Table 1
BCD standard stars observed with the INT and NOT telescopes.
| Name | Telescope | Sp/LCMK | Sp/LCBCD | λ1(Å) | D(dex) | Δλ(Å) | Disp.(Å/pix) | G(Å) |
|
|
||||||||
| HR 533 | INT | B2 V | B2 V | 65 | 0.144 | 4 | 1.85 | 4.8 |
| HR 1122 | NOT | B5 III | B5-6 III | 42 | 0.286 | 2 | 0.72 | 3.5 |
| HR 2347 | NOT | B9 V | B9 V | 64 | 0.422 | 2 | 0.72 | 3.5 |
| HR 2461 | INT | B8 III | B7 III | 41 | 0.340 | 3 | 1.40 | 4.0 |
Notes.Columns 4−6 are the standard BCD spectral type and D and λ1 parameters respectively, from Zorec & Briot (1991). The different Δλ and dispersion values for the two stars observed at the INT are due to different instrumental configurations. The last column lists the width of the Gaussian filter used to reproduce the standard BCD parameters from each spectra.
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