At the edge of source confusion in optical astronomy with new ultra-deep imaging surveys
The deepest ground-based optical surveys (in terms of surface brightness mu~31 mag/arcsec^2) show that we are close to the dreaded source confusion limit. The typical distance between sources in these images is a few arcseconds, on the order of the natural seeing in these images. When this source confusion limit is reached, low surface brightness
Hosseini Shahisavandi, Seyedeh Zahra et al.
Advertised on:
7
2024