Galaxies | Free Full-Text | Features of Secular Changes in the Flux Density of the Cas a Supernova Remnant, from Centimeter to Decameter Wavelengths | HTML
Basic concepts of radio interferometric VLBI observations Hiroshi
Radio Astronomy
Radio Telescope Front & Backend Systems Lecture 3 by Mike Garett (2013) | Sampling (Signal Processing) | Detector (Radio)
Irbene RT-32
Station Amplitude Calibration: Why we need it and how to do it
BROADBAND RECEIVING SYSTEMS FOR 4.5 – 8.8 GHZ RADIO ASTRONOMICAL OBSERVATIONS AT IRBENE RADIO TELESCOPES RT-32 AND RT-16
nsurumqi
Tian Ma 65-m Radio Telescope
ZHENG Weimin
Untitled
Spectroscopy with TianMa 65m and also FAST - ppt download
Station Amplitude Calibration: Why we need it and how to do it
Basic concepts of radio interferometric (VLBI) observations Hiroshi Imai Department of Physics and Astronomy Graduate School of Science and Engineering. - ppt download
Basic concepts of radio interferometric VLBI observations Hiroshi
Single-dish Spectroscopy and Science with TianMa 65m
