A search for periodic gravitational waves from three recycled pulsars using the AURIGA detector - An implementation of a modified version of the unified approach method

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Table 1:

$\nu _0$ is the spin frequency of the targeted MSPs at the time of the AURIGA run, whereas $\nu _{\rm gw} {\rm [Hz]}$ is the frequency of the GW signal we searched for.
Name	$\nu _0$ [Hz]	$\nu_{\rm gw}$ [Hz]
PSR J0024-7204J	476.0468584406(...)	952.0937168812(...)
PSR J0218+4232	430.4610663457(...)	860.9221326914(...)
PSR J1939+2134	641.9282611068(...)	855.9043481424(...)

Notice that, for the third source, we are looking for the r-mode emission channel.

Source LaTeX | All tables | In the text

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