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We simulate the response of a Storage Ring Gravitational-wave Observatory(SRGO) to astrophysical gravitational waves (GWs), numerically obtaining itssensitivity curve, parameter degeneracies, and optimal choices of somecontrollable experiment parameters. We also generate synthetic noisy GW dataand use Markov Chain Monte Carlo (MCMC) methods to perform parameter estimationof the source properties. With this, we show that a single SRGO couldpotentially localize the GW source in the sky using Earth's rotation. Then, westudy the source sky localization area, mass and distance estimation errors asfunctions of noise, data sampling rate, and observing time. Finally, wediscuss, along with its implications, the capacity of an SRGO to detect andconstrain the parameters of millihertz (mHz) GW events.

Detection of gravitational waves in circular particle accelerators II. Response analysis and parameter estimation using synthetic data