  The precise measurements of energy spectra and anisotropy could help us
uncover the local cosmic-ray accelerators. Our recent works have shown that
spectral hardening above $200$ GeV in the energy spectra and transition of
large-scale anisotropy at $\sim 100$ TeV are of local source origin. Less than
$100$ TeV, both spectral hardening and anisotropy explicitly indicate the
dominant contribution from nearby sources. In this work, we further investigate
the parameter space of sources allowed by the observational energy spectra and
anisotropy amplitude. To obtain the best-fit source parameters, a numerical
package to compute the parameter posterior distributions based on Bayesian
inference, which is applied to perform an elaborate scan of parameter space. We
find that by combining the energy spectra and anisotropy data, the permissible
range of location and age of local source is considerably reduced. When
comparing with the current local SNR catalog, only Geminga SNR could be the
proper candidate of the local cosmic-ray source.

High Energy Astrophysical Phenomena