EXAMPLES -------- Commands to execute the examples: cd periodCorrect ../bin/timing2periodCorrect.Linux 5.dbl 5.res 5.err 0.4465 0.1855 >! output.txt cd .. cd timing ../bin/timing.Linux 5.dbl 5.res 0.4465 0.1855 >! output.txt cd .. cd timing_eclipse ../bin/timing_eclipse.Linux 5.dbl 5.res 0.4465 0.1855 >! output.txt cd .. These utilities run the last 4 binaries in the catalog. One of the binaries is "ambiguous"- same light curve, but different period, thus making 5 example light curves: uma0_08.dphca.07468.lc - "ambiguous" uma0_08.dphca.07587.lc uma0_10.dphca.09087.lc uma0_11.dphca.10277.lc ==================================================== FILE FORMATS ------------ periodCorrect results file format fields: 1. filename 2. period 3. corrected period 4. e * cos(w) ; where, e = eccentricity, and w = angle of perihelion 5. e ; the orbital eccentricity, less accurate 6. number of eclipse events used 7. reduced chi-squared of the linear fit --------------- timing/timing_eclipse results file format fields: 1. filename 2. period 3. alarm Score 4. corrected period 5. number of eclipses used 6. reduced chi-squared of the linear fit 7. parabolic F-test 8. Period rate of change, or P dot (sec/sec) 9. sinusoidal F-test 10. sinusoidal period (days) 11. sinusoidal amplitude (seconds) Note that columns 7-8 relate to the parabolic fit, and columns 9-11 relate to the sinusoidal fit to the timing O-C. ----------------------- timing_eclipse *.data file format: 1. time stamp 2. magnitude of an observation in the eclipse 3. magnitude uncertainty for the observation --- timing_eclipse *.fit file format: 1. time stamp 2. model light curve of the eclipse, with the original offset 3. model light curve of the eclipse, with the best-fit offset --- timing/timing_eclipse *.fitParab and *.fitSin file formats: 1. time stamp 2. best fit model (parabolic/sinusoidal) --- timing/timing_eclipse *.fourier 1. period (days) 2. frequency (1/days) 3. F-test for a sinusoidal O-C model the given period/frequency --- All the other output files are meant to be used by the SuperMongo (*.sm) script: *.plot.1 - O-C data points from the primary eclipses *.plot.2 - O-C data points from the secondary eclipses *.linear - A linear fit to all data points *.offset1 - An offsetted linear fit to the primary eclipse data points *.offset2 - An offsetted linear fit to the secondary eclipse data points