Open keflavich opened 2 years ago
from Qizhou: "MAPS paper: https://ui.adsabs.harvard.edu/abs/2021ApJS..257....2C/abstract Original paper: https://ui.adsabs.harvard.edu/abs/1995AJ....110.2037J/abstract Extragalactic paper commenting on these corrections: https://ui.adsabs.harvard.edu/abs/2008AJ....136.2563W/abstract"
Another implementation from tp2vis, by comparing fluxes in clean/dirty images, which is a different strategy than that in the MAPS paper. But it requires a dirty image to be available: https://github.com/tp2vis/distribute/blob/master/tp2vis.py#L1106
We need diagnostic figures like these:
as done here: https://github.com/ALMA-IMF/reduction/blob/master/analysis/psf_check_figures.py https://github.com/ALMA-IMF/reduction/blob/master/analysis/imstats.py