The following sequence of image and spectra shows a representative Be star, Omega Orionis. Note the broad, double-peaked H-Alpha emission line in the high- resolution spectrum.
| Object | Omega Orionis (SAO 113001) |
| Telescope | 14" Meade RCX400 at f/8 |
| Spectrograph / CCD | SBIG SGS, SBIG ST-7XME at -30C; Low Resolution = 150 lines/mm grating, High Resolution = 600 lines/mm |
| Integration Details | Low Resolution: 5 x 180s; High Resolution: 5 x 600s, dark subtracted and median combined |
| Date / Time (UTC) | Low Resolution: 05-Jan-2007 0530 UTC; High Resolution: 08-Jan-2007 0540 UTC |
| Moon Phase | 97% (Low) & 79% (High) |
| Approximate Airmass | 1.14 |
| CCD Response Curve Source | Epsilon Orionis |
| Wavelength Calibration | H and Ne lamps |
| Software Used | CCDSoft, CCDStack, Iris, vSpec, Excel, Adobe Photoshop |
| Comments | The image was taken on 08-Jan-2007 using a 105mm apochromatic refractor at f/5.6, with an ST-10XME and an Astrodon H-Alpha filter with a 60 Angstrom FWHM bandpass. 9 x 10 minutes at -30C, dark subtracted, flat fielded, mean combined. |