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The galactic binary GW noisewill be modulated by the LISA orbital motion,
whereas the extragalactic one will not.If the latter is comparable with galactic
values at some galactic latitudes, it can impede detection by LISA of some inter­
esting relic cosmological GW backgrounds, and specific statistical features of the
relic GW should be used to separate them against the noise from astrophysical
sources.
The galactic binary GW noisewill be modulated by the LISA orbital motion,
whereas the extragalactic one will not. If the latter is comparable with galactic
values at some galactic latitudes, it can impede detection by LISA of some inter­
esting relic cosmological GW backgrounds, and specific statistical features of the
relic GW should be used to separate them against the noise from astrophysical
sources.
Just crossing out text out, X out.
The galactic binary GW noisewill be modulated by the LISA orbital mo­
tion, whereas the extragalactic one will not. If the latter is comparable with
galactic values at some galactic latitudes, it can impede detection by LISA of
some interesting relic cosmological GW backgrounds, and specific statistical
features of the relic GW should be used to separate them against the noise from
astrophysical sources.
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