Step Arguments
The straylight
step has the following optional arguments.
--clean_showers
(boolean, default=False)A flag to indicate whether to remove straylight due to residual cosmic ray showers using pixels between the IFU slices.
--shower_plane
(int, default=3)Identifies the throughput plane to use from the MRS regions reference files to identify between-slice pixels. Lower values identify pixels with less science signal, but result in fewer (or no) pixels between slices in some bands.
--shower_x_stddev
(float, default=18)Standard deviation to use for gaussian kernel convolution in the X (between-slice) direction. Must be large enough to reach the middle of the IFU slices.
--shower_y_stddev
(float, default=5)Standard deviation to use for gaussian kernel convolution in the Y (along-slice) direction.
--shower_low_reject
(float, default=0.1)Percentile of low-valued pixels to reject when performing gaussian kernel convolution. Important to ensure unmasked bad pixels do not bias the kernel convolution.
--shower_high_reject
(float, default=99.9)Percentile of high-valued pixels to reject when performing gaussian kernel convolution. Important to ensure unmasked bad pixels do not bias the kernel convolution.