Extended Data Table 1 The MIR AB magnitudes of SN 2018evt, and the parameters describe the newly-formed dust

From: Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt

  1. The CH1 and CH2 magnitudes were measured from the images taken by the Infrared Array Camera (without host subtraction) and the host-subtracted W 1 and W 2 magnitudes were measured from the observations by the NEOWISE reactivation mission. The presented parameters are deduced for a = 0.3 μm, and a = 0.05 μm graphite and silicate dust grains.
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