(re)start processing at conclude processing at enable explicit subset of exposures instrument-exposure id list true reflection orders for spectrum generation orders in [1:6] delete intermediate files Dispersion binning method enable filename prefix override prefix for product filenames true [seconds] time step timestep in [0:] [arcmin] GTI attitude drift limit driftlimit in [0:] use last exposure attitude points for filtering instead of full exposure add sources from an epic-derived source list name of the epic-derived source list true add a source with user-defined position, rate etc label for the user-defined source true rate value (if known) for the user-defined source srcrate in [0:] style for entering the position of the user-defined source [decimal degrees] right ascension of the user-defined source true [decimal degrees] declination of the user-defined source true [arcmin] dispersion off-axis angle of the user-defined source true [arcmin] cross-dispersion off-axis angle of the user-defined source true for defining the reference attitude [decimal degrees] right ascension of the user-defined attitude true [decimal degrees] declination of the user-defined attitude true [decimal degrees] position angle of the user-defined attitude true calculate offsets from diagnostic mode Store histograms in a dataset enable offset subtraction from Diagnostic Offset Average files enable gain correction enable CTI correction include non-uplinked CCF bad pixels include found hot pixels include (do not discard) non-uplinked CCF cool pixels hot pixel threshold pulse height pixnoiselimit in [0:4095] hot column threshold pulse height colnoiselimit in [0:4095] hot pixel sharpness criterion pixsharpness in [0:] hot column sharpness criterion colsharpness in [0:] detector coordinate system enable detector coordinate output enable event reconstruction Specify number or size of beta bins midpoint of bin for which BETACHA is one [rad] true width of beta bin [rad] betabinwidth in [0:] number of beta bins nbetabins in [1:] lowerleft of first beta bin [rad] true top end of last beta bin [rad] true Specify number or size of cross-dispersion bins midpoint of bin for which XDSPCHA is one [rad] true width of cross dispersion bin [rad] xdispbinwidth in [0:] number of xdisp bins nxdispbins in [1:] lowerleft of first xdisp bin [rad] true top end of last xdisp bin [rad] true Produce columns with Spacecraft Pointing Produce column with m*lambda (source at requested position) Apply heliocentric velocity correction to mlambda column Apply Sun Angle correction to mlambda column event rejection flags [arcsec] drift quantization width driftbinsize in [0:] generate the combined exposure map Additional GTI tables true vertices per node across spatial regions spatialres in [2:] vertices per node across order regions orderres in [2:] percent of cross-dispersion PSF included xpsfincl in [0:100] percent of cross-dispersion PSF excluded from background xpsfexcl in [0:100] percent of pulse-height distribution included pdistincl in [0:100] PI cutoff switch Excluded PI region below this value (eV). Extended regions selected background selected select which sources to process true select which sources to exclude from background true background correct the spectra generate background spectra Calculate background model flag chip-edge channels as dubious edgechannels in [0:] dispersion channel rebinning factor rebin in [1:] add FRAC_EXP column to output files minimum good fractional exposure exposed in [0:1] QUALITY used to flag bad channels badquality in [0:5] number of response energy bins rmfbins in [1:] convolution size exponent fftdim in [1:5] whether to include the standard mirror PSF distribution whether to include a custom angular distribution user-defined angular distribution file flux all orders together output file format computational mode minimum output wavelength or energy flxmin in [0:] maximum output wavelength or energy flxmax in [0:] number of output bins flxbins in [1:] usable quality in promotion order flxquality in [0:5] enable alternate NaN value alternate NaN value true enable dynamic Effective Area Correction. Use empirical RGS effective area correction midpoint of bin for which LAMBDACHA is one [Angstrom] true width of lambda bin [Angstroms] lambdabinwidth in [0:] number of lambda bins nlambdabins in [1:] Calculate Heliocentric velocity correction Size of time bins for time series files timebinsize in [0:] Substract background