K$^0_{s}\pi^{\pm}$ invariant mass distribution after the uncorrelated background subtraction

Scope: PWG
PWG-LF (Light Flavour Spectra)
Energy
13 TeV
System
p-p
Figure Image
Figure image (.eps)
Figure image (.pdf)
Figure Caption

K$^0_{s}\pi^{\pm}$ invariant mass  distribution for the 1.6 $<$ $p$\textsubscript{T}  $<$ 2.0 GeV/$c$ bin in the VI V0M class (black full circles) after the uncorrelated background subtraction. The solid green curve is the result of the final fit, the dashed red line represents the residual background, while the dashed blue line is the non-relativistic Breit-Wigner function. Colored regions show the areas interested in the bin counting method.