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Taurus A is the radio source in Taurus constellation that corresponds to the Crab Nebula (M1), the supernova remnant exploded on July 4, 1054 and noted by Chinese and Arabian astronomers of the time. Since then, the gas cloud has expanded and today is over 6 light years large. In this article we see how the SPIDER radio telescope "discovered" it by capturing the radio waves emitted by Taurus A and converting them into a radio map, a real photograph in radio waves of this nebula. In fact it is believed that Taurus A emits radio waves for synchrotron radiation caused by electrons in fast spiral motions around magnetic field lines generated by the pulsar inside it. Thanks to the large antenna and the 1420 MHz H142-One receiver, the SPIDER radio telescope was able to easily record the weak signal and, thanks to the precise mount and pointing system, it generated a radio map with the same technique used by professional radio telescopes.
Cassiopeia A is a very important supernova remnant for radio astronomy since it's the brightest extrasolar radio source in the sky when studying at frequencies above 1 GHz. This feature makes it a conquest within the reach of radio telescopes equipped with not huge antennas, but it is still a relatively weak radio source. In fact, having a flux of around 2400 Jansky at a frequency of 1,42 GHz, it's a lot weaker than the Sun that is around 40000 Jansky! In this article we will see how to use SPIDER radio telescope and its RadioUniversePRO software to record the signal from Cassiopea A by aligning the antenna, removing the artificial signals and recording transists, spectra and radio maps.
Solar radio emission can be studied by using SPIDER radio telescopes. The Sun is in fact one of the most interesting radio source in the sky. In fact the Sun not only emits visible light but also other frequencies in the electromagnetic spectrum. For example, everyone can feel the Sun heat on our skin, expression of infrared radiation. In this article, with step-by-step guide, we see how the SPIDER radio telescopes detect radio waves coming from the Sun and we show how to generate transits, radio images and spectra by using the RadioUniversePRO control software. We perform automatic pointing and tracking on the Sun, detection and removal of eventual artificial signal and capture of different results.