Collision broadening of rotational transitions in the O2A band by molecular perturbers

Experimental intensity and lineshape parameters of the oxygen A-band using frequency-stabilized cavity ring-down spectroscopy

“…Anderson and Brecha [35] determined self-broadening coefficients which were on average 7% larger than the HITRAN values. This was in agreement with the FTS measurements of Pope et al [31] who reported self and N 2 -broadening coefficients 10% larger than those of HITRAN.…”

“…56 2.20 (3) G Predoi-Cross et al [36] 2007 FTS Line param. 56 2.23 (2) V Anderson and Brecha [35] 2007 TDLAS Line strength 49 2.10 (6) V Tran et al [15] 2006 FTS Line shape 2.29 (1) V Di Stefano [34,38] 2004 Afterglow Line strength 25 V Pope et al [31] 2004 FTS Press. broadening 42 V Hill et al [33] 2003 FTS Press.…”

“…Table 1 summarizes the high-resolution spectroscopy of the O 2 A-band over the last 20 years [2,[13][14][15][24][25][26][27][28][29][30][31][32][33][34][35][36]. Brown and Plymate [13] provide a detailed summary of the work prior to 2000.…”

Rare Gas Pressure Broadening of the NO Fundamental Vibrational Band

“…The utility of this algorithm has been discussed in Refs. (12,17). With three parameters for each line plus three parameters for the instrument effects and three more for the baseline, there were potentially 96 free parameters in the fit.…”

A study of collision broadening in the O2 A-band with the noble gases using fourier transform spectroscopy

“…The majority of these studies utilized N 2 , O 2 , and ''air'' as collision partners for obvious atmospheric applications. Recently, we reported new O 2 pressure broadening coefficients, which expanded the collision space to include the molecular collision partners CO, CO 2 , and SF 6 [20]. Currently, no complete systematic study of pressure broadening in the O 2 A-band by the noble gases has appeared in the refereed literature.…”