Wilkinson Microwave Anisotropy Probe DR3The data made available through this page has been updated. The most recent version of this data may be accessed through https://lambda.gsfc.nasa.gov/product/wmap/current/" Optimal TimeDomain FiltersDownload Links:
The optimal timedomain filters are used in the creation of the first estimate of the WMAP maximum likelihood sky map solution: (M^{T} N^{1} d) product, also called the iteration zero (it0) map. Final maps are produced by multiplying the it0 maps by (M^{T} N^{1} M)^{1} through an iterative process. The N^{1} term represents the inverse radiometer noise correlation matrix and is computed using the inverse noise correlation function. This correlation function is the optimal timedomain filter. Please refer to Jarosik, et.at., 2006 for details on how the filter is used to create the inverse radiometer noise correlation matrix. There are three FITS files containing the collection of filters, one file for each year of data, and with each file containing the filters for all ten differencing assemblies. Each differencing assembly filter is written to its own FITS binary table extension, so there are ten such extensions in each file. The first column represents the lag time measured in samples of that radiometer. There are two columns that supply the the filters for each channel of that differencing assembly; the names of these columns names contain the radiometer channel names (e.g., FILTER_K11 and FILTER_K12, FILTER_W31 and FILTER_W32). Filter CreationDaily autocorrelation functions of timeordered data were calculated over lag time from 0 to 10^{4} s for each radiometer, using uncalibrated timeordered data from which a linear interpolation of the hourly baseline was subtracted and an estimate of the sky signal in counts was subtracted (Hinshaw et al 2003). Yearly mean autocorrelation functions C(Δt) were formed from 60 days of data for each year. A cubic of the form C(Δt)/C(0) = a + b log(Δt) + c [log(Δt)]^{2} + d [log(Δt)]^{3} was fit to the yearly mean data over lag time Δt from 2 times the sampling interval to 1000 s. Linear fits in log(Δt) were used for the K band radiometers, and quadratic fits were used for Ka; we make available the autocorrelation fit parameters in the form of an ASCII table. Optimal time domain filters were made using the measured C(Δt)/C(0) at lag 1, the fit from lag 2 to the lag time where the fit crosses zero (from 400 to 1000 s), and C(Δt)/C(0) equal to zero for greater times. For each radiometer and each year, the filter was formed as follows:
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