Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
dynpsrch
produce a dynamical period search of a timeseries and display PSD or \chi^2 of Epoch Fold
time series analysis
dynpsrch,tt,rr,file,ghost=ghost,dt=dt,tlen=tlen, pmin=pmin,pmax=pmax,numf=numf, /log, /epoch, /nolabel
tt: time rr: count rate file: file name of encapsulated PS-File to be produced
dt: time distance between individual PSDs (default: 4) tlen: length of the individual time series that are used to generate the PSD pmin: minimum period to consider (2.*dt default) pmax: maximum period to consider (tlen/2) numf: number of frequency points (500) sig : significance levels (99, and 99.9 %) raterr: error bars for rate. Plot symbols instead of lines. sunangdist: angular distance between the sun and the ASM object. Make an angular distance versus time plot. multiple: number of simulations to obtain the significance levels, if not set or <=0, then the significance is computed from the standard formula, and not using simulations (faster, but not recommended...) ylaxisv: The data values for each tick mark for the y left axis.
ghost: invoke ghostscript after plot is done gray: gray scale plot instead of color color: It's color instead of count rate tbin: Do psym=10 plots, with errors, in a way that will make even Joern happy (i.e., gaps are explicit) nolabel: Don't put a label on the ASM significance levels! log: Make logarithmic period axes on the plot epoch: Epoch fold instead of Lomb-Scargle (default) window: Apply a Welch Window to the data
an encapsulated postscript file is produced
px: PSD values for lomb-Scargle periodogram or \chi^2 values for Epoch Fold period: period corresponding to each PSD value for lomb-Scargle periodogram or trial periods for Epoch Fold maxchi2per: period of maximum chi^2 for Epoch Fold psdpeaksort : array with the maximum peak from the lom-Scargle periodogram pro each simulation simsigni : power threshold corresponding to the given false alarm probabilities fap according to white noise simulations for the PSD;
it is not checked whether the desired period range is meaningful
pieces of length tlen of the time series are transformed with the lomb scargle periodogram or epoch folded and then are normalized to the maximum value. The result is plotted.
Requires: scargle.pro, epfold.pro (=> pfold.pro), jwoploterr, jwmjdaxis, jwdateaxis, open_print, close_print
Version 0.5: 1999/08/07 (dynscarg): Joern Wilms (wilms@astro.uni-tuebingen.de) Version 0.6: 1999/08/25: Joern Wilms I hope the normalization is now finally all right... Version 0.7: 1999/08/26: Michael Nowak (mnowak@rocinante.colorado.edu) Added raterr as an optional input, color as a keyword, tbin as a keyword Version 0.8 (dynpsrch): 1999/10/21: Michael Nowak Added log as a keyword, to produce logarithmic plots Added epoch as a keyword, to do an epoch fold instead tvscal now centers pixels on mid-point of PSD/Fold, & width of plot is now more carefully calculated pmin is defaulted to 2.*dt Version 0.9: 1999/11/02: Michael Nowak Following Padi Boyd's suggestion, added padding of lightcurves to allow dynamical PSD to be done over whole lightcurve range. Added keyword to window function the lightcurve with a Welch window. Version 1.0: 1999/11/30: Sara Benlloch Added sunangdist as a optional input, to plot the angular distance between the sun and the ASM object versus the time, in order to check the sun influence. Version 1.1: 2000/08/31: Sara Benlloch / J. Wilms adopted to new (fast) scargle routine
[Home Page] [Software, Documentation] [IDL Documentation] [Quick Reference] [Feedback]