RMS N1 N2 N3 METHOD WEIGHTS -- Work out RMS variability spectrum Works out RMS spectrum from a time series of spectra Output slot contains : rms = sqrt ( < (f-Related commands: pbin , group , average , flare)^2 > ) Danny Steeghs @ soton mar 2000 Parameters: N1 -- Slot number of first spectrum to average N2 -- Slot number of last spectrum to average N3 -- Slot in which to put results METHOD - Averaging method. At present supports U -- Unit weights D -- Dwell weights R -- Response weights V -- Variance weights WEIGHTS -- a file of weights that multiply whatever weights are generated by method. to ignore. The weights should be for every spectrum regardless of selection. Response weights are proportional to the local ratio of COUNTS/FLUX and thus effectively add the counts together (optimum for photon counting data). Variance weights use a single value equal to the mean Signal/noise**2 for each spectrum. Selection is done. The spectra must have equal numbers of pixels, but no other properties in common. A warning is given if the wavelength scales differ but averaging still goes ahead
This command belongs to the class: time_series