A fuller description of the processing steps is contained in Morganson et al. 2018.
Please note that the internal format of some of these files is not fully documented here, but mechanisms to read the contents of these files may be found embedded in the associated codes in the github repositories and elsewhere.
Please note that when a set of calibration file has separate entries by ccdnum and/or by filter, that only one ccdnum and/or filter sample element file is included here.
The set of sample cal/config of files included:
Brighter-fatter deconvolution matrix:
http://data.darkenergysurvey.org/aux/sample/cal/bf/20170407-r2959/p01/D_n20170406_r2959p01_bf.fits
Bad pixel map (ccdnum=1 only)
Non-linearity correction table for each ccdnum/amp:
http://data.darkenergysurvey.org/aux/sample/cal/lintable/lin_tbl_v0.7.fits
Binned-full-focal-plane r-band (only) sky template correction map, co-efficents:
Full (unbinned) sky template PCA (4-component) correction map (ccdnum=1, r-band only):
Skyflat (low-frequency multiplicitive response correction map, g-band, ccdnum=1):
Crosstalk amp-to-amp, ccd-to-ccd correction coefficients:
http://data.darkenergysurvey.org/aux/sample/cal/xtalk/20130606/DECam_20130606.xtalk
TPV WCS astrometric chip position/rotation/scale/cubic coefficients (i-band):
Updates to SISPI (DAQ) default ccd readnoise, fullwell, gains for select chips:
Dome flat (Y-band ccdnum=1 only):
Bias image (ccdnum=1 only):
Supercal bias (average of 10-30 precal bias images, ccdnum=1):
Supercal dome flat (average of 10-30 precal dome flat images, ccdnum=1, z-band):