prompt> gtpspec
This is gtpspec version v10r5
Event data file name[] my_pulsar_events_v3.fits
Spacecraft data file name[] my_pulsar_spacecraft_data_v3r1.fits
Name of input pulsar ephemerides database file (for binary demodulation only)[]  master_pulsardb_v3.fits
Pulsar name (for binary demodulation only)[ANY] PSR B0540-69
Output FITS file name (NONE for no FITS output)[] gtpspec-example-3.fits
Width of time bins, in seconds (0.:) [1.e-2] 0.01
Number of time bins to be transformed at once[1000000] 1000000
How will the time origin of the periodicity test be specified? (START|STOP|MIDDLEE|USER) [MIDDLE] MIDDLE
Right Ascension to be used for barycenter corrections (degrees)[0.] 85.0482
Declination to be used for barycenter corrections (degrees)[0.] -69.3319
How will spin ephemeris be specified? (FREQ|PER) [FREQ] PER
Ratio of period first time derivative to period at the time origin (Hz)[0.] 9.51 3929377105503722e-12
Ratio of period second time derivative to period at the time origin (Hz/s)[0.] 0 .0
Search Type: Fourier Analysis
Fourier Resolution: 0.0001 Hz
Sampling Frequency: 0.0001 Hz
Data Binning: 8 segments with 1000000 time bins in each segment
Probability Distribution: Chi Squared with 16 degrees of freedom
Search Range (Hz): [0.01, 50]
Number of Trial Frequencies: 499900
Number of Independent Trials: 499900
Maximum Statistic: 458.596889004188 at 19.834 Hz
Chance Probability Range: (8.90394487367336e-82, 8.90483527617709e-82)
Warning in <TClass::TClass>: no dictionary for class st_graph::IFrame is available
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