Ukrainian Centre of determination of the Earth Orientation Parameters
Main astronomical observatory of the National academy of sciences of Ukraine
Radioastronomy station Simeiz of laboratory of radioastronomy
of Crimean astrophysical observatory
| LOCATION | STAFF | hardware | projects | results | observations | LINKS | NEWS | ADDRESS |
| 1. | Very Long Baseline Interferometry (VLBI) | Astrophysical and geodetical projects with the international networks. Facilities for VLBI observations at frequencies of 326, 612 MHz, 1.6, 2.3, 5.0 and 8.4 GHz are available. The observations are supported by the hydrogen mazer frequency standard CH1-70 with a stability of 10-14 over an interval from 1 to 24 hours and MK-III recorders |
| 2. | Multi-wavelength monitoring of Active Galactic Nuclei (AGN) | The station carries out the monitoring at 22 and 36 GHz frequencies with a sensitivity of 0.1 Jy for 1 sec of integration time |
| 3. | Molecular line observations at wavelengths of the order of 1 mm | Observations in molecular lines of maser sources, star forming regions and other objects have been intensively carried out since 1978 over a range from 1.6 GHz up to 100 GHz |