The coaddition pipeline is similar to the top-level pipeline.
It can be initialized from the config file or using overrides from kwargs.
It then accepts either a list of images or a time range (with both start and end date optional, we can set reasonable defaults for them) + a filter, section ID and coordinates (or target).
If using time range/filter/coordinates it will look for all the images within that range and pull them up to make the coadd.
The pipeline will output a coadded image that has source extraction, PSF extraction, astro/photo calibration all done on it.
It can then be saved either as a combined science image (e.g., nightly/weekly science coadds) or as a reference image.
The coaddition pipeline is similar to the top-level pipeline. It can be initialized from the config file or using overrides from
kwargs
. It then accepts either a list of images or a time range (with both start and end date optional, we can set reasonable defaults for them) + a filter, section ID and coordinates (or target). If using time range/filter/coordinates it will look for all the images within that range and pull them up to make the coadd.The pipeline will output a coadded image that has source extraction, PSF extraction, astro/photo calibration all done on it.
It can then be saved either as a combined science image (e.g., nightly/weekly science coadds) or as a reference image.