Summary of recipes available in SPARK for processing KMOS data.
|Basic calibration and pipeline recipes|
|kmo_dark||Create master dark frame and preliminary bad pixel mask|
|kmo_flat||Create master flatfield frame, spatial calibration frames, and final badpixel map|
|kmo_wave_cal||Create a spectral calibration frame|
|kmo_illumination||Create calibration frame to correct spatial non-uniformity of flatfield|
|kmo_std_star||Create telluric correction spectra and calculate zeropoint|
|kmo_sci_red||Perform standard science reduction on a set of observations|
|kmo_multi_reconstruct||Reconstruct and combine cubes simultaneously from multiple frames|
|kmo_arithmetic||Perform basic arithmetic on frames and cubes|
|kmo_sky_tweak||Subtract sky cubes from object cubes, applying scaling based on OH line strengths|
|kmo_make_image||Collapse a cube spectrally to create a spatial image|
|kmo_extract_spec||Extract a spectrum from a cube|
|kmo_fit_profile||Fit spectral or spatial profiles to lines or objects|
|kmo_stats||Calculate basic statistical properties of a frame or cube|
|kmo_reconstruct||Perform cube reconstruction on a single frame|
|kmo_combine||Combine reconstructed cubes|
|kmo_shift||Shift a cube spatially by a sub-pixel increment|
|kmo_rotate||Rotate a cube spatially|
|kmo_noise_map||Generate a noise map from a raw frame|
|kmo_copy||Copy a section of a cube|
|kmo_fits_check||Check contents of a KMOS fits file|
|kmo_sky_mask||Create a mask of spatial pixels that can be considered as sky|
|kmo_fits_strip||Strip extensions (noise, rotator angles, and/or empty extensions) from a file|
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