Mid-Infrared Period$-$Luminosity Relations for Miras in the Large
  Magellanic Cloud
  We present the mid-infrared (mid-IR) period$-$luminosity relations (PLRs)
using over 1000 Mira variables in the Large Magellanic Cloud (LMC), for the
four Wide-Field Infrared Survey Explorer (WISE) and the four Spitzer bands.
These PLRs cover a mid-IR wavelength range from $3.4$ $\mu$m to $22$ $\mu$m and
are presented separately for the oxygen-rich (O-rich) and carbon-rich (C-rich)
Miras. These relations can be used to measure distances to individual O-rich
and/or C-rich Mira stars with the accuracy of $5\%$ and $12\%$, respectively.
They are the most accurate Mira PLRs in the mid-IR to date.
