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Create a master bias from set of raw bias frames.
Create a master dark from set of raw dark frames.
Determine ron, gain, and bad pixels from a set of flat field exposures.
Generate ifu calibrations from a set of flat and arc lamp exposures.
Combine partial ifu field-of-views reconstructed by vmifuscience from different quadrants.
Rearrange into cube format images of extracted spectraproduced by vmifucalib, vmifuscience, and vmifustandard.
Extract spectra from an ifu scientific exposure.
Extract a standard star spectrum.
Determine photometric calibration from a set of observed standard stars.
Create a master screen flat field from set of raw screen flat field frames.
Create a master sky flat field from set of raw sky flat field frames.
Reduce and combine a set of jittered imaging exposures.
Reduce an imaging science exposure.
Reduce a preimaging science exposure.
Reduce an imaging standard star exposure.
Determination of the extraction mask
Combine reduced mos observations from different obs.
Reduce and combine a set of jittered mos observations.
Reduce a mos science exposure.
Extraction of scientific spectra
Reduce a mos standard star exposure.
Determine spectral distortion models from flat field and arc lamp exposure.
Build master flat field from a set of raw mos flat fields.
Apply to ifu or mos 1d-extracted spectra a flux correction.