aorfile = "m31_3x3_cycle.001.isds" File created by aorexpand (output = "3x3/") Path for output directory (include final /) (dosky = yes) Simulate exposures to model sky? (model1 = "m31_sim_ch1_1.2.fits") Image of model sky at 3 um (model2 = "m31_sim_ch2_1.2.fits") Image of model sky at 4 um (model3 = "m31_sim_ch3_1.2.fits") Image of model sky at 6 um (model4 = "m31_sim_ch4_1.2.fits") Image of model sky at 8 um (restart = no) Use already-rotated model sky images (possible (truepos = yes) Use true relative positions of FOVs and map ras (dopnterr = yes) Simulate relative and absolute pointing errors? (pnterr = 1.2) Magnitude of average pointing error (arcsec) (dojitter = yes) Simulate telescope jitter? (shotnoise = yes) Simulate shot (photon) noise? (crrate = 1.) Cosmic ray hit rate (hits/sec/detector)? (background = yes) Add constant sky background to model sky images (picdfrac = 1.) Fraction of PICD background in simulation (readnoise = yes) Simulate read noise? (library = "/ssc/testdata/irac/isds/images/") iracsim image library (inclu (gains = no) Simulate pixel-to-pixel gain maps? (bias = no) Simulate fluctuating bias? (darks = no) Simulate dark charge? (dobandwidth = no) Simulate finite-bandwidth A/D converter readout (bandwidthmag = 0.01) Magnitude of the finite-bandwidth effect (nonlinear = no) Simulate nonlinearities in the array pixels? (latent = no) Simulate latent image effects? (latency = 0.002) Strength of image latency (0.0-1.0) (muxbleed = no) Simulate multiplexer bleed? (rawheader = no) Output FOS headers(yes) or BCD headers(NO) (rawimage = no) Output raw science data (yes) or BCD style(NO) (verbose = 4) Print out (>1) or not (1) diagnotic messages (mode = "ql")