This step creates image catalogs of point-like sources whose centroids are then used to compute corrections to the WCS of the input images such that sky catalogs obtained from the image catalogs using the corrected WCS will align on the sky.
Stars are detected in the image using the Photutils “daofind” function. Photutils.daofind is an implementation of the DAOFIND algorithm (Stetson 1987, PASP 99, 191). It searches images for local density maxima that have a peak amplitude greater than a specified threshold (the threshold is applied to a convolved image) and have a size and shape similar to a defined 2D Gaussian kernel. Photutils.daofind also provides an estimate of the objects roundness and sharpness, whose lower and upper bounds can be specified.
The source catalogs for each input image are compared to each other and linear (affine) coordinate transformations that align these catalogs are derived. This fit insures that all the input images are aligned relative to each other. This step produces a combined source catalog for the entire set of input images as if they were combined into a single mosaic.
If the step parameter
align_to_gaia is True, an astrometric
reference catalog then gets generated by querying
a GAIA-based astrometric catalog web service for all astrometrically
measured sources in the combined field-of-view of the set of input
images. This catalog gets generated from the catalogs available
through the GSSS STScI web services at GSSSCATALOGS.
The combined source catalog derived in the first step then gets cross-matched and fit to this astrometric reference catalog. The pipeline initially supports fitting to the GAIADR2 catalog, with the option to select the GAIADR1 instead. The results of this one fit then gets back-propogated to all the input images to align them all to the astrometric reference frame while maintaining the relative alignment between the images.
The linear coordinate transformation computed in the previous step
is used to define tangent-plane corrections that need to be applied
to the GWCS pipeline in order to correct input image WCS.
This correction is implemented by inserting a
v2v3corr frame with
tangent plane corrections into the GWCS pipeline of the image’s WCS.
tweakreg step has the following optional arguments:
Source finding parameters:
save_catalogs: A boolean indicating whether or not the catalogs should be written out. (Default=`False`)
strindicating catalog output file format. (Default=’ecsv’)
floatvalue indicating the Gaussian kernel FWHM in pixels. (Default=2.5)
floatvalue indicating SNR threshold above the background. (Default=5.0)
brightest: A positive
intvalue indicating the number of brightest objects to keep. (Default=100)
floatvalue used to filter out objects with pixel values >=
Optimize alignment order:
enforce_user_order: a boolean value indicating whether or not take the first image as a reference image and then align the rest of the images to that reference image in the order in which input images have been provided or to optimize order in which images are aligned. (Default=`False`)
Reference Catalog parameters:
expand_refcat: A boolean indicating whether or not to expand reference catalog with new sources from other input images that have been already aligned to the reference image. (Default=False)
Object matching parameters:
minobj: A positive
intindicating minimum number of objects acceptable for matching. (Default=15)
floatindicating the search radius in arcsec for a match. (Default=1.0)
use2dhist: A boolean indicating whether to use 2D histogram to find initial offset. (Default=True)
separation: Minimum object separation in arcsec. (Default=0.5)
tolerance: Matching tolerance for
xyxymatchin arcsec. (Default=1.0)
xoffset: Initial guess for X offset in arcsec. (Default=0.0)
yoffset: Initial guess for Y offset in arcsec. (Default=0.0)
Catalog fitting parameters:
strvalue indicating the type of affine transformation to be considered when fitting catalogs. Allowed values:
'shift': x/y shifts only
'rscale': rotation and scale
'rshift': rotation and shifts
'general': shift, rotation, and scale (Default=”general”)
nclip: A non-negative integer number of clipping iterations to use in the fit. (Default = 3)
sigma: A positive
floatindicating the clipping limit, in sigma units, used when performing fit. (Default=3.0)
Astrometric fitting parameters:
align_to_gaia: A boolean indicating whether or not to fit to perform the fit to an astrometric catalog. (Default=False)
gaia_catalog: String indicating what astrometric catalog should be used. Initially supported options: ‘GAIADR2’ and ‘GAIADR1’. (Default=’GAIADR2’)
min_gaia: Minimum number of matches to astrometric sources to initiate a fit. (Default=5)
save_gaia_catalog: A boolean specifying whether or not to write out the astrometric catalog used for the fit as a separate product. (Default=False)
This step does not require any reference files.