Multimessenger Science Reach and Analysis Method for Common Sources of
  Gravitational Waves and High-energy Neutrinos
  We present the baseline multimessenger analysis method for the joint
observations of gravitational waves (GW) and high-energy neutrinos (HEN),
together with a detailed analysis of the expected science reach of the joint
search. The analysis method combines data from GW and HEN detectors, and uses
the blue-luminosity-weighted distribution of galaxies. We derive expected
GW+HEN source rate upper limits for a wide range of source parameters covering
several emission models. Using published sensitivities of externally triggered
searches, we derive joint upper limit estimates both for the ongoing analysis
with the initial LIGO-Virgo GW detectors with the partial IceCube detector (22
strings) HEN detector and for projected results to advanced LIGO-Virgo
detectors with the completed IceCube (86 strings). We discuss the constraints
these upper limits impose on some existing GW+HEN emission models.
