Lightining-fast continuum fitting
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QSOnic is an MPI-parallelized, highly optimized quasar continuum fitting package for DESI built on the same algorithm as picca <https://github.com/igmhub/picca>
_, but faster. It also provides an efficient API to read DESI quasar spectra. If you use this software, please cite the article in the Journal of Open Source Software (JOSS).
--var-fit-eta
. A covariance matrix is calculated based on delete-one Jackknife over subsamples between var_pipe and var_obs data points, and used in var_lss, eta fitting if --var-use-cov
passed (soft recommendation to always enable this).IVAR
, and output WEIGHT
is based on this smoothed ivar. This smoothing can be turned off.CONT
column is mean flux times continuum even when fiducial mean flux is passed.MEANSNR
in header file and chi2 catalog is average of flux times square root of positive ivar values. Header values are per arm, but catalog values are the average over all arms.IVAR
output. Pipeline noise will be modified with explicit calibration option.