“…One explanation is that f 60 depends on biomass fuels, burning conditions (e.g., flaming or smoldering), and also chemical aging (Hennigan et al, 2011;Schneider et al, 2006;Collier et al, 2016). In addition, we also observed relatively high fractions of C x H y N + z in BBOA (4.2 %-10.2 %) and high N/C ratios (0.014-0.039), consistent with the observations of abundant nitrogen-containing organic compounds, e.g., N-heterocyclic alkaloid compounds, amines, and nitrated phenols from biomass burning (Reyes-Villegas et al, 2018b;Bottenus et al, 2018;Wang et al, 2017;Laskin et al, 2009;Desyaterik et al, 2013). Compared with SV-AMS, the BBOA spectra of CV-ACSM are overall similar (R 2 = 0.93-0.96, Fig.…”