For each model atmosphere, we have calculated with Synspec a detailed spectrum in the UV range, from 90 to 320 nm. Two files are available for each model atmosphere: the detailed spectrum (*.uv.7) and the continuum spectrum (*.uv.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 | BCuvspec_v2.tar (486 MB) | 2 | BCuvspec_v10.tar (212 MB) | |||
| 1 | BGuvspec_v2.tar (444 MB) | 1 | BGuvspec_v10.tar (208 MB) | |||
| 1 / 2 | BLuvspec_v2.tar (408 MB) | 1 / 2 | BLuvspec_v10.tar (209 MB) | |||
| 1 / 2 | BSuvspec_v2.tar (370 MB) | 1 / 2 | BSuvspec_v10.tar (209 MB) | |||
| 1 / 10 | BTuvspec_v2.tar (346 MB) | 1 / 10 | BTuvspec_v10.tar (200 MB) |
Last update: October 18, 2006