dmcep: Double Mode Cepheid.
In iAR: Irregularly Observed Autoregressive Models
dmcep R Documentation
Double Mode Cepheid.
Description
Time series of a double mode cepheid variable star obtained from OGLE.
Usage
dmcep
Format
A data frame with 191 observations on the following 3 variables:
- t
heliocentric Julian Day
- m
magnitude
- merr
measurement error of the magnitude (in mag).
Details
The dominant frequency computed by GLS for this light curve is 0.7410152.
The second frequency computed by GLS for this light curve is 0.5433353.
OGLE-ID:175210
Examples
data(dmcep)
f1=0.7410152
foldlc(dmcep,f1)
fit=harmonicfit(dmcep,f1)
f2=0.5433353
foldlc(cbind(dmcep$t,fit$res,dmcep$merr),f2)
iAR documentation built on Nov. 25, 2022, 1:06 a.m.
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| dmcep | R Documentation |
Double Mode Cepheid.
Description
Time series of a double mode cepheid variable star obtained from OGLE.
Usage
dmcep
Format
A data frame with 191 observations on the following 3 variables:
- t
heliocentric Julian Day
- m
magnitude
- merr
measurement error of the magnitude (in mag).
Details
The dominant frequency computed by GLS for this light curve is 0.7410152. The second frequency computed by GLS for this light curve is 0.5433353. OGLE-ID:175210
Examples
data(dmcep) f1=0.7410152 foldlc(dmcep,f1) fit=harmonicfit(dmcep,f1) f2=0.5433353 foldlc(cbind(dmcep$t,fit$res,dmcep$merr),f2)
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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