XYZ2scotopic.Rawtran: Approximation of the scotopic luminance

Description Usage Arguments Value Author(s) Source References

View source: R/CVD.R

Description

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.

Usage

1

Arguments

XYZmatrix

matrix (or array) with XYZ values

Value

Matrix (or array) with approximated scotopic luminance.

Author(s)

Jose Gama

Source

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/

References

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/


CVD documentation built on May 2, 2019, 1:58 p.m.