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In the space of two months, you discovered the first four pulsars; 3, are known today. Why are pulsars interesting?

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If you jammed the population of the globe into a sewing thimble, it would weigh the same as if it was full of pulsar material. They have a lot of extreme physics going on inside them and scientists use them to test theories of relativity on a cosmic scale. How would you describe yourself as a year-old PhD student?

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JBB: I was very, very thorough, making sure I really understood how that telescope worked, and that it was working properly. You famously used the letters LGM to label your charts. Tell us about the Little Green Men. JBB: Radio telescopes pick up human-generated interference: arc welders, sparking thermostats, badly suppressed cars. I had to identify this interference and got quite used to recognising features on the chart.

So, it became LGM. How did this turn into discovering the first pulsar, which you later named CP Cambridge pulsar at 19 hours 19 minutes right ascension? I got out previous recordings from that bit of sky. I talked to my supervisor, Professor Tony Hewish, and he pointed out that it was only occupying a quarter inch of space on the charts — about one part in 10 million of all the charts I had.

He suggested I switch to a better, faster recorder. For a month it recorded nothing, and then one day, on 28 November , it came again, a string of pulses one-and-a third seconds apart. Tony was cautious.

So we checked on another radio telescope on the site. The thing was pulsing nicely on mine but as we stood by the pen recorder of this other telescope, nothing happened. It was a horrible moment.

And suddenly there it was, five minutes later because we had miscalculated when the telescope would see it. Images: the first detection of radio signals from CP was on 6 August , although the pulsed nature was not suspected at this time. The first observation of pulses was on 28 November