Pulsars and neutron stars/Telescopes involved in pulsar research

Introduction edit

Radio telescopes edit

Observatory setup edit

In this section we describe the Parkes observatory in detail.

Receivers edit

Backend instruments edit

Observatory time standard edit

The maser system at Parkes does not produce a signal such as a 1 second tick. Instead it produces an accurate 5 MHz waveform. This waveform is read by the clock system (known as the Australia Telescope Distributed Clock, ATDC). The actual day, month and year of that clock are set manually when the clock is started and continually updated with IERSA data.

Calibration edit

Arecibo edit

Effelsberg edit

FAST edit

GMRT edit

Green Bank edit

Jodrell Bank edit

Lofar edit

Molonglo edit

MWA edit

Nancay edit

Nanshan edit

Parkes edit

Qitai edit

Sardinia edit

Westerbork edit

X-ray telescopes edit

Gamma-ray telescopes edit

Optical telescopes edit