dmcep {iAR}

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)