Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jcrl...42...99t&link_type=abstract
J. Commun. Res. Lab., Vol. 42, No. 1, p. 99 - 107
Astronomy and Astrophysics
Astronomy
Radio Astronomy
Scientific paper
CRL's 34 m antenna at Kashima which is equipped with low noise receivers which operate from 1.5 GHz to 43 GHz, covers most of the radio astronomical bands in this frequency range. The antenna has extremely accurate surface panels and is highly efficient even on the millimeter wavelength. Many kinds of single dish observations and radio astronomical VLBI observations have been performed. Domestic VLBI experiments between the Kashima 34 m and the Nobeyama 45 m antennas are called KNIFE and are highly sensitive on the short centimeter and millimeter wavelengths. VLBI experiments between the Usuda 64 m and the Kashima 34 m antennas were called UKAI and are highly sensitive on the 2 GHz and 8 GHz bands. The paper reviews published work on radio astronomy by using data obtained from the 34 m antenna at Kashima. The results of observations of astronomical masers, extragalactic radio continuum sources, pulsars, and interplanetary scintillation (IPS) observations are presented.
Amagai Jun
Hama Shin'ichi
Hanado Yuko
Imae Masato
Iwata Takahiro
No associations
LandOfFree
Related results and activities in western Pacific VLBI network. 4. Radio astronomy with the Kashima 34 m antenna. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Related results and activities in western Pacific VLBI network. 4. Radio astronomy with the Kashima 34 m antenna., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Related results and activities in western Pacific VLBI network. 4. Radio astronomy with the Kashima 34 m antenna. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-844765