“…6a, the spectral ringing along most of the spectrum occurs as a consequence of the infinite interferogram length, which can be attenuated by the apodization function [29]. The observed spectral features are characteristic for the emission of MMA [9]. As summarized in Table 1, we can identify in the LWIR, combination of CeH and CeOeC deformation at 811 cm À1 , out of plane bending peaks for ¼ CH at 938 and 1015 cm À1 , CeO stretching at 1159 and 1202 cm À1 , CH 3 -bending peaks at 1308 and 1446 cm À1 , a C]C stretching peak at~1632 cm À1 , a C]O stretching peak at 1737 cm À1 , and atmospheric H 2 O absorption overlapping with the C]C and C]O stretching peaks from~1330 to 1800 cm À1 .…”