| #a | Object | Median counts | Slit | Prog.-ID |
| type | [ADU] | [″×″] | ||
|
|
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| 1 | Seyfert 2 | 462 | 1.5 × 11 | 087.B-0614 |
| 2 | GRB | 241 | 0.9 × 11b | 091.C-0934 |
|
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| 3 | B[e] star | 7684 | 0.4 × 11 | 084.C-0952 |
| 4 | E0 galaxy | 5236 | 0.9 × 11 | 384.B-1029 |
| 5 | Carbon star | 50587 | 0.9 × 11 | 084.D-0117 |
| 6 | PN | 6214 | 0.4 × 11 | 385.C-0720 |
Notes.
(a)
Objects #1 and #2 are data with low S/N used for tests on the reliability of molecfit when applied to such data. #3 through #6 are used for a detailed comparison with the classical method.
(b)
Observed with the K band blocking filter (Vernet et al. 2011).
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