Thomas Robitaille
Thomas Robitaille
Similar to my suggestion in #85, I think we should make it so that ``load_fits_data`` returns some kind of Image object on which we can set the current slice for...
We should make it so that the central position of the view is a trait, as this will ensure that the current target will be preserved when splitting the output...
We need a way to provide a table with 3D coordinates/parameters for an orbit or trajectory and have those show up in WWT.
I'm not sure yet how one does this within WorldWideTelescope, but we need to have a way for users to provide e.g. FITS files or RGB images with AVM meta-data...
This is a little bit more advanced, but down the road, if a javascript command fails, we should pass this back to Python so that a proper exception can be...
Filters have to be ordered by increasing frequency, but we should explicitly check this.