A Dataset Designed to Train and Test Very Long Baseline Interferometry Image Reconstruction Algorithms
Challenge Number | Source Location | Telescopes | Total Flux (Janskys) | Suggested FOV (arcseconds) | Noise Property |
1 | Sgr A* | SMA, SMT, LMT, ALMA, PV, PDB, SPT | 2 | 0.000200 | Thermal & Atmospheric |