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cpl-plugin-fors-doc
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cpl-plugin-fors-doc
33
Section 7:
Miscellaneous
fors_align_sky.7
Upgrade wavelength solution using sky lines
fors_align_sky_lss.7
Upgrade wavelength solution using sky lines
fors_bias.7
Compute the master bias frame
fors_calib.7
Determination of the extraction mask
fors_config.7
Creation of fors recipes configuration tables
fors_dark.7
Compute master dark frame
fors_detect_objects.7
Detect objects in slit spectra
fors_detect_spectra.7
Detect mos/mxu spectra on ccd
fors_extract.7
Extraction of scientific spectra
fors_extract_objects.7
Extract objects in slit spectra
fors_extract_slits.7
Spatial rectification of spectral image
fors_flatfield.7
Flat field correction of input frame
fors_img_science.7
Reduce scientific exposure
fors_img_screen_flat.7
Compute master screen flat frame
fors_img_sky_flat.7
Compute master img_sky_flat frame
fors_normalise_flat.7
Normalise master flat spectrum
fors_photometry.7
Compute corrected flatfield
fors_pmos_calib.7
Determination of the extraction mask
fors_pmos_extract.7
Extraction of scientific spectra
fors_pmos_science.7
Extraction of scientific spectra
fors_remove_bias.7
Subtract bias from input frame
fors_resample.7
Resample input spectra at constant wavelength step
fors_science.7
Extraction of scientific spectra
fors_spec_mflat.7
Computes master spectroscopic flat, removing bias first
fors_subtract_sky.7
Subtract sky from scientific spectra
fors_subtract_sky_lss.7
Subtract sky from calibrated long slit exposure
fors_sumflux.7
Integrate flux from all or part of the input frame
fors_trace_flat.7
Determine spectral curvature model
fors_wave_calib.7
Derive dispersion relation from rectified arc lamp frame
fors_wave_calib_lss.7
Derive dispersion relation from long-slit arc lamp frame
fors_zeropoint.7
Compute zeropoint
montecarlo.7
Test function mos_montecarlo_polyfit()
test_hough.7
Test hough transform on any table of points