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Institut für Astronomie und Astrophysik

Abteilung Astronomie

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TRIPP_SHOW_RELFLUX Source code in tripp_show_relflux.pro

TRIPP_SHOW_RELFLUX

Name
       TRIPP_SHOW_RELFLUX
Purpose
       Plot lightcurve and period spectrum as found with SCARGLE
       of reduced photometrical data obtained with
       TRIPP_CALC_RELFLUX using different extraction radii and save results
       to ps-File for inspection
Category
       Astronomical Photometry.
Calling Sequence
       TRIPP_SHOW_RELFLUX, LOGNAME = logName
Input Parameters
       IDL SAVE files *_*.RMS
Output Parameters
       PS file '*_relflux.PS' showing lightcurve  of data block
       and its period spectrum
Restrictions
       file type:      RMSExtended as produced by TRIPP_CALC_RELFLUX
       Input directory and filename structure as specified in Log
Revision History
       Version 1.0, 1999/07, Sonja Schuh    (combined TRIPP_SHOW_RELFLUX
                                             and TRIPP_SHOW_FT)
       Version 1.1, 2000/11, Sonja L. Schuh, added panels with cut
                                             flux, switched to /landscape
       Version 1.2, 2001/02, Sonja L. Schuh, - added keyword /mouse,
                     which triggers the usage of, mainly, the CCD_MEAN routine for
                     a display of the quality of the lightcurves at different
                     extraction radii; new extraction radius can then
                     be chosen and will change the log- and rmsfile for consistency.
                                             - use new scargle from aitlib
                    2001/02 SLS, added messages
                    2001/02 SLS, comparison for radii needs to be
                                 done in floats
                    2001/05 SLS, adapted to frame transfer method
                                 (keywords frame*)
                    2002/05 SLS, added approximate JD start of
                                 observation
                    2004/08 SLS, S.D. Huegelmeyer, sorting of time
                                 indices in order to do a Fourier
                                 Transform. Important for  use with
                                 'filelist'.
                    2004/10 S.D. Huegelmeyer, creating of .ps files
                                 with lightcurves for all reference
                                 stars.
                    2005/09 S.S.,avoid plots with zero axis length
                                 for the case of only one ref star
                    2006/10 S.S.,require indices for t/fanschauen
                                 GT 2 instead of GE 2

Last modified by pro2html on 2006 December 19 at 04:11 UTC

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Jörn Wilms ([email protected])
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