We present the mid-infrared (mid-IR) period-luminosity relations (PLRs) using over 1000 Mira variables in the Large Magellanic Cloud, for the four Wide-field Infrared Survey Explorer and the four Spitzer bands. These PLRs cover a mid-IR wavelength range from 3.4-22{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 an accuracy of 5% and 12%, respectively. They are the most accurate Mira PLRs in the mid-IR to date.

Cone search capability for table J/ApJ/919/99/table3 (Basic parameters for 1663 LMC Miras from the Soszynski+ (2009, J/AcA/59/239) catalog, supplemented with improved pulsation periods and mean magnitudes with uncertainties for all WISE and Spitzer bands)