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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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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
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