This is straight forward for Roman and JWST data since we know where they are located. But in general, other users of ASDF data may use different conventions so an elaboration of this is allowing users to provide their own means of defining where the default image will be located.
This is straight forward for Roman and JWST data since we know where they are located. But in general, other users of ASDF data may use different conventions so an elaboration of this is allowing users to provide their own means of defining where the default image will be located.