The Committee on Radio Astronomy Frequencies (CRAF) is a committee of
the European Science Foundation (ESF).
Some details of the Kayseri radio observatory:
| geographic longitude: | 36o 17'58" |
| geographic latitude: | 38o 59'45" |
| altitude above sea level: | 1054 meter |
| diameter telescope: | 5 meter |
| minimum elevation: 10o |
Available observing mode: single dish.
Frequencies used currently1):
| Frequency band | Observing mode |
| 1330.0 - 1400.0 MHz | single dish |
| 1400.0 - 1427.0 MHz | single dish |
| 1610.6 - 1613.8 MHz | single dish |
| 1660.0 - 1670.0 MHz | single dish |
| 1718.8 - 1722.2 MHz | single dish |
| 2655.0 - 2690.0 MHz | single dish |
| 2690.0 - 2700.0 MHz | single dish |
| 3260.0 - 3267.0 MHz | single dish |
| 3332.0 - 3339.0 MHz | single dish |
| 3345.8 - 3352.5 MHz | single dish |
| 4800.0 - 4990.0 MHz | single dish |
| 4990.0 - 5000.0 MHz | single dish |
| 6650.0 - 6675.2 MHz | single dish |
| 10.6 - 10.7 GHz | single dish |
| 14.47 - 14.50 GHz | single dish |
Note: 1): frequencies used: 1-15 GHz
Research programs: galactic research (1420 MHz neutral hydrogen observations) and supernova remnants.