Using machine learning methods in Julia to analyze astronomical time series data.
##Process
- Galex data stuff
- Split Data for Parallelization
- Preprocessing
- more descriptive stuff here
- more stuff
- Combine Features
- Normalize and Impute Features
- Cluster
##Keywords Extracted from Kepler FITS Files
- KEPLERID unique Kepler target identifier
- GRCOLOR [mag] (g-r) color, SDSS bands
- JKCOLOR [mag] (J-K) color, 2MASS bands
- GKCOLOR [mag] (g-K) color, SDSS g - 2MASS K
- TEFF [K] Effective temperature
- LOGG [cm/s2] log10 surface gravity
- FEH [log10([Fe/H])] metallicity
- RADIUS [solar radii] stellar radius
##Things TO DO:
- Clean up the directory
- make this documentation more comprehensive
create multiplotslightcurveperiodgramsphasefolded light curve
- finish multiplot driver
title the plot with KID- print the plots to a directory
- get membership of clustering results
- look at projections of the feature space
- plot the targets against two features
- Clean up drivers and use SETTINGS.txt to make code work for any machine
- Investigate artifacts on feature plots