MUSE Pipeline Reference Manual  1.0
Modules
Here is a list of all modules:
oArtifact handling
oAstronomical tools
oBasic-processing function
oCombination of images
oCPL wrappers
oDAR (Differential Atmospheric Refraction)
oExternal FITS table formats
oDatacube handling
oFlux calibration
oGeometrical calibration
oImage handling for the MUSE format
oImagelist processing for the four-extension image format
oLine Spread Function related functions
oProtected access to FITS headers
oPixel grid
oPixel table handling
oPost-processing functions
oProcessing framework
oQuadrants and other CCD regions
oQuality flag handling
oResampling
oRadial velocity corrections
oSky subtraction
oTracing
oUtilities
oWavelength calibration
oWorld coordinate system (WCS) related functions
oXposure combination
oTool muse_badpix_from_ascii
oTool muse_badpix_from_dq
oTool muse_badpix_from_region
oTool muse_cube_combine
oTool muse_cube_filtermuse_cube_filter: Add filtered images for existing MUSE cubes
oTool muse_fill_image
oTool muse_geo_plot
oTool muse_image_fwhm
oTool muse_lsf_fwhm
oTool muse_pixtable_crop
oTool muse_pixtable_dump
oTool muse_pixtable_erase_slice
oTool muse_trace_plot_samples
oTool muse_trace_plot_widths
oTool muse_wave_plot_column
oTool muse_wave_plot_residuals
oRecipe muse_ampl: Determine the instrumental throughput from exposures taken with the pico-amplifier / photo diode readings.
oRecipe muse_astrometry: Compute an astrometric solution.
oRecipe muse_bias: Combine several separate bias images into one master bias file.
oRecipe muse_create_sky: Create night sky model from selected pixels of an exposure of empty sky.
oRecipe muse_dark: Combine several separate dark images into one master dark file and locate hot pixels.
oRecipe muse_exp_combine: Combine several exposures into one datacube.
oRecipe muse_flat: Combine several separate flat images into one master flat file, trace slice locations, and locate dark pixels.
oRecipe muse_geometry: Compute relative location of the slices within the field of view and measure the instrumental PSF on the detectors.
oRecipe muse_lsf: Compute the LSF
oRecipe muse_qi_mask: Create image masks for use with the quick image reconstruction.
oRecipe muse_scibasic: Remove the instrumental signature from the data of each CCD and convert them from an image into a pixel table.
oRecipe muse_scipost_apply_astrometry: Calibrate astrometry for MUSE pixel tables.
oRecipe muse_scipost_calibrate_flux: Calibrate flux for MUSE pixel tables.
oRecipe muse_scipost_combine_pixtables: Combine MUSE pixel tables, either from different IFUs, or from different exposures, or both.
oRecipe muse_scipost_correct_dar: Apply DAR correction for MUSE pixel tables.
oRecipe muse_scipost_correct_rv: Apply RV correction for MUSE pixel tables.
oRecipe muse_scipost_make_cube: Make a MUSE cube from a MUSE pixel table.
oRecipe muse_scipost_subtract_sky: Subtract night sky model.
oRecipe muse_scipost: Prepare reduced and combined science products.
oRecipe muse_standard: Create a flux response curve from a standard star exposure.
oRecipe muse_twilight: Combine several twilight skyflats into one cube, compute correction factors for each IFU, and create a smooth 3D illumination correction.
\Recipe muse_wavecal: Detect arc emission lines and determine the wavelength solution for each slice.