Committee on Radio Astronomy Frequencies

 The Committee on Radio Astronomy Frequencies (CRAF) is a committee of the European Science Foundation (ESF).


Radio astronomy in Italy:


Some details of the Medicina radio observatory (operated by the Bologna Istituto di Radioastronomia):

geographic longitude:11o 38'49"
geographic latitude:44o 31'14"
altitude above sea level:28 meter
diameter telescope:32 meter
minimum elevation: 5o
diameter telescope (Northern Cross):600 (EW) x 34 (NS) meter
minimum elevation: 15o
Note: the Northern Cross is a transit instrument and has an azimuth range of +/-3o only

Available observing mode: single dish, local interferometry, Very Long Baseline Interferometry (VLBI).

Frequencies used currently:
Frequency bandObserving mode
322.0 -328.6 MHzsingle dish, VLBI
406.1 - 410.0 MHzsingle dish
608.0 - 614.0 GHzsingle dish, VLBI
1330.0 - 1400.0 MHzsingle dish, VLBI
1400.0 - 1427.0 MHzsingle dish, VLBI
1610.6 - 1613.8 MHzsingle dish
1660.0 - 1670.0 MHzsingle dish, VLBI
1718.8 - 1722.2 MHzsingle dish
2290.0 - 2300.0 MHzsingle dish, VLBI
4800.0 - 4990.0 MHzsingle dish, VLBI
4990.0 - 5000.0 MHzsingle dish, VLBI
8387.0 - 8443.0 MHzsingle dish, VLBI
10.6 - 10.7 GHzsingle dish
15.35 - 15.40 GHzsingle dish
22.01 - 22.21 GHzsingle dish
22.21 - 22.50 GHzsingle dish, VLBI
22.81 - 22.86 GHzsingle dish
23.07 - 23.12 GHz GHzsingle dish
23.6 - 24.0 GHzsingle dish
42.5 - 43.5 GHzsingle dish, VLBI

Research programs: Very Long Baseline Interferometry: astronomy and geodesy, pulsar research and pulsar searches, at 22 GHz observations of H2O masers, molecular spectroscopy, receiver development.


Last modified: April 19, 2007