API

Public Step API

jwst.wfss_contam.wfss_contam_step Module

Classes

WfssContamStep([name, parent, config_file, ...])

Perform contamination correction of WFSS spectra.

Complete Developer API

jwst.wfss_contam.disperse Module

Functions

disperse(xs, ys, fluxes, ...[, ...])

Compute the dispersed image pixel values from the direct image.

jwst.wfss_contam.observations Module

Functions

background_subtract(data[, box_size, ...])

Apply a simple astropy background subtraction.

Classes

Observation(direct_image, segmentation_map, ...)

Define an observation leading to a single grism image.

jwst.wfss_contam.sens1d Module

Functions

get_photom_data(phot_model, filter_name, ...)	Retrieve wavelength and response data from photom ref file.
create_1d_sens(data_waves, ref_waves, relresps)	Find photometric conversion values based on per-pixel wavelength-dependent response.

jwst.wfss_contam.wavefit Module

Fit a spectral shape to a WFSS dispersed source.

Functions

apply_basis_coeffs(simul_slit, coeffs)	Reconstruct a fitted slit as a linear combination of dispersed basis images.
fit_slit_by_basis_images(observed_slit, ...)	Fit a linear combination of dispersed basis images to the observed slit.

jwst.wfss_contam.wfss_contam Module

Top-level module for WFSS contamination correction.

Functions

contam_corr(input_model, waverange, photom, ...)

Correct contamination in WFSS spectral cutouts.