JWST v1.1.0 (Build 7.7.1)
assign_mtwcs
- Fixed a bug which caused the step to fail with
MultiSlitModel
input. [#JP-1907]
assign_wcs
-
Added velocity aberration-corrected frame
'v2v3vacorr'
to the WCS
pipeline which takes into account DVA effects. [#5602] -
Renamed MIRI frame
'V2_V3_spatial'
to'v2v3_spatial'
and
'V2_V3_vacorr_spatial'
to'v2v3vacorr_spatial'
. Added axes names
to the'v2v3'
frame fornircam
,niriss
,miri
, andfgs
.
Renamed axes fornirspec
fromV2
andV3
to
v2
andv3
. [#5765] -
Changed units of the
'v2v3'
frame fornircam
fromu.deg
to
u.arcsec
[#5765] -
Added spectral frames to the output WCS frame of TSO and WFSS observations. [#5771]
associations
-
Warn about duplicate product names and do not write duplicate associations [#5721]
-
Added new Lvl2 rule, Asn_Lv2NRSLAMPImage, to run Image2 pipeline for NRSLAMP
exposures with OPMODE=image [#5740] -
Ignore duplicate product names while handling Level 2 associations [#5780]
-
Constraint added to Asn_Lv3Coron to remove background exposures [#5781]
combine_1d
- Pull source_id from input x1d headers (from source_catalog) to populate
c1d output headers [#5759]
cube_build
-
Added support for cross-dichroic configurations [#5722]
-
Added infrastructure to support NIRSpec opaque + grating options to build lamp mode data [#5757]
-
When building MIRI internal_cal type cubes removed the requirement that cdelt1=cdelt2 [#5757]
datamodels
-
Updated keyword_readpatt, core, preadpatt schemas for new MIRI detector
readout patterns 'FASTR1', 'FASTR100' and 'SLOWR1' [#5670] -
Added extr_x and extr_y to multispec datamodel. These values are center
of extraction region for IFU data [#5685] -
Added segmentation map output file name to core schema keywords, under
keyword 'SEGMFILE' [#5730] -
Added '1LOS' to PATTTYPE enum list in core.schema datamodel [#5728]
-
Added 'IMAGE' to OPMODE enum list [#5745]
-
Added source_id to combinedspec and multicombinedspec schemas to populate
combine1d output headers [#5759]
extract_1d
-
Adding writing SRCTYPE, EXTR_X, and EXTR_Y to extracted spec for IFU data [#5685]
-
Only update the output x1d data using the PRIMARY input data. Prevents SCI data in x1d data [#5694]
-
Fixed bug in background region fitting for image columns/rows that have zero weight
for all pixels [#5696] -
Determine the background using sigma clipping of entire extended region for
extended source IFU data [#5743]
group_scale
- Fix premature model closing in group_scale_step [#5692]
lib
-
Make EngDB_Value public for JSDP use [#5669]
-
Update code in
set_velocity_aberration.py
functions based on Colin Cox
suggestions: simplify DVA scale computation and improve apparentRA
and
DEC
aberrated position computation. Also, attributesra_offset
and
dec_offset
ofdatamodel.meta.velocity_aberration
have been renamed to
va_ra_ref
andva_dec_ref
and their corresponding FITS keywords
have been renamed fromDVA_RA
andDVA_DEC
to
VA_RA
andVA_DEC
. [#5666] -
Make get_wcs_values_from_siaf public for JSDP use [#5669]
outlier_detection
- Remove hard-coded MRS outlier detection values now that a parameter reference
file exists. [#5753]
photom
- Fixed handling of NIRSpec IFU extended source data, so that the flux
calibration gets converted to surface brightness [#5761]
pipeline
- Remove references to Numpy globals
np.int
,np.float
,np.bool
and
np.str
in the package. [#5769]
ramp_fitting
-
Fixed bug in handling NGROUPS=2 exposures for pixels that saturate in group 2.
Proper slope, err, and other quantities are now computed from the good data
in group 1. [#5700] -
Update documentation to define optimal weighting algorithm [#5682]
resample
- Make inverse variance
weight_type="ivm"
the default weighting scheme for
multiple exposures resampled into a single output. [#5738]
source_catalog
- Added the segmentation map as an output data file, with
suffix "segm". [#5730]
srctype
-
Changed default SRCTYPE for non-primary NIRSpec slits in a FIXEDSLIT
exposure to 'EXTENDED' rather than 'POINT' [#5671] -
Changed logic for handling NIRSpec MOS exposures to blank out the "global"
value of SRCTYPE, to ensure that only the individual slit-specific values
of SRCTYPE get used downstream. [#5754]