Luminosity Density

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Description

Calculate the luminosity density from a given set of input (Schechter) luminosity function inputs.

Usage

1
lumdens(knee, slope, norm, msun = solar("r"), mag = TRUE, log = FALSE)

Arguments

knee

The knee(s) of the luminosity distribution

slope

The faint-end slope(s) of the luminosity distribution

norm

The normalisation(s) of the luminosity distribution

msun

The absolute magnitude of the sun

mag

Are the input knee values in magnitudes?

log

Are the input knee values logged?

Author(s)

Lee Kelvin <lee.kelvin@uibk.ac.at>

See Also

The astronomy package: astro.

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