The LVM-DAP recovers gas emission-line fluxes and kinematics with claimed survey-grade accuracy, but its stellar parameter estimates are reliable only for single stars and biased for mixed stellar populations.
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The SDSS-V Local Volume Mapper (LVM): Data Analysis Pipeline
The LVM-DAP recovers gas emission-line fluxes and kinematics with claimed survey-grade accuracy, but its stellar parameter estimates are reliable only for single stars and biased for mixed stellar populations.