Name of input spectrum true Get ebins from response set Name of input response set true Name of output ancillary response set true Specify the detector map origin Name of input detector map array true Specify bounds for psf/flat detector maps explicitly Upper/lower bounds of psf/flat detmap along x-dirn, wrt source posn detxoffset in [0:30000] Upper/lower bounds of psf/flat detmap along x-dirn, wrt source posn detyoffset in [0:30000] Specify the number of bins for psf/flat detector maps explicitly Number of bins along x-dirn in psf or flat detector map detxbins in [1:] Number of bins along y-dirn in psf or flat detector map detybins in [1:] Energy at which to compute PSF in psf detector map psfenergy in [0:30] Filter the input detector map Write out the detmap filtered pixel list Name of detmap filtered pixel list true Source position specified Coordinate system for which source position is specified X position of source true Y position of source true Source is extended Model Effective Area Model Quantum Efficiency Model Filter Transmission Model contamination Model Encircled Energy Model out-of-time factor Apply the effective area correction stored in CORRAREA ? Energy grid oversampling factor eegridfactor in [1:] Correct for bad pixels in source box File containing bad pixel extensions true The model to use for the instrument point spread function Bad pixel resolution set The resolution to use to check for bad pixels of all types and to calculate the PSF correction true Set the BACKSCAL value in input spectrum Whether to keep the generated ARF file Whether to use ODF attitude file Whether area outside the field-of-view should be excluded from calculations Whether to calculate the ARF due to flux from a different region Name of file containing the region where the flux originally falls