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Table 3
Spectral configurations used with VEGA and MIRC for the ϕ Persei observations.
| λ nm | Δλ nm | Channels | |
|
|
|||
| VEGA | [483; 498] | 15 | 1 |
| [636; 651] | 15 | 1 | |
| [648; 663] | 15 | 1 | |
| [663; 678] | 15 | 1 | |
|
|
|||
| VEGA | [646; 666] | 0.1 | 200 |
|
|
|||
| MIRC | [1501; 1712] | 35 | 6 |
Notes. Column 2 gives the spectral band, Col. 3 the spectral width of one channel, and Col. 4 the number of channels.
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