For each model atmosphere, we have calculated with Synspec a detailed spectrum in the optical range, from 320 nm to 1 micron. Two files are available for each model atmosphere: the detailed spectrum (*.vis.7) and the continuum spectrum (*.vis.17). With program ROTIN, spectra can readily be convolved with instrumental and rotational profiles, and/or normalized.
Each file in the tar archives (two files for each model atmosphere) is a two-column ASCII file:
- Wavelength [A]
- Eddington Flux Hl at the stellar surface [erg s-1 cm-2 A-1]
The spectra are available for 5 scaled-solar chemical compositions and 2 microturbulent velocities:
| Z / Zo | File (Vt = 2 km/s) | Z / Zo | File (Vt = 10 km/s) | |||
|---|---|---|---|---|---|---|
| 2 | BCvispec_v2.tar (345 MB) | 2 | BCvispec_v10.tar (204 MB) | |||
| 1 | BGvispec_v2.tar (342 MB) | 1 | BGvispec_v10.tar (204 MB) | |||
| 1 / 2 | BLvispec_v2.tar (340 MB) | 1 / 2 | BLvispec_v10.tar (209 MB) | |||
| 1 / 2 | BSvispec_v2.tar (340 MB) | 1 / 2 | BSvispec_v10.tar (216 MB) | |||
| 1 / 10 | BTvispec_v2.tar (339 MB) | 1 / 10 | BTvispec_v10.tar (211 MB) |
Last update: October 18, 2006