XYZ2scotopic.Rawtran {CVD} | R Documentation |
XYZ2scotopic.Rawtran
approximates the scotopic luminance from XYZ values, illuminant D65, from Filip Hroch (1998).
Used in the astronomy software Rawtran.
XYZ2scotopic.Rawtran.array
idem, however the data type used is array.
XYZ2scotopic.Rawtran(XYZmatrix)
XYZmatrix |
matrix (or array) with XYZ values |
Matrix (or array) with approximated scotopic luminance.
Jose Gama
Filip Hroch, 1998, Computer Programs for CCD Photometry, 20th Stellar Conference of the Czech and Slovak Astronomical Institutes, DusekJ., http://adsabs.harvard.edu/abs/1998stel.conf...30H Rawtran - integral.physics.muni.cz Masaryk University http://integral.physics.muni.cz/rawtran/
Filip Hroch, 1998, Computer Programs for CCD Photometry, 20th Stellar Conference of the Czech and Slovak Astronomical Institutes, DusekJ., http://adsabs.harvard.edu/abs/1998stel.conf...30H Rawtran - integral.physics.muni.cz Masaryk University http://integral.physics.muni.cz/rawtran/