XYZ2scotopic.Rawtran

XYZ2scotopic.Rawtran.array

XYZmatrix

<code>XYZ2scotopic.Rawtran</code> approximates the scotopic luminance from XYZ values, illuminant D65, from Filip Hroch (1998).
Used in the astronomy software Rawtran.<p></p><p><code>XYZ2scotopic.Rawtran.array</code> idem, however the data type used is array.
</p>

programming

Methods for color vision deficiencies (CVD), to help understanding and mitigating issues with CVDs and to generate tests for diagnosis and interpretation.

Jose Gama

Color Vision Deficiencies

XYZ2scotopic.Rawtran function

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
<a href="http://integral.physics.muni.cz/rawtran/">http://integral.physics.muni.cz/rawtran/</a>

Source

<code>XYZ2scotopic.Rawtran</code> approximates the scotopic luminance from XYZ values, illuminant D65, from Filip Hroch (1998).
Used in the astronomy software Rawtran.

<code>XYZ2scotopic.Rawtran.array</code> idem, however the data type used is array.


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
<a href = 'http://integral.physics.muni.cz/rawtran/'>http://integral.physics.muni.cz/rawtran/</a>

XYZ2scotopic.Rawtran: Approximation of the scotopic luminance

Description

Usage

Arguments

Value

Source

References