The FORS 4.12.8 pipeline
These pages describe the python interface for the FORS pipeline recipes.
Additional recipes
- fors_wave_calib_lss
- Derive dispersion relation from long-slit arc lamp frame
- fors_resample
- Resample input spectra at constant wavelength step
- fors_config
- Creation of FORS recipes configuration tables
- fors_extract_objects
- Extract objects in slit spectra
- fors_detect_objects
- Detect objects in slit spectra
- fors_pmos_science
- Extraction of scientific spectra
- fors_extract_slits
- Spatial rectification of spectral image
- test_hough
- Test Hough transform on any table of points
- fors_subtract_sky
- Subtract sky from scientific spectra
- fors_remove_bias
- Subtract bias from input frame
- fors_normalise_flat
- Normalise master flat spectrum
- montecarlo
- Test function mos_montecarlo_polyfit()
- fors_photometry
- Compute corrected flatfield
- fors_subtract_sky_lss
- Subtract sky from calibrated long slit exposure
- fors_wave_calib
- Derive dispersion relation from rectified arc lamp frame
- fors_flatfield
- Flat field correction of input frame
- fors_detect_spectra
- Detect MOS/MXU spectra on CCD
- fors_trace_flat
- Determine spectral curvature model
- fors_align_sky_lss
- Upgrade wavelength solution using sky lines
- fors_align_sky
- Upgrade wavelength solution using sky lines
- fors_spec_mflat
- Computes master spectroscopic flat, removing bias first
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.