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Radio Astronomy
Radio Astronomy

An ultra-wide bandwidth (704 to 4 032 MHz) receiver for the Parkes radio telescope | Publications of the Astronomical Society of Australia | Cambridge Core
An ultra-wide bandwidth (704 to 4 032 MHz) receiver for the Parkes radio telescope | Publications of the Astronomical Society of Australia | Cambridge Core

Radio Astronomy
Radio Astronomy

An ultra-wide bandwidth (704 to 4 032 MHz) receiver for the Parkes radio telescope | Publications of the Astronomical Society of Australia | Cambridge Core
An ultra-wide bandwidth (704 to 4 032 MHz) receiver for the Parkes radio telescope | Publications of the Astronomical Society of Australia | Cambridge Core

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

Radio Astronomy
Radio Astronomy

Radio Astronomy
Radio Astronomy

Yebes CX-band receiver
Yebes CX-band receiver

Poonam Chandra National Centre for Radio Astronomy
Poonam Chandra National Centre for Radio Astronomy

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

Radio Astronomy
Radio Astronomy

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

Tian Ma 65-m Radio Telescope
Tian Ma 65-m Radio Telescope

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

PDF) Performance Evaluation of Irbene RT-16 Radio Telescope Receiving System
PDF) Performance Evaluation of Irbene RT-16 Radio Telescope Receiving System

Radio Astronomy
Radio Astronomy

Radio Astronomy
Radio Astronomy

Tian Ma 65-m Radio Telescope
Tian Ma 65-m Radio Telescope

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Untitled

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

Untitled
Untitled

PDF] An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope
PDF] An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope

Galaxies | Free Full-Text | Features of Secular Changes in the Flux Density of the Cas a Supernova Remnant, from Centimeter to Decameter Wavelengths | HTML
Galaxies | Free Full-Text | Features of Secular Changes in the Flux Density of the Cas a Supernova Remnant, from Centimeter to Decameter Wavelengths | HTML

VLA Test Memorandum No. 164 GAIN CURVES FOR 1.3CM VLBI WITH A SINGLE VLA ANTENNA J.M. Wrobel National Radio Astronomy Observator
VLA Test Memorandum No. 164 GAIN CURVES FOR 1.3CM VLBI WITH A SINGLE VLA ANTENNA J.M. Wrobel National Radio Astronomy Observator

Radio Astronomy
Radio Astronomy

Untitled
Untitled

Radio Astronomy
Radio Astronomy

Station Amplitude Calibration: Why we need it and how to do it
Station Amplitude Calibration: Why we need it and how to do it

Radio Astronomy
Radio Astronomy

Radio Astronomy
Radio Astronomy