completeness: AUC function
In m-a-r-i-o/aRtistic: Finding Intermediate Mass Black Holes In Star Clusters With Machine Learning
Description
Usage
Arguments
Examples
Description
This function returns the probability that a star at rho and L is seen
by using an analytical recipe for completeness
Usage
1
completeness(R2D, R2Dcut, L, Lcut)
Arguments
R2D
vector of 2D- radial positions of stars
R2Dcut
scale radius (e.g. half-mass radius)
L
vector of stellar luminosities
Lcut
scale luminosity (e.g. 0.5 solar)
Examples
1
completeness(r, 1.0, L, 0.5)
m-a-r-i-o/aRtistic documentation built on May 7, 2019, 9:37 a.m.
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Description Usage Arguments Examples
Description
This function returns the probability that a star at rho and L is seen by using an analytical recipe for completeness
Usage
1 | completeness(R2D, R2Dcut, L, Lcut)
|
Arguments
R2D |
vector of 2D- radial positions of stars |
R2Dcut |
scale radius (e.g. half-mass radius) |
L |
vector of stellar luminosities |
Lcut |
scale luminosity (e.g. 0.5 solar) |
Examples
1 | completeness(r, 1.0, L, 0.5)
|
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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