lumdens: Luminosity Density

In taranu/astro: Astronomy Functions, Tools and Routines

Description

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

Usage

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 <[e-mail]>

See Also

The astronomy package: astro.

taranu/astro documentation built on May 23, 2019, 7:36 a.m.