# Configuration for pyLINEAR cpu: &CPU ncpu: 1 # number of processors to use verbose: True calib: &CALIB h5conf: hst_wfc3_ir_beams.h5 # HDF5 file for beam info h5flat: Null # HDF5 file for flat field h5siaf: hst_wfc3_ir_detector.h5 # HDF5 file for detectors tables: &TABLES path: TABLES2/ # relative path for the tables remake: False gzip: True # gzip the resulting data nsub: 5 # number of intervals for TrapZ cpu: *CPU # import CPU settings sources: segmap: seg.fits # segmentation map for sources obslst: obs.lst # file describing the bands detindex: 0 # detection index in obslst maglim: 26. # magnitude limit of sources modules: simulation: perform: True # flag to run the simulation beam: A # beams to simulate grism: G102 # which grism to simulate imgtype: wcs # where WCS comes from: wcs or img gzip: True # gzip the outputs imglst: wcs.lst sedlst: sed.lst noise: perform: False exptime: 700. skyrate: 0.3 cpu: *CPU calib: *CALIB tables: *TABLES extraction: perform: True mode: fixed group: False logdamp: -3.45161 #[-6., -1., 0.1] outroot: test2 imglst: flt.lst beam: A mask: Null dlamb: 25. initialize: 'broadband' # can be direct or broadband lsqr: atol: 1e-10 # a tol btol: 1e-10 conlim: 1e10 maxiter: 1e5 show: False cpu: *CPU calib: *CALIB tables: *TABLES mcmcunc: perform: False nwalkers: 100 nstep: 100 burn: 0.2 cpu: *CPU residuals: perform: True gzip: False cutout: perform: False beam: A #grism: G102 imglst: flt.lst padding: [0, 2] cpu: *CPU calib: *CALIB