| Name | Alpha Leo |
| Spectral type | B8IVn |
| Exposure | 9 x 1 sec |
| Altitude | 50.7° |
| Azimuth | 157° |
| Name | Alpha CMi |
| Spectral type | F5IV-V |
| Exposure | 9 x 1 sec |
| Altitude | 43° |
| Azimuth | 207° |
| Name | Epsilon Leo |
| Spectral type | G1II |
| Exposure | 9 x 10 sec |
| Altitude | 64° |
| Azimuth | 181° |
| Name | Eta Leo
|
| Spectral type | A0Ib |
| Exposure | 9 X 10 sec |
| Altitude | 59° |
| Azimuth | 159° |
| Name | Gamma Leo |
| Spectral type | K0 |
| Exposure | 9 x 5 sec |
| Altitude | 58° |
| Azimuth | 155° |
| Name | Mu Leo |
| Spectral type | K2III |
| Exposure | 9 x 10 sec |
| Altitude | 66° |
| Azimuth | 172° |
| Name | Zeta Leo |
| Spectral type | F0III |
| Exposure | 9 x 10 sec |
| Altitude | 63° |
| Azimuth | 158° |
| Name | Alpha CMi |
| Spectral type | F5IV-V |
| Exposure | 9 x 0.5 sec |
| Altitude | 42° |
| Azimuth | 209° |
Sur cette série, deux spectres divergent de la moyenne, dont l'un trrés sensiblement
Sur les spectres bruts, il apparait que ces deux specstres sont ceux qui correspeondent aux plus mauavis acquisitions avec un signal maximal faible
