Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
scargle
Compute the lomb-scargle periodogram of an unevenly sampled lightcurve. Refer procedure "scargle" in the aitlib.
cafe
scargle[,range] [,subgroup][,group][,/add]
range - (optional) Defines range of data points to fold. This can be either: - Data point range, denoted by the data point number: <n1>[-], while , are positive numbers. Data point numbers start from zero. Open intervals can be represented with a "*" instead of the number. If only one number is given, a single data point will be referenced. If <val2> is less than all but the interval <val2>.. are referenced. - X value range, denoted by float point numbers: <val1>- , while , represents X values defining the interval to reference. Open intervals can be represented with a * instead of the value. If <val2> is less than <val1> all but the interval <val2>.. is referenced. - Vector of data point indices. The vector is denoted with [val,val,...,val] (indgen may be used also). - Boolean expressions with X/Y values. All values for which this expression is true are referenced. The expression may contain algebraic formulas combined with comparison operators "lt", "le", "eq", "gt", "ge" as used in IDL comparisons. For each data point a keyword is defined which has meaning and can be used for the boolean expression: x - The x-column value. y - The y-column value. error - The error column value. selected - True when the data point is selected. def - True when the data point is defined. x1 - Multi column first column value. x2 - Multi column second column value. x3 - Multi column third column value. To avoid interference with functions which also can be used a lower/upper case distinction is made. IDL funktions should be upper case. Default is to fold the entire data set. subgroup - (optional) The data set (subgroup) for which the model should be applied. This can be either the subgroup number or the file name representing the data set. It is possible to set more than one subgroup, either with numbers in brackets ([]) separated with ","; or denoting filenames with wildcards ("*"). Default are all subgroups in currently used group. group - (optional) The data group for which folding should applied. Default is the current group. Must be in range [0..29].
add - Do not overwrite existing subgroups (0) but use the next free one in current result group. periodout - Create period as x axis instead of frequencies (default) verbose - Report progress.
Following parameter could be set: fmin - minimum fmax - maximum frequency (NOT ANGULAR FREQ) to be used (has precedence over pmin,pmax) pmin - minimum pmax - maximum period to be used fap - false alarm probability desired (see Scargle et al., p. 840, and signi keyword). Default equal to 0.01 (99% significance) noise - for the normalization of the periodogram and the compute of the white noise simulations. If not set, equal to the variance of the original lc. multiple - number of white noise simulations for the FAP power level. Default equal to 0 (i.e., no simulations). numf - number of independent frequencies
The lomb-scargle psd in result group set with chres. The x-values are frequencies, the y values the computed power density spectrum.
Creates/Overrides first subgroup in the result group. If /add is used a new subgroup will be created.
The Lomb Scargle PSD is computed according to the definitions given by Scargle, 1982, ApJ, 263, 835, and Horne and Baliunas, 1986, MNRAS, 302, 757. Beware of patterns and clustered data points as the Horne results break down in this case! Read and understand the papers and this code before using it! For the fast algorithm read W.H. Press and G.B. Rybicki 1989, ApJ 338, 277.
> set, pmin=100 > set, pmax = 500 > scargle -> compute lomb-scargle periodogram between P=100..500sec
$Id: cafe_scargle.pro,v 1.6 2005/02/16 13:37:18 goehler Exp $
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