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Table 1
Objects, their derived spectral types, and the number of observations at each slit width to test the method and obtain the statistical scatter and the mean measured D⋆ and λ1 values.
| Star | Sp Type | N of observations/slit | D ⋆ | λ1-3700 | |||||
| 0.5″ | 0.8″ | 1.0″ | 1.3″ | 1.6″ | 5.0″ | dex | Å | ||
|
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| HD 130163 | A1V | – | – | 38 | 5 | 6 | 1 | 0.545 ± 0.006 | 63.65 ± 0.97 |
| HD 190285 | A1V | 14 | 8 | 15 | 1 | 5 | – | 0.565 ± 0.013 | 68.16 ± 1.1 |
| HIP 1115 | B3IV | – | 2 | 2 | – | 5 | 2 | 0.253 ± 0.006 | 45.65 ± 2.0 |
| HIP 32474 | A0IIIe | 1 | – | 7 | – | 2 | – | 0.522 ± 0.01 | 44.525 ± 3.5 |
| HIP 39483 | B4IIIe | – | 3 | 5 | 1 | 1 | – | 0.281 ± 0.008 | 34.44 ± 1.0 |
| HIP 52977 | B4IIIe | 7 | – | 5 | 8 | 1 | – | 0.263 ± 0.017 | 34.44 ± 3.04 |
| HIP 71974 | A0IIIe | 5 | – | 5 | 1 | 2 | – | 0.522 ± 0.007 | 47.89 ± 1.1 |
| HIP 85138 | B7IIIe | 6 | – | 4 | – | 3 | – | 0.393 ± 0.011 | 34.44 ± 2.4 |
| HIP 85195 | B9IIIe | 5 | – | 16 | 3 | 6 | – | 0.479 ± 0.007 | 38.92 ± 1.1 |
| HIP 88374 | B9IVe | 1 | 2 | 10 | 2 | 2 | 2 | 0.443 ± 0.006 | 44.52 ± 2.07 |
| HIP 89486 | A0IIIe | 4 | – | 6 | – | 4 | – | 0.512 ± 0.01 | 41.16 ± 0.88 |
| HIP 94986 | B4IIIe | 8 | 5 | 7 | 1 | 5 | – | 0.278 ± 0.02 | 36.68 ± 3.52 |
| Hip104508 | B7IIIe | – | 6 | 14 | – | 1 | – | 0.431 ± 0.014 | 36.68 ± 2.95 |
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