| Class: | jwst.wavecorr.WavecorrStep |
|---|---|
| Alias: | wavecorr |
The wavelength correction (wavecorr) step in the
:ref:`calwebb_spec2 <calwebb_spec2>` pipeline updates the wavelength
assignments for NIRSpec fixed-slit (FS) and MOS point sources that are
known to be off center (in the dispersion direction) in their slit.
For NIRSpec MOS exposures (EXP_TYPE="NRS_MSASPEC"), wavelength assignments created during :ref:`extract_2d <extract_2d_step>` are based on a source that's perfectly centered in a slitlet. Most sources, however, are not centered in every slitlet in a real observation. The MSA meta data assigned to each slitlet in the :ref:`extract_2d <extract_2d_step>` step includes estimates of the source x (dispersion) and y (cross-dispersion) location within the slitlet. These are recorded in the "SRCXPOS" and "SRCYPOS" keywords in the SCI extension header of each slitlet in a FITS product.
The wavecorr step loops over all slit instances in the input
science product and applies a wavelength correction to slits that
contain a point source. The point source determination is based on the
value of the "SRCTYPE" keyword populated for each slit by the
:ref:`srctype <srctype_step>` step. The computation of the correction is
based on the "SRCXPOS" value. A value of 0.0 indicates a perfectly centered
source, and ranges from -0.5 to +0.5 for sources at the extreme edges
of a slit. The computation uses calibration data from the WAVECORR
reference file. The correction is computed as a 2-D grid of
wavelength offsets, which is applied to the original 2-D grid of
wavelengths associated with each slit.
Fixed slit data do not have an a priori estimate of the source
location within a given slit, so the estimated source location is
computed by the wavecorr step. It uses the target coordinates in
conjunction with the aperture reference point in V2/V3 space to
estimate the fractional location of the source within the given slit.
Note that this computation can only be performed for the primary slit
in the exposure, which is given in the "FXD_SLIT" keyword. The positions
of sources in any additional slits cannot be estimated and therefore
the wavelength correction is only applied to the primary slit.
The estimated position of the source within the primary slit (in the dispersion direction) is then used in the same manner as described above for MOS slitlets to compute offsets to be added to the nominal wavelength grid for the primary slit.
Upon successful completion of the step, the status keyword "S_WAVCOR" is set to "COMPLETE".