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Institut für Astronomie und Astrophysik

Abteilung Astronomie

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TRIPP_SHOW_EPOC Source code in tripp_show_epoc.pro

TRIPP_SHOW_EPOC

Name
       TRIPP_SHOW_EPOC
Purpose
       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.
Category
       Astronomical Photometry.
Calling Sequence
       TRIPP_SHOW_EPOC, fileName, wc
Input Parameters
       ASCII LIGHTCURVE, TIME IN DAYS
Optional Input Parameters
       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
Output Parameters
       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
Restrictions
       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!
Revision History
       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                                    been replaced by maxchierg)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

Last modified by pro2html on 2005 January 04 at 16:57 UTC

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Jörn Wilms (wilms@astro.uni-tuebingen.de)
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