Dear colleagues,
Aperture magnitudes are calculated in circular apertures, whereas galaxies often appear elongated on the sky (due to the presence of a disk for the vast majority, which can be seen with various inclinations).
Being able to calculate apertude magnitudes in elliptical apertures, defined either by the isophotal elongation, or better, with a predefined elongation per source would be a significant plus.
Thanks a lot in advance for your opinion on such a feature.
Best regards