lum.sol: Flux to luminosity in Sols
In mlpeck/cosmo: Cosmological distances
Description
Usage
Arguments
Details
Value
Author(s)
See Also
Description
Convert observed flux from an object at redshift z
to luminosity over Sun's bolometric luminosity.
Usage
1
Arguments
flux
Observed flux in units of 10^(-17) erg/cm^2/sec
z
redshift
...
cosmological parameters passed to dcos
Details
All values can be vectors.
Cosmological parameters must be named if they are used.
See dcos.
Value
Luminosity in units of the solar bolometric luminosity.
Values < 0 return NA.
Author(s)
M.L. Peck
See Also
mlpeck/cosmo documentation built on May 23, 2019, 3:02 a.m.
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Description Usage Arguments Details Value Author(s) See Also
Description
Convert observed flux from an object at redshift z to luminosity over Sun's bolometric luminosity.
Usage
1 |
Arguments
flux |
Observed flux in units of 10^(-17) erg/cm^2/sec |
z |
redshift |
... |
cosmological parameters passed to |
Details
All values can be vectors.
Cosmological parameters must be named if they are used.
See dcos.
Value
Luminosity in units of the solar bolometric luminosity.
Values < 0 return NA.
Author(s)
M.L. Peck
See Also
R Package Documentation
Browse R Packages
We want your feedback!
Note that we can't provide technical support on individual packages. You should contact the package authors for that.
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