![]() |
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been replaced by maxchierg)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
[Home Page] [Software, Documentation] [IDL Documentation] [Quick Reference] [Feedback]