Benacquista and Holley-Bockelmann look at LISA confusion noise from compact WD binaries.
Fusco-Femiano et al. analyze two BeppoSAX PDS observations of A2256 and find a hard X-ray signal consistent with that seen using RXTE.
Tod Strohmayer shows that the putative compact X-ray binary RX J0806.3+1527 has a spin-down rate of 3.77+/-0.8 x10^-16 Hz/s consistent with gravitational radiation losses.
Keywords: GW, clusters
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