Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
TRIPP_SHOW_EPOC
Calculate epoc folding of reduced photometrical data obtained with TRIPP_WRITE_FINAL from several combined blocks (or a single one). Show processed data as lightcurve, and result of epoc folding as obtained with epfold in one ps-File. The front page contains additional information about the processing etc.
Astronomical Photometry.
TRIPP_SHOW_EPOC, fileName, wc
ASCII LIGHTCURVE, TIME IN DAYS
FT_MIN : MINIMUM FREQUENCY IN MICRO-HZ FT_MAX : MAXIMUM FREQUENCY IN MICRO-HZ P_MIN : MINIMUM PERIOD IN SECONDS P_MAX : MAXIMUM PERIOD IN SECONDS NR_PER : min. number of periods you want to be covered NIF : Number of frequencies used in SCARGLE SCSMOOTH: SMOOTHING OF THE LIGHTCURVE NBINS : Number of Phase bins, default set by epfold
PS file '*_all.PS' showing Fourier Transforms and Lightcurves of unbinned and binned data block file '*_PulsProfile' containing the normalized puls profile over one phase
file type: ascii x,y table of known length wc as input No restrictions due to LogFile, not needed here. You can either use p_min/max OR ft_min/max, if you give both the values for p_min/max will be ignored!
Version 1.0, 2000/03, Stefan Dreizler Version 1.1, 2001/02, SLS: - wc is not a necessary input any more - adapted to new epfold (period has been replaced by maxchierg) 2002/05, SLS, added approximate JD start of observation SLS, added print-out of period at which pulse profile is calculated
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