The FORS 5.0.11 pipeline
These pages describe the python interface for the FORS pipeline recipes.
Additional recipes
- fors_align_sky
- Upgrade wavelength solution using sky lines
- fors_align_sky_lss
- Upgrade wavelength solution using sky lines
- fors_config
- Creation of FORS recipes configuration tables
- fors_detect_objects
- Detect objects in slit spectra
- fors_detect_spectra
- Detect MOS/MXU spectra on CCD
- fors_extract_objects
- Extract objects in slit spectra
- fors_extract_slits
- Spatial rectification of spectral image
- fors_flatfield
- Flat field correction of input frame
- fors_normalise_flat
- Normalise master flat spectrum
- fors_photometry
- Compute corrected flatfield
- fors_pmos_science
- Extraction of scientific spectra
- fors_remove_bias
- Subtract bias from input frame
- fors_resample
- Resample input spectra at constant wavelength step
- fors_spec_mflat
- Computes master spectroscopic flat, removing bias first
- fors_subtract_sky
- Subtract sky from scientific spectra
- fors_subtract_sky_lss
- Subtract sky from calibrated long slit exposure
- fors_trace_flat
- Determine spectral curvature model
- fors_wave_calib
- Derive dispersion relation from rectified arc lamp frame
- fors_wave_calib_lss
- Derive dispersion relation from long-slit arc lamp frame
- montecarlo
- Test function mos_montecarlo_polyfit()
- test_hough
- Test Hough transform on any table of points
Bug reports
If you experience an unexpected behavior of any component of the FORS
pipeline recipes package, please, first refer to the list of known problems
and limitations in the pipeline manual of the current FORS pipeline
release.
For any other issues or requests, please, send a report to the ESO User
Support Department, describing:
- the FORS pipeline version,
- the version of your OS and C compiler,
- the exact sequence of actions that were performed before the problem occurred,
- what were precisely the symptoms and the possible error message(s),
- whether the problem is repeatable.