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recipe_scipost_raman Overview

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Attribute nameAttribute typeDocstringUnit
crsigmafloatSigma level clipping for cube-based CR rejection (using "median", see muse_scipost). It can be switched off, by passing zero or a negative value.
fractionfloatFraction of the image (without the ignored part) to be considered as sky. If an input sky mask is provided, the fraction is applied to the regions within the mask. If the whole sky mask should be used, set this parameter to 1.
ignorefloatLowest fraction of the image to be ignored. If an input sky mask is provided, the fraction is applied to the regions within the mask. If the whole sky mask should be used, set this parameter to 0.
lambdamaxfloatCut off the data above this wavelength after loading the pixel table(s).
lambdaminfloatCut off the data below this wavelength after loading the pixel table(s).
lambdareffloatReference wavelength used for correction of differential atmospheric refraction. The R-band (peak wavelength ~7000 Angstrom) that is usually used for guiding, is close to the central wavelength of MUSE, so a value of 7000.0 Angstrom should be used if nothing else is known. A value less than zero switches DAR correction off.
object_idoidtypeThe object identifier

The object identifier is an attribute shared by all persistent
instances. It is the prime key, by which object identity is established
recipe_versionintVersion of the recipe
widthfloatWavelength range around Raman lines [Angstrom].

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