The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. We perform two directional searches for persistent GWs using data from the LIGO S5 science run: one optimized for pointlike sources and one for arbitrary extended sources. Finding no evidence to support the detection of GWs, we present 90% confidence level (C.L.) upper-limit maps of GW strain power with typical values between $2-20\times {10}^{-50}{\mathrm{strain}}^2{\mathrm{Hz}}^{-1}$ and $5-35\times {10}^{-49}{\mathrm{strain}}^2{\mathrm{Hz}}^{-1}{\mathrm{sr}}^{-1}$ for pointlike and extended sources, respectively. The latter result is the first of its kind. We also set 90% C.L. limits on the narrow-band root-mean-square GW strain from interesting targets including Sco X-1, SN 1987A and the Galactic center as low as $\approx 7\times {10}^{-25}$ in the most sensitive frequency range near 160 Hz.

• Received 9 October 2011

DOI:https://doi.org/10.1103/PhysRevLett.107.271102