rate -- To create light curves binned on 30-s intervals for the seven bands.
rate obs r1lband imask maskname
To create light curves binned on 30-s intervals for the seven bands. The output is used in conjunction with the output of the program AO in the program RATE_FIT to fit the scattered solar X-ray and long-term enhancement background contamination. The capability now exists to mask out the contributions of bright point sources or extended sources to the light curves. This can become important when, for instance, a strong flaring source affects the modeling process. In practice this has not been much of a problem, but the possibility should be kept in mind. The most noticeable effect comes when a bright source is found near the window support structure or the edge of the field and is wobbled in and out of the open area. In this case, there will be strong variations in the light curve with the wobble period. The light-curve described below is in general not sensitive to that frequency of variation so the fitted parameters remain reasonable while the reduced Chi squared value can be very large (e.g., 5-10). Note that if a mask is used in RATE, the same mask must be used in CAST_SSX.
The RATE package uses the following input files.
1) Observation data fits files : xxx_ANC.FITS and xxx_BAS.FITS for RDF data
2) valid_times_all.dat
3) Mask: (if desired); mask file should have same format as the output of DETECT.
The output from the RATE package are the following ASCII files.
RATE1.DAT and RATE2.DAT: Files containing light-curve count rates, count-rate uncertainties, and particle background count rates.
PARAMETERS
1. For input data files test_ANC.FITS and test_BAS.FITS, assuming low-gain data and a maskfile name mask_17.fits;
ft> rate test no 1 mask_17.fits
The "OBS" parameter must be limited to 8 characters. Versions prior to FTOOLS 4.3 required that the input files be in uppercase; this requirement was removed in FTOOLS 4.3