Compute the spectral distribution for a black body

spectralDistribution(x, measure = "nanometer")

Arguments

x

Numeric vector. Wavelength values. Values are interpreted in nanometers when measure = "nanometer" and in micrometers when measure = "micrometer".

measure

Character. Unit used for the wavelength scale and returned spectral density. One of "nanometer" or "micrometer".

Value

A numeric vector of spectral density values.

Examples

spectralDistribution(c(500, 600))
#> [1] 0 0
spectralDistribution(c(0.5, 0.6), measure = "micrometer")
#> [1] 0 0