  The Fermilab Muon $g-2$ collaboration recently announced the first result of
measurement of the muon anomalous magnetic moment ($g-2$), which confirmed the
previous result at the Brookhaven National Laboratory and thus the discrepancy
with its Standard Model prediction. We revisit low-scale supersymmetric models
that are naturally capable to solve the muon $g-2$ anomaly, focusing on two
distinct scenarios: chargino-contribution dominated and pure-bino-contribution
dominated scenarios. It is shown that the slepton pair-production searches have
excluded broad parameter spaces for both two scenarios, but they are not closed
yet. For the chargino-dominated scenario, the models with $m_{\tilde{\mu}_{\rm
L}}\gtrsim m_{\tilde{\chi}^{\pm}_1}$ are still widely allowed. For the
bino-dominated scenario, we find that, although slightly non-trivial, the
region with low $\tan \beta$ with heavy higgsinos is preferred. In the case of
universal slepton masses, the low mass regions with $m_{\tilde{\mu}}\lesssim
230$ GeV can explain the $g-2$ anomaly while satisfying the LHC constraints.
Furthermore, we checked that the stau-bino coannihilation works properly to
realize the bino thermal relic dark matter. We also investigate heavy staus
case for the bino-dominated scenario, where the parameter region that can
explain the muon $g-2$ anomaly is stretched to $m_{\tilde{\mu}}\lesssim 1.3$
TeV.
