Jansky

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For other uses, see Jansky (disambiguation).

In radio astronomy, the flux unit or jansky (symbol Jy) is a non-SI unit of electromagnetic flux equivalent to 10−26 watts per square metre per hertz. The unit is named after the pioneering radio astronomer Karl Jansky.

The brightest natural radio sources have flux densities of the order of one to one hundred janskys, which makes the jansky a suitable unit for radio astronomy.

For example the Third Cambridge Catalogue (3C) which was prepared in 1959 and revised in 1962, lists some 300 to 400 radio sources in the Northern Hemisphere brighter than 9 Jy at 159 MHz.

1 \ \mathrm{ Jy} = 10^{-26} \frac{ \mathrm{W} }{ \mathrm{m^2 } \cdot \mathrm{ Hz} } (SI)

1 \ \mathrm{ Jy} = 10^{-23} \frac{\mathrm{erg}}{ \mathrm{sec} \cdot \mathrm{ cm^{2}} \cdot \mathrm{ Hz}} (cgs)

The flux density in Jy can be converted to a magnitude basis, for suitable assumptions about the spectrum. For instance, converting an AB magnitude to a flux-density in microjanskys is straightforward:[1]

F_v \ [\mathrm{\mu Jy}] = 10^{29} \cdot 10^{-\frac{AB+48.6}{2.5}}


Here is a list of pulsars detected by the Second Cambridge Survey where the pulsar strengths are given in mJy at two different radio frequencies.

[edit] References

  1. ^ M. Fukugita (1995). "Galaxy Colors in Various Photometric Band Systems". PASP 107: 945-958. 
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